ViaSat AMSS Reply Comments

0048-EX-PL-2007 Text Documents

ViaSat, Inc.

2007-07-18ELS_82613

                                                                     ViaSat, Inc. Reply Comments
                                                                              IB Docket No. 05-20
                                                                             Filed August 3, 2005

                                         Before the
                         FEDERAL COMMUNICATIONS COMMISSION
                               Washington, D.C. 20554


In the Matter of                             )
                                             )
Service Rules and Procedures to Govern the )
Use of Aeronautical Mobile Satellite Service )   IB Docket No. 05-20
Earth Stations in Frequency Bands Allocated )
to the Fixed Satellite Service               )
                                             )




                            REPLY COMMENTS OF VIASAT, INC.




                                                 John P. Janka
                                                 Teresa D. Baer
                                                 Elizabeth R. Park
                                                 LATHAM & WATKINS LLP
                                                 555 Eleventh St., N.W., Suite 1000
                                                 Washington, D.C. 20004
                                                 202-637-2200

                                                 Counsel for ViaSat, Inc.




August 3, 2005




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                                                                                                         ViaSat, Inc. Reply Comments
                                                                                                                  IB Docket No. 05-20
                                                                                                                 Filed August 3, 2005

                                                 TABLE OF CONTENTS

I.      Introduction and Summary ..................................................................................................1

II.     AMSS Spectrum Allocation ................................................................................................4

        A.         AMSS Should Be Treated as Co-Primary With FSS...............................................4
        B.         ViaSat Supports AMSS Operations in the Extended Ku-Band On The
                   Same Basis As FSS..................................................................................................6
        C.         Coordination With RAS and TDRSS Should Be Required Only In The
                   Bands In Which Those Services Operate.................................................................8

III.    AMSS Service Rules............................................................................................................9

        A.         AMSS Service Rules Should Be Consistent With VSAT Service Rules But
                   Should Accommodate AMSS Technology..............................................................9
        B.         Antenna Pointing Errors Do Not Cause Harmful Interference Into
                   Adjacent Satellites .................................................................................................11
        C.         The Contention Table Would Account For Multiple Factors That Cause
                   AMSS Networks to Exceed Off-Axis EIRP Density Limits .................................13
        D.         AMSS Operators Have Proven That An Aggregate Network Power
                   Density Limit Is Feasible .......................................................................................14
        E.         The Commission Should Allow Coordination With Satellite Operators For
                   Higher Power Operations.......................................................................................16

IV.     The Commission Should Address The Issues Raised By Law Enforcement
        Agencies In A Separate Proceeding...................................................................................17

V.      The Commission Should Not Require Operators To Submit Tracking Data Into A
        Publicly Accessible Database ............................................................................................19

VI.     Licensing Issues .................................................................................................................21

        A.         Technical Showings ...............................................................................................21
        B.         ALSAT Designation ..............................................................................................22

VII.    Conclusion .........................................................................................................................23




DC\778232.4


                                                                                 ViaSat, Inc. Reply Comments
                                                                                          IB Docket No. 05-20
                                                                                         Filed August 3, 2005



                                           Before the
                               FEDERAL COMMUNICATIONS COMMISSION
                                     Washington, D.C. 20554


In the Matter of                             )
                                             )
Service Rules and Procedures to Govern the )
Use of Aeronautical Mobile Satellite Service )             IB Docket No. 05-20
Earth Stations in Frequency Bands Allocated )
to the Fixed Satellite Service               )
                                             )

                                   REPLY COMMENTS OF VIASAT, INC.

                  ViaSat, Inc. (“ViaSat”) replies to the comments filed in response to the Notice of

Proposed Rulemaking (“NPRM”) regarding the implementation of service rules and licensing

procedures for the aeronautical mobile satellite service (“AMSS”) in the Fixed Satellite

Service (“FSS”) bands.1

I.        INTRODUCTION AND SUMMARY

                  ViaSat and other AMSS system operators commenting in this proceeding have

developed and implemented new technology that allows broadband services to be provided on

board aircraft using the frequency bands currently used for FSS. AMSS technology promises to

facilitate a number of important public policy goals articulated in the Commission’s recently-

released Strategic Plan: (i) providing more competitive choices for U.S. consumers, (ii)

facilitating the ubiquitous deployment of broadband services, (iii) using spectrum more




1
    See Comments of ViaSat, Inc., Service Rules and Procedures to Govern the Use of Aeronautical Mobile
    Satellite Service Earth Stations in Frequency Bands Allocated to the Fixed Satellite Service, IB Docket
    No. 05-20 (filed July 5, 2005) (“ViaSat Comments”).


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                                                                                    ViaSat, Inc. Reply Comments
                                                                                             IB Docket No. 05-20
                                                                                            Filed August 3, 2005

efficiently and effectively, and (iv) fostering investment and innovation in broadband

technologies and services.2

                   ViaSat’s AMSS system couples spread spectrum technology with dynamic power

management over the entire AMSS network in order to direct system capacity where and when it

is needed to serve user demands, and to reduce the potential for interference into other systems.

The full benefits of this technology can be achieved, however, only if the Commission adopts a

regulatory regime that is flexible enough to allow greater shared use of the FSS frequency bands.

As several commenters have shown, adopting rules based on existing FSS rules, which were

designed for now decades-old technologies, would constrain the development of the technology

implemented in AMSS systems.3 Without citing a single incident of interference from AMSS in

FSS bands, certain parties in this proceeding urge the Commission to impose on AMSS the same

rules that constrain VSAT development in the FSS today.4 Fortunately, the Commission has

recently rejected a number of those arguments in its Earth Station Licensing Sixth Report and

Order.5

                   More fundamentally, the Commission has recently recognized, as ViaSat has

urged, that more efficient uses of spectrum can be facilitated by “enlightened” regulatory

approaches that do not specify the use of certain system designs or technologies. In the context

of allowing mobile satellite service (“MSS”) providers to implement an ancillary terrestrial


2
    See Public Notice, Public Invited to Review Draft Strategic Plan (rel. Jul. 5, 2005).
3
    See ARINC Comments at 11; Boeing Comments at 27; SES Americom Comment at 2-3.
4
    PanAmSat Comments at 3; Intelsat Comments at 3.
5
    2000 Biennial Regulatory Review – Streamlining and Other Revisions of Part 25 of the Commission’s
    Rules Governing the Licensing of, and Spectrum Usage by, Satellite Network Earth Stations and Space
    Stations, IB Docket No. 00-248, Sixth Report and Order and Third Further Notice of Proposed
    Rulemaking, FCC 05-62 at ¶ 119 (rel. Mar. 15, 2005) (“Earth Station Licensing Sixth Report and
    Order”).

                                                        2
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                                                                             ViaSat, Inc. Reply Comments
                                                                                      IB Docket No. 05-20
                                                                                     Filed August 3, 2005

component (“ATC”), the Commission established appropriate aggregate interference limits, but

provided the ATC operator great latitude to choose the operational parameters and technology

necessary to comply with those limits.6 The comments in this proceeding amply support such an

“enlightened” approach to regulation of AMSS.

                  ViaSat and the other AMSS interests commenting in this proceeding set forth very

similar proposals regarding the service rules and licensing of AMSS. All agree that the

Commission should afford aeronautical earth station (“AES”) terminals in an AMSS network the

same regulatory status and treatment as VSAT terminals in an FSS network.7 AMSS operators

are able to control the power density of aeronautical terminals on an aggregate basis and thus,

can limit off-axis power density into adjacent satellites to levels that are comparable to that of

VSATs. From the perspective of adjacent satellites, AES terminals do not present any greater

interference potential than a typical VSAT network. Existing AMSS systems have proven that

AMSS operations can successfully operate in FSS bands without causing harmful interference.

Therefore, there is no need for the Commission to limit AMSS technology in the manner that

PanAmSat and Intelsat advocate.8 To the contrary, their proposals would constrain the spectrum

efficiency and the scope of broadband service that AMSS use of FSS bands promises.

                  Finally, the Department of Justice, including the Federal Bureau of Investigation,

and the Department of Homeland Security (collectively, the “Departments”) raise issues that




6
    See Flexibility for Delivery of Communications by Mobile Satellite Service Providers in the 2 GHz
    Band, the L-Band, and the 1.6/2/4 GHz Bands, IB Docket No. 01-185, Memorandum Opinion and Order
    and Second Order on Reconsideration, FCC 05-30 at ¶¶ 47, 50 (rel. Feb. 25, 2005) (“ATC Second Order
    on Reconsideration”).
7
    ARINC Comments at 5, 24; Boeing Comments at 15.
8
    PanAmSat Comments at 3; Intelsat Comments at 3.

                                                    3
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                                                                         ViaSat, Inc. Reply Comments
                                                                                  IB Docket No. 05-20
                                                                                 Filed August 3, 2005

warrant careful review by the Commission. Given the complexity of the issues and the need for

a full record, the Commission should commence a separate proceeding to address these issues.

II.       AMSS SPECTRUM ALLOCATION

          A.      AMSS Should Be Treated as Co-Primary With FSS

                  AMSS uplinks and downlinks in the Ku-band should be treated as co-primary

with FSS, consistent with the Commission’s proposed footnote in the NPRM. The comments

submitted in this proceeding support ViaSat’s arguments that AMSS systems are no more

interfering, and no more susceptible to interference than, an FSS system due to the spread

spectrum multiple access and dynamic power control technologies employed by AMSS systems.

Therefore, the Commission should adopt the co-primary AMSS footnote, but should revise its

proposed language, as indicated below, to recognize that the technology AMSS systems employ

may be different than that used in traditional VSATs.

                  Boeing supports ViaSat’s position that AMSS systems can operate such that they

are no more interfering than an FSS system.9 ViaSat appreciates the need to protect FSS; ViaSat

itself operates FSS VSAT networks, and would not support proposals for AMSS systems that do

not protect FSS. However, existing AMSS systems have already demonstrated that operators

can control the total level of aggregate power in the network such that the power density towards

adjacent satellites is within the prescribed limits. Boeing and SES Americom have experienced

first hand the ability of AMSS networks to operate without causing harmful interference into

adjacent satellites.10 Since 2001, Boeing has successfully managed network power in its

Connexion AMSS system, demonstrating that AMSS systems and FSS operations can coexist in



9
    Boeing Comments at 7, 9.
10
     Id. at 10; SES Comments at 2.

                                                 4
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                                                                          ViaSat, Inc. Reply Comments
                                                                                   IB Docket No. 05-20
                                                                                  Filed August 3, 2005

the Ku-band without incidents of harmful interference into FSS operations. SES Americom,

which provides capacity to both FSS and AES system operators, indicates that AES terminals

can be deployed without creating harmful interference into other FSS applications.11

                 Boeing’s experience operating AMSS networks demonstrates that Telesat Canada

and PanAmSat’s doubts regarding the ability of systems to control aggregate EIRP are

unfounded.12 AMSS networks, such as ViaSat’s system, clearly can manage off-axis EIRP

density on an aggregate basis to prevent harmful interference into adjacent satellites. ViaSat has

worked with FSS satellite operators, including SES Americom, to test the aggregate power

control of its AMSS system, with successful results. Without citing a single incident of

interference by AMSS networks, PanAmSat asserts that the mobile nature of AMSS creates a

higher potential for creating interference and is more susceptible to receiving interference.13 As

discussed in more detail below, the antenna pointing variability associated with mobile antennas

does not significantly increase the interference potential because each antenna in an AMSS

network using spread spectrum emits at extremely low power density levels.

                 In its comments, Boeing has changed its position on priority for Ku-band AMSS

downlinks and now agrees with ViaSat that the Commission should afford protection to AMSS

downlink operations.14 As a policy matter, co-primary treatment of AMSS is necessary to create

an environment where broadband services on aircraft may proliferate. Co-primary status would

provide the level of certainty required to encourage investors and the market to promote AMSS

technology. Just like earth stations on vessels (“ESVs”), which have co-primary status with FSS,


11
     SES Comments at 2.
12
     Boeing Comments at 10.
13
     PanAmSat Comments at 2.
14
     Boeing Comments at 7.

                                                 5
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                                                                           ViaSat, Inc. Reply Comments
                                                                                    IB Docket No. 05-20
                                                                                   Filed August 3, 2005

AES terminals would use existing FSS infrastructure to provide broadband service. AMSS is

essentially another application of FSS, and thus, should be treated as co-primary with FSS.

Therefore, Section 25.209(c) should apply equally to AMSS, such that an AES terminal is

protected from interference to the extent the terminal is no more susceptible to harmful

interference than a conforming earth station antenna.

                 ViaSat endorses Boeing’s request that the Commission adopt its proposal in the

NPRM to add a non-Federal government footnote to the U.S. Table of Frequency Allocations

affording AMSS protection as a co-primary service in the Ku-band uplink and downlink

frequencies.15 However, the Commission should revise its proposed footnote to reflect the fact

that AES terminals may use different technologies than traditional VSATs, and thus, may not

necessarily operate under the “same parameters” as VSATs. The language of the footnote

should be as follows:

                 NGyy In the bands 11.7-12.2 GHz (space-to-Earth) and 14.0-14.5 GHz (Earth-to-
                 space), aircraft earth stations in the aeronautical mobile-satellite service are an
                 application of the Fixed Satellite Service (FSS). The provision of the ITU Radio
                 Regulations Nos. 5.29, 5.30 and 5.31 apply, except that reception from
                 geostationary space stations in the fixed-satellite service in the 11.7-12.2 GHz
                 shall be protected on a primary basis, to the extent provided that aircraft earth
                 stations are no more susceptible to interference than operate under the same
                 parameters as earth stations in the fixed-satellite service.

          B.     ViaSat Supports AMSS Operations in the Extended Ku-Band On The Same
                 Basis As FSS

                 In their respective comments, ARINC and Boeing both urge the Commission to

permit AMSS operations in the 10.95-11.2 and 11.45-11.7 GHz bands.16 ViaSat agrees that the

Commission should afford AMSS the same regulatory status as FSS in the Ku-band, as well as in



15
     See NPRM at ¶ 31.
16
     ARINC Comments at 25; Boeing Comments at 8.

                                                   6
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                                                                                 ViaSat, Inc. Reply Comments
                                                                                          IB Docket No. 05-20
                                                                                         Filed August 3, 2005

the extended Ku-band.17 The U.S. Table of Frequency Allocations currently includes a footnote

that allows FSS downlinks in the extended Ku-bands on a co-primary basis with fixed services

(“FS”) only when the FSS uplink originates outside the U.S.18 The Commission adopted this

allocation to limit the number of FSS networks with which FS providers would need to

coordinate. However, the Commission has granted waivers to applicants requesting use of the

extended Ku-band for domestic FSS on an unprotected, non-interference basis.19 In those cases,

the Commission determined that such use on an unprotected, non-interference basis would not

require FS providers to coordinate with domestic FSS and thus, would not undermine the

purpose of the rule.

                   AMSS should be treated as an application of the FSS, as the Commission

proposes in the NPRM. As such, the Commission should allow AES terminals to operate in the

extended Ku-bands on a co-primary basis with the FS where the uplink originates outside of the

U.S., and on a non-interference basis vis-à-vis the FS where the uplink originates domestically.

ViaSat agrees with Boeing and ARINC that permitting AMSS operations in these bands would

allow seamless broadband service to passengers on U.S. registered aircraft flying over

international territories.20 Due to the international nature of many aeronautical routes, the

Commission should afford AMSS operators the flexibility to operate throughout internationally

allocated Ku-band FSS spectrum.21



17
     Boeing Comments at 9.
18
     47 C.F.R. § 2.106 n. NG104.
19
     See, e.g., EchoStar KuX Corporation Application for Authority to Construct, Launch and Operate a
     Geostationary Satellite Using the Extended Ku-band Frequencies in the Fixed-Satellite Service at the
     121 W.L., Orbital Location, Order and Authorization, DA 04-3164 at ¶ 13 (rel. Sept. 30, 2004).
20
     Boeing Comments at 8; ARINC Comments at 25.
21
     ARINC Comments at 25.

                                                       7
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                                                                            ViaSat, Inc. Reply Comments
                                                                                     IB Docket No. 05-20
                                                                                    Filed August 3, 2005

           C.    Coordination With RAS and TDRSS Should Be Required Only In The Bands
                 In Which Those Services Operate

                 The National Radio Astronomy Observatory (“NRAO”) asserts in its comments

that imposing coordination requirements below 14.47 GHz is unnecessary to protect Radio

Astronomy Services (“RAS”) in the 14.47-14.5 GHz band.22 NRAO cites as evidence the

memoranda of understanding between National Science Foundation, and ARINC and Boeing,

respectively, which include a requirement to incorporate “’proper’ hardware design” into their

networks, as provided in ITU-R M. 1643, Part C.23 ViaSat agrees that the incorporation of this

ITU regulation as a license condition is appropriate, and NRAO’s comments confirm that

compliance with this regulation is sufficient to prevent AMSS operations below 14.47 GHz from

interfering with RAS in the 14.47-14.5 GHz band.

                 Adopting this ITU regulation as a license condition would make moot National

Academy of Sciences’ (“NAS”) proposal that the Commission require AMSS to coordinate with

RAS in the entire 14.0-14.5 GHz band in order to afford NAS “optimal” protection.24 NAS

indicates in its comments that limiting coordination to the 14.47-14.5 GHz band would be

“acceptable” if systems comply with ITU-R M. 1643. Thus, the Commission should make clear

that as long as the requirements of ITU-R M. 1643 are met, coordination requirements with

research facilities are limited to the narrow bands used by those facilities.




22
     National Radio Astronomy Observatory Comments at 2.
23
     Id. at 3.
24
     National Academy of Sciences’ Committee on Radio Frequencies Comments at 6.

                                                  8
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                                                                            ViaSat, Inc. Reply Comments
                                                                                     IB Docket No. 05-20
                                                                                    Filed August 3, 2005

III.       AMSS SERVICE RULES

           A.       AMSS Service Rules Should Be Consistent With VSAT Service Rules But
                    Should Accommodate AMSS Technology

                    In its comments, Boeing notes that “certain elements of the Commission’s

proposed approach do not appear to be consistent with . . . recent Commission actions adopting

analogous ESV rules and addressing other station licensing reforms.”25 ViaSat agrees that the

Commission should adopt service rules and licensing procedures for AMSS that are comparable

to the requirements for VSATs in FSS as currently proposed in the Earth Station Licensing Sixth

Report and Order.26 As discussed above, AMSS should be treated as an application of FSS, and

thus, should be subject to the same regulatory approaches.

                    In the pending Earth Station Licensing Sixth Report and Order, the Commission

proposes to adopt an off-axis power density limit to allow VSAT operators to employ a “power-

pattern” trade off, and thereby use smaller antennas that do not meet the Section 25.209 antenna

mask. This approach recognizes that small antennas can operate without causing harmful

interference into adjacent satellites by reducing transmit power levels to compensate for the

amount by which the antenna gain pattern exceeds the Section 25.209 requirements.27

                    Developing regulations for all Ku-band services based on a power-pattern trade

off would accommodate a broad range of antenna technologies that do not comply with the

Section 25.209 antenna mask. For instance, the dynamic power control technology employed by

AMSS systems expands the potential of networks using FSS satellites by increasing spectrum

use efficiency. As the Commission recognized in the case of VSATs, network operators can


25
     Boeing Comments at 15.
26
     See, generally, Earth Station Licensing Sixth Report and Order.
27
     Id. at ¶ 74.

                                                      9
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                                                                              ViaSat, Inc. Reply Comments
                                                                                       IB Docket No. 05-20
                                                                                      Filed August 3, 2005

reduce the overall power into a VSAT to compensate for a non-compliant pattern. In AMSS

networks, network operators can adjust the power of hundreds or thousands of antennas

simultaneously operating on a co-channel basis, using spread spectrum techniques, such that the

aggregate power density transmitted by all antennas in the network remains below a threshold

level that the Commission deems acceptable to protect adjacent satellites from harmful

interference. This technology, which enables aeronautical terminals to use the Ku-band, readily

could be extended to “traditional” VSAT terminals to allow VSATs to use spectrum capacity

more efficiently. The innovations in spectrum-sharing technology employed by AMSS networks

make possible the use of smaller antennas. The Commission recognizes the need to afford

flexibility to VSATs to use small antennas and should allow AMSS the same flexibility to

accommodate such technologies.

                  Therefore, the off-axis power density limits, contention table and coordination

requirements for higher power operations should be the same for AMSS as for FSS, as proposed

by many of the commenters in this proceeding.28 Further, the Commission should reject

proposals to adopt an antenna pointing accuracy requirement for AMSS, as it did for VSATs.29

SES Americom supports consistent regulatory treatment of AMSS and FSS in its comments,

cautioning the Commission that additional requirements should be imposed only where they are

necessary to prevent harmful interference.30 Consistent regulatory treatment of AMSS and FSS

is critical to the development of AMSS into a commercially viable, widely-available service.




28
      See, e.g., Boeing Comments at 15; ARINC Comments at 2, 24; Intelsat Comments at 3-4 (supporting
     the consistent off-axis power density limits); SES Americom Comments at 4 (supporting consistent
     treatment of coordination of higher power operations).
29
     Earth Station Licensing Sixth Report and Order at ¶ 23.
30
     SES Americom Comments at 2.

                                                      10
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                                                                          ViaSat, Inc. Reply Comments
                                                                                   IB Docket No. 05-20
                                                                                  Filed August 3, 2005

           B.     Antenna Pointing Errors Do Not Cause Harmful Interference Into Adjacent
                  Satellites

                  ViaSat, Boeing and ARINC agree that an antenna pointing accuracy requirement

is unnecessary because the off-axis EIRP density limit already accounts for pointing errors.31

The off-axis power density envelope is intended to define a level of power density for non-

compliant antenna patterns that is deemed to be “pre-coordinated” with adjacent satellites. By

adopting a “power-pattern trade off” approach, the Commission recognizes that the antenna gain

pattern of the antenna does not matter as long as the antenna does not exceed the pre-coordinated

power density levels into adjacent satellites. AMSS networks can be controlled such that the

aggregate power density of the antennas in the network does not exceed the pre-coordinated

power density levels. Because AMSS operators can control the aggregate network power density

into adjacent satellites, any variations in individual antenna performance, including mispointing,

can be alleviated by reducing the aggregate power level of all antennas in the network.

                  ViaSat agrees with ARINC’s argument that a specific pointing accuracy

requirement could limit advancement in antenna technology.32 ARINC cites as an example an

omni-directional antenna, which has no main lobe, and thus, is not compliant with the Section

25.209 antenna gain pattern.33 The Commission purpose in adopting the “power pattern

tradeoff” is to allow various antenna technologies that do not conform with Section 25.209.

Although it would not comply with Section 25.209, an omni-directional antenna could instead

comply with the off-axis EIRP density envelope to prevent harmful interference into adjacent

satellites. However, an antenna pointing accuracy requirement for an antenna with no mainbeam


31
     Boeing Comments at 27; ARINC Comments at 12.
32
     ARINC Comments at 11.
33
     Id. at 12.

                                                 11
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                                                                                    ViaSat, Inc. Reply Comments
                                                                                             IB Docket No. 05-20
                                                                                            Filed August 3, 2005

is meaningless because the beam radiates in all directions. ViaSat agrees with ARINC that

pointing accuracy must be a function of antenna power and beamwidth, which is more

effectively addressed through the aggregate off-axis EIRP.

                    Likewise, AES terminals using spread spectrum technology have non-compliant

antenna patterns and wide beamwidths. Pointing errors by these terminals, however, do not

significantly increase interference into adjacent satellites. In AMSS networks that employ

spread spectrum multiple access techniques, individual AES terminals are characterized by wide

beamwidths with extremely low power density. Because the power density level of any given

antenna in such an aeronautical network is so low, any individual antenna that is “mispointed” is

unlikely to be noticeable to an adjacent satellite. Indeed, because the main lobe of the antenna is

so wide, even when the antenna is accurately pointed, some portion of the mainbeam will spill

over in the direction of an adjacent satellite.34

                    Even assuming the deployment of a large number of AES terminals, the

likelihood of a number of AES terminals all mispointing into the same satellite is miniscule due

to the random nature of antenna pointing errors.35 ViaSat has prepared a Technical Summary of

Pointing Error Effects, attached hereto as Exhibit A, which describes the simulated effect of AES

terminal pointing errors. The simulation assumes a network of 100 AES terminals, using spread

spectrum multiple access techniques, in which off-axis power density is controlled on an

34
      The Satellite Industry Association (“SIA”) recently filed a Petition for Reconsideration in the Earth
     Station Licensing Sixth Report and Order arguing that smaller earth station antennas are prone to larger
     pointing errors than those of larger antennas. While this might be the case for VSATs, it is not relevant
     to AES terminals. AES terminals operate in a dynamic environment, and antenna orientation is
     continually adjusted to point accurately at the antenna’s point of communication. Therefore, these
     terminals do not face the same factors that cause VSAT antennas to be mispointed in a static
     environment, such as installation errors, wind and other environmental factors.
35
      The random nature of mispointing also means that an antenna may be as likely pointed away from an
     adjacent satellite as towards it, thereby balancing the aggregate power into that satellite at any given
     time.

                                                        12
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                                                                          ViaSat, Inc. Reply Comments
                                                                                   IB Docket No. 05-20
                                                                                  Filed August 3, 2005

aggregate basis. This analysis demonstrates that, even assuming mispointing angles of 5° to 10°,

the network aggregate off-axis antenna gain profile would exceed the Section 25.209 mask by

relatively small amounts. For instance, assuming that the AES terminals are mispointed by less

than 10° 99.7% of the time, the network aggregate EIRP would need to be reduced by 1.35 dB in

order to comply with the mask. Due to the ability of currently existing AMSS networks to

control aggregate power density at any given time, the AMSS operator can reduce the aggregate

power density to account for any increases in off-axis power density resulting from mispointed

antennas.

          C.     The Contention Table Would Account For Multiple Factors That Cause
                 AMSS Networks to Exceed Off-Axis EIRP Density Limits

                 ViaSat, Boeing and ARINC each propose that the Commission adopt for AMSS

the exceedance table proposed for VSATs in the Earth Station Licensing Sixth Report and

Order.36 All agree that while AMSS systems are designed to adjust aggregate power levels to

take into account statistical variations in the off-axis EIRP density, the Commission should make

its rules clear that such variations are anticipated and permitted.37 The off-axis EIRP density

emitted by AES terminals will vary over time from the perspective of an adjacent satellite due to

the short bursts of power resulting from the use of contention protocols, as the Commission

recognized in the context of VSATs. However, variations in off-axis EIRP density from AES

terminals can also result from pointing factors and adjustments in the aggregate power of the

network. Therefore, in AMSS networks, the contention table would provide added flexibility to

trade off all of these factors.




36
     Boeing Comments at 18; ARINC Comments at 24.
37
     Boeing Comments at 19.

                                                13
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                                                                           ViaSat, Inc. Reply Comments
                                                                                    IB Docket No. 05-20
                                                                                   Filed August 3, 2005

                  ViaSat agrees with Boeing’s argument that the contention exceedance table would

appropriately provide AMSS operators a margin for error to account for mispointing.38 While

the Commission proposed the table in the VSAT context only to deal with multiple access

techniques, the contention table would also allow flexibility for AMSS networks to exceed the

limits for short periods as a result of other factors, such as antenna pointing and lags in dynamic

power control. Just like increases in the network aggregate power density due to the use of

contention protocols, increases in off-axis power toward an adjacent satellite due to antenna

mispointing are likely to last only for very short periods. Because AES terminals are in motion

and because the dynamic power control mechanism constantly adjusts the power into individual

antennas, any exceedance of the off-axis EIRP density limits would not last long and could be

adequately captured by the exceedance allowances in the contention table.

           D.     AMSS Operators Have Proven That An Aggregate Network Power Density
                  Limit Is Feasible

                  The comments in the record support the ability of AMSS networks to meet the

off-axis EIRP density limits on an aggregate basis.39 An aggregate limit would provide AMSS

operators the most flexibility to use any technology that is capable of meeting the off-axis power

density mask, thereby promoting new technologies and encouraging the deployment of new

broadband services. ViaSat urges the Commission to recognize, as it did in the context of ATCs

in MSS bands, that an aggregate limit would facilitate more efficient uses of spectrum.40 In

order to promote new and improved services and greater spectrum efficiency, the Commission

authorized terrestrial use of the MSS spectrum in the L-band, on a secondary basis. In that


38
     Id. at 19.
39
     ARINC Comments at 2; SES Americom Comments at 4.
40
     ATC Second Order on Reconsideration at ¶ 47.

                                                    14
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                                                                         ViaSat, Inc. Reply Comments
                                                                                  IB Docket No. 05-20
                                                                                 Filed August 3, 2005

proceeding, the Commission adopted an aggregate limit on the amount of interference that a

network of ATC terminals is permitted to generate, on a co-frequency basis, into MSS

operations.

               Significantly, the Commission did not require ATC operators to use any specific

technology to meet these limits, and instead allowed operators to meet the limits in accordance

with their own designs and business plans. The Commission applied this “enlightened”

regulatory approach to afford network operators broad discretion to design ATC systems in any

manner that would not exceed the aggregate noise level, and thus, did not require specific

technology or constraints. In that case, the Commission determined that an aggregate limit was

appropriate even though, at the time, there were no ATC technologies that were proven to

operate at such limits and without causing interference to MSS operations.

               The Commission should adopt the same enlightened regulatory approach for

AMSS as it did for ATCs. Indeed, there is no reason to adopt a different approach for AMSS.

Adoption of an aggregate off-axis EIRP density limit for AMSS should be even less

controversial than in the ATC context because AMSS providers have demonstrated that AMSS

systems can operate within prescribed limits and in a manner that avoids harmful interference to

incumbent services. Dynamic power control technology is proven technology that allows AMSS

networks to comply with the same off-axis EIRP density limits as VSATs. As discussed above,

ViaSat, Boeing and SES Americom have experience with the actual operation of such networks,

demonstrating that the technology works. Thus, the doubts that Telesat Canada and PanAmSat




                                               15
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                                                                           ViaSat, Inc. Reply Comments
                                                                                    IB Docket No. 05-20
                                                                                   Filed August 3, 2005

express regarding AMSS operators’ ability to control aggregate network power and to ensure

protection of adjacent satellites are unsubstantiated.41

                  Further, PanAmSat’s proposals to adopt an antenna pointing accuracy

requirement run counter to the approach that the Commission has taken in the ATC proceeding.42

Such a requirement would impose design limitations on AMSS antenna technology. As

discussed above, an antenna pointing requirement is unnecessary to protect adjacent satellites

from harmful interference and would only serve to hinder the development of AMSS technology.

          E.      The Commission Should Allow Coordination With Satellite Operators For
                  Higher Power Operations

                  ViaSat supports proposals to permit AMSS networks to operate at a higher power

density than the off-axis EIRP density limits, subject to coordination with adjacent satellite

operators. Like VSAT operators, AMSS operators should have the flexibility to coordinate with

adjacent satellite operators any transmissions in excess of the off-axis EIRP density limits set

forth in the Commission’s rules.43 VSAT operators and satellite operators routinely coordinate

such higher power operations. Coordination among AMSS operators and satellite operators

would proceed in the same manner. Intelsat and SES Americom both support this approach. As

Intelsat notes, operator-to-operator coordination agreements are the “norm” and thus,

certification by satellite operators and AES licensees should satisfy the Commission in licensing

such AMSS networks.44




41
     Telesat Canada Comments at 3; PanAmSat Comments at 2.
42
     PanAmSat Comments at 3.
43
     Boeing Comments at 23.
44
     Intelsat Comments at 5; see also, SES Americom Comments at 4.

                                                   16
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                                                                                ViaSat, Inc. Reply Comments
                                                                                         IB Docket No. 05-20
                                                                                        Filed August 3, 2005

                   Coordinating operations at levels higher than off-axis power density limits is

particularly important for AMSS networks because foreign systems often operate at higher

routine power levels than U.S. systems.45 AES terminals are likely to communicate with non-

U.S. networks during international flights. Thus, U.S. AMSS operators should be permitted to

operate with satellites outside of U.S. airspace so that they may compete effectively with foreign

operators. Imposing a strict requirement that AMSS networks operate within the off-axis EIRP

density limits, even where adjacent satellite operators agree that they would not be harmed, could

severely limit the ability of AMSS licensees to operate in foreign jurisdictions, thereby

constraining development of AMSS by U.S. operators. By allowing coordination of higher

power AMSS operations in the Ku-band, the Commission can “preserve operational flexibility

for AMSS licensees while fully protecting the interests of potentially affected parties.”46

IV.        THE COMMISSION SHOULD ADDRESS THE ISSUES RAISED BY LAW
           ENFORCEMENT AGENCIES IN A SEPARATE PROCEEDING

                   The Departments propose that AMSS systems meet certain design requirements

and technical capabilities to address the public safety and national security concerns.47 ViaSat

agrees that law enforcement must have the tools it needs to protect our country, and ViaSat is

prepared to do its part to assist in that important effort. In the NPRM, the Commission notes that

AMSS operators may be subject to any rules adopted in the Commission’s currently pending

proceeding on the applicability of CALEA requirements to broadband services, including




45
     Boeing Comments at 24.
46
     Id. at 24.
47
     See Comments of the Department of Justice, Including the Federal Bureau of Investigation, and the
     Department of Homeland Security (“DOJ Comments”).

                                                     17
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                                                                               ViaSat, Inc. Reply Comments
                                                                                        IB Docket No. 05-20
                                                                                       Filed August 3, 2005

services provided via satellite.48 Therefore, to the extent that the Departments’ comments

address issues relating to CALEA, those concerns are addressed in that proceeding.

                   The Departments’ comments also address the need for AMSS operational

capabilities that go beyond the scope of CALEA. Some of the capabilities that the Departments

propose, however, have not yet been developed, and others may be technologically infeasible or

prohibitively expensive. The Commission should review these proposals carefully to identify the

capabilities that should be implemented and to determine a reasonable transition period for

AMSS operators to implement those the Commission decides are appropriate. Given the

complexity of the Departments’ proposals, and the difficult policy questions some of the

proposals raise, the Commission should ensure that it reviews those proposals on a fully

developed record.

                   The Departments submitted comments with substantially similar proposals in the

Commission’s proceeding to implement rules that would allow the use of cellular telephone and

wireless devices on board aircraft.49 This proceeding currently is open, with reply comments due

in August 2005. While the “pico cell” technology for cellular communications on board aircraft

employs different technology than aeronautical satellite antennas, the concerns of the law

enforcement agencies with respect to these services appear to be similar to those relating to

AMSS. Any policies that the Commission adopts for law enforcement access to aeronautical




48
     See NPRM at n. 7; Communications Assistance for Law Enforcement Act and Broadband Access and
     Services, ET Docket No. 04-295, RM-10865, Notice of Proposed Rulemaking and Declaratory Ruling,
     FCC 04-187 at ¶ 37 (rel. Aug. 9, 2004).
49
     See Amendment of the Commission’s Rules to Facilitate the Use of Cellular Telephones and Other
     Wireless Devices Aboard Aircraft, Notice of Proposed Rulemaking, WT Docket No. 04-435, FCC 04-
     288 (rel. Feb. 15, 2005) (“Pico Cell Proceeding”); DOJ Pico Cell Proceeding Comments (filed May 26,
     2005).

                                                     18
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                                                                          ViaSat, Inc. Reply Comments
                                                                                   IB Docket No. 05-20
                                                                                  Filed August 3, 2005

communications systems should be consistent for all such systems, to the extent technically

feasible and appropriate.

                  Therefore, the Commission should institute a separate proceeding to focus on law

enforcement issues relating to aeronautical communications systems. The purpose of the AMSS

NPRM proceeding is to address technical issues relating to radio frequency interference and to

develop service rules and licensing procedures for AMSS, and thus, law enforcement issues

relating generally to aeronautical communications systems would more appropriately be

addressed separately from the issues in this NPRM.

V.         THE COMMISSION SHOULD NOT REQUIRE OPERATORS TO SUBMIT
           TRACKING DATA INTO A PUBLICLY ACCESSIBLE DATABASE

                  Although ViaSat agrees with other commenters that AMSS operators should be

required to maintain tracking data, neither the Commission nor a third party needs to maintain a

database of such data, as some suggest. In the FSS arena, earth station licensees and satellite

operators cooperate with one another to identify and resolve instances of interference. There is

no third-party tracking database interference database for FSS or for ESVs. In the context of

ESVs, the Commission determined that making real-time location information available to third

parties was unnecessary and that “the risk associated with ubiquitous distribution of such

tracking information outweighs the benefit it may provide in preventing interference to other

operations.”50 The Commission determined that the point of contact requirement and the

requirement that operators maintain tracking data for one year are sufficient to resolve

interference issues.51




50
     ESV Order at ¶ 112.
51
     Id.

                                                 19
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                                                                             ViaSat, Inc. Reply Comments
                                                                                      IB Docket No. 05-20
                                                                                     Filed August 3, 2005

                  Boeing and ARINC support this approach in their respective comments.52

Satellite operator, Telesat Canada, also notes that “[a]s in other cases of interference, the best

recourse is contact between satellite operators.”53 As ARINC points out, satellite operators have

an excellent track record in cooperating with each other to locate and eliminate interference.54

AMSS operators are able to coordinate with satellite operators through the same procedures.

ViaSat agrees that AMSS operators should maintain their own tracking data and make available

any information that is relevant to resolving specific instances of interference through a point of

contact in the U.S. However, for purposes of determining the source of interference, such

information should be provided without any information that might identify the particular aircraft

or its owners or passengers.55

                  The databases proposed by PanAmSat and the Satellite Users Interference

Reduction Group (“SUIRG”) would jeopardize the security of confidential data.56 Additionally,

the administrative burdens of maintaining a database that can be accessed by FSS operators are

unnecessary and unjustifiable. The expense and resources that a third-party database would

require would add to the cost of providing AMSS services, which could hinder deployment of

the service, without any added benefit. As noted by ViaSat, Boeing and ARINC, making real-

time AES tracking data raises security and privacy concerns, especially to business jets used by

individuals or corporations.57 AMSS services would be significantly less attractive to customers

due to the risk of security breaches that could result if satellite operators and other private

52
     Boeing Comments at 36; ARINC Comments at 17.
53
     Telesat Canada Comments at ¶ 14.
54
     ARINC Comments at 16.
55
     Id. at 17.
56
     SUIRG Comments at 2; PanAmSat at 5.
57
     Boeing Comments at 37; ARINC Comments at 17; ViaSat Comments at 22.

                                                  20
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                                                                            ViaSat, Inc. Reply Comments
                                                                                     IB Docket No. 05-20
                                                                                    Filed August 3, 2005

citizens were able to access information that could be used to monitor a person’s location and

travel destinations.

VI.       LICENSING ISSUES

          A.      Technical Showings

                  Telesat Canada supports a requirement for a technical showing from AMSS

applicants that the proposed system will not exceed the off-axis EIRP density limits.58 ViaSat

agrees that AMSS applicants should provide technical information in applications, including

non-proprietary system design information, to demonstrate that the system performance would

conform with the rules. The Commission should examine carefully any proposals to impose

informational requirements on AMSS operators to ensure that the required showings are not

burdensome and would not defeat the purpose of adopting streamlined licensing procedures.

                  Boeing proposes a specific requirement to submit a report regarding performance

verification testing of new AMSS systems prior to commencement of commercial operations.59

Boeing argues that such a requirement would not be overly burdensome given that AMSS

operators are likely to conduct such tests in any event. However, a requirement to submit a

report would not be meaningful and is more than is necessary to ensure that systems comply with

off-axis power density limits. The Commission’s rules already provide that earth station

licensees are required to certify within one year of the date of grant of a license that licensed

facilities have been constructed and are operating in accordance with the licensed parameters.60

This certification requirement is all that is necessary for AMSS systems. Requiring AMSS

operators to provide a report or further information on performance tests would impose

58
     Telesat Canada Comments at 3.
59
     Boeing Comments at 29.
60
     47 C.F.R. § 25.133.

                                                 21
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                                                                             ViaSat, Inc. Reply Comments
                                                                                      IB Docket No. 05-20
                                                                                     Filed August 3, 2005

administrative burdens on the AMSS operator and is unlikely to provide any additional benefit to

the Commission or other service providers in the Ku-band.

           B.       ALSAT Designation

                    The comments submitted in this proceeding reinforce ViaSat’s support for

allowing ALSAT authority for AES terminals.61 In addition to the comments of AMSS

operators, Telesat Canada also supports ALSAT designations for AES antennas.62 However,

Telesat Canada proposes to limit ALSAT authority to AES terminals that are 2-degree

compliant. The off-axis EIRP density limits and the contention exceedance table are intended to

represent the level of interference that satellites in a 2-degree spacing environment are able to

tolerate. Thus, the Commission should instead make clear that ALSAT authority is available for

antennas that comply with the off-axis power density limits, as adjusted by the contention

exceedance table.63

                    As the Commission determined in the context of ESVs, allowing ALSAT

designations to Ku-band AMSS operators would afford flexibility to negotiate with multiple

satellite service providers for satellite capacity.64 Requiring AMSS operators to file

modifications each time they wish to change satellite providers, or in instances where traffic is

migrated to a different satellite in the satellite operator’s fleet, would impose unnecessary

burdens on AMSS applicants and on the Commission.

                    AES terminals are no different than VSATs from an interference perspective; i.e.,

an AES terminal that complies with the same off-axis EIRP density limits as VSAT terminals


61
     Boeing Comments at 35; ARINC Comments at 23.
62
     Telesat Canada Comments at 4.
63
     ARINC at 23.
64
     Id.

                                                    22
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                                                                              ViaSat, Inc. Reply Comments
                                                                                       IB Docket No. 05-20
                                                                                      Filed August 3, 2005

 would not cause any more interference into adjacent satellites. Therefore, there is no reason not

 to afford AES licensees the ability to modify their points of communication without prior FCC

 authority, as long as the satellite is U.S.-licensed or is a non-US-licensed satellite with an

 ALSAT designation.

 VII.    CONCLUSION

                For the foregoing reasons, ViaSat respectfully requests that the Commission adopt

 service rules and streamlined licensing procedures for AMSS consistent with the proposals in

 ViaSat’s comments and in these reply comments. Further, ViaSat requests that the Commission

 consider the issues raised by the Departments in a separate proceeding.

                                                    Respectfully submitted,

                                                    VIASAT, INC.




                                                    By:       /s/ John P. Janka
                                                          John P. Janka
                                                          Teresa D. Baer
                                                          Elizabeth R. Park
                                                          LATHAM & WATKINS LLP
                                                          555 Eleventh St., N.W., Suite 1000
                                                          Washington, D.C. 20004
                                                          202-637-2200

                                                          Counsel for ViaSat, Inc.


Filed: August 3, 2005




                                                   23
 DC\778232.4


                                                                          ViaSat, Inc. Reply Comments
                                                                                              Exhibit A
                                                                                   IB Docket No. 05-20
                                                                                  Filed August 3, 2005



                                          Exhibit A
Technical Summary of Pointing Error Effects
Introduction
This document describes the effects of antenna pointing errors of aeronautical earth
stations (AES) terminals in a network using direct sequence spread spectrum and CDMA.
Analysis of the components that induce pointing error, and simulation of a population of
such AES terminals with random error, show that pointing errors of individual AES
terminals do not cause harmful interference to adjacent satellite systems – even at
pointing errors an order of magnitude greater than the 0.2° pointing accuracy requirement
proposed by the FCC in the Notice of Proposed Rulemaking (NPRM).

Additionally, the simulation shows that AMSS networks employing dynamic power
control and congestion control1 can model and account for pointing error of individual
terminals on an aggregate basis, such that the overall network off-axis EIRP density is
maintained within the FCC’s proposed mask.


Elements of Pointing Error
A number of factors can cause AES antennas to become mispointed. These errors can be
described as either static or dynamic and may be nonrandom or random in nature.

An example of static error would be the case where upon installation, the antenna base
plate was improperly aligned in the azimuth plane by some fixed amount. In practice
however, the installation process includes a calibration routine where any alignment
errors are detected and corrected. Therefore, this analysis does not include this type of
error as a factor.

An example of a dynamic error would be a case where during turbulence the airframe
flexes to a degree where some mis-alignment between the nose and tail is present. This
momentary mispointing would return to normal after the aircraft transits the air pocket.
The direction and magnitude of error induced would be random. This simulation
assumes dynamic, random errors.

The ViaSat tail mounted antenna subsystem (TMASS) used by ARINC in their AMSS
network uses an open loop pointing algorithm. The algorithm takes in to account:
   • Ephemeris data stored in the AES to determine the satellite location and
      polarization


1
 Congestion control reduces the number of simultaneously transmitting AES terminals when network
aggregate EIRP density levels reach defined thresholds.

                                                  1
DC\781749.1


                                                                    ViaSat, Inc. Reply Comments
                                                                                        Exhibit A
                                                                             IB Docket No. 05-20
                                                                            Filed August 3, 2005

    •   Stored constants to determine the antenna orientation relative to the airframe (part
        of commissioning calibration test procedure)
    •   Latitude, longitude, and altitude data from the aircraft inertial navigation system
        (INS) to determine the aircraft location
    •   Heading, pitch, roll, and yaw data from the aircraft INS to determine the aircraft
        orientation
    •   Speed, pitch, roll, and yaw rate of change data from the aircraft INS to predict
        changes in aircraft location and orientation.

Once the AES terminal is assigned to a particular point of communication, the antenna
control unit (ACU) continuously updates the pointing of the antenna based on new data
from the INS. New data is provided from the INS every 0.02 seconds with a resolution
of 0.05º. The ACU computes the desired steering inputs for the antenna’s azimuth,
elevation, and polarization motors once every millisecond. The antenna mechanical
resolution is 0.09º and the motors accelerate at up to 40º/s2 and drive each axis at a
nominal 30º/s. The calculated root mean squared (RMS) pointing error for the system
typically is less than 0.1º during normal flight operations.

If the AES detects an ACU or TMASS error or loses receive lock on the downlink signal
from the satellite, the transmitter is inhibited within 250 ms.


The Simulation
The simulation has several inputs: a reference antenna gain pattern for individual AES
terminals, the number of iterations to run, and the standard deviation for the pointing
error.

Reference Antenna Pattern
The simulations in this summary represent a simplified 0.2921 m reference antenna
pattern that is symmetric about both the elevation and azimuth planes. The reference
pattern was generated based on the mean magnitude of off-axis gain at each 0.2° angle
increment off the main beam in any direction. The purpose of this approach is to
simplify the look-up of off-axis gain in any direction, especially at off-axis angles greater
than 5º, where the sidelobe patterns for azimuth and elevation planes are significantly
different.


Standard Deviation for Pointing Error
The simulation generates a random error in degrees for both the elevation and azimuth
planes with a normal, or Gaussian, probability distribution. The initial simulation run in
this analysis is based on the FCC’s proposal in the NPRM that pointing accuracy be
maintained with 0.2º. While the FCC does not provide an allowance for exceeding such a
limit, the standard deviation values used in the simulation were selected based on
reasonable “real-world” assumptions common in the satellite industry. The simulation

                                              2
DC\781749.1


                                                                                                                                                                                                                                                                                          ViaSat, Inc. Reply Comments
                                                                                                                                                                                                                                                                                                              Exhibit A
                                                                                                                                                                                                                                                                                                   IB Docket No. 05-20
                                                                                                                                                                                                                                                                                                  Filed August 3, 2005

assumes that AES pointing accuracy is maintained within 0.2°, 99.73% of the time, or
three standard deviations (3σ). Accuracy at a 99.73% level is consistent with the
common satellite industry standard for link availability, and thus, is a reasonable
assumption for this simulation. In addition to the 0.2º pointing error simulation, other
simulations were run at increasingly higher 3σ values of 0.5º, 1º, 5º, and 10º. ViaSat does
not propose these higher values as alternative antenna pointing accuracy requirements.
Instead, ViaSat includes the results of such simulations in this analysis to illustrate that
aggregate off-axis EIRP density increases are relatively small, even when random
pointing errors are 20 times greater than the FCC’s proposed pointing accuracy
requirement. AMSS operators can adequately manage the effects of any such errors
through dynamic power control / congestion control of the network.

The standard deviation (1σ) values selected for the simulation runs were 0.0666º,
0.1666º, 0.3333º, 1.6666º, and 3.3333º. These values correspond to the 3σ values of 0.2º,
0.5º, 1.0º, 5º, and 10º, respectively. Figure 1 shows the familiar normal curve for the
1.6666º standard deviation (3σ = 5.0°) case.

 700




 600




 500




 400




 300




 200




 100




   0
       -6.667
                -6.316
                         -5.965
                                  -5.614
                                           -5.263
                                                    -4.912
                                                             -4.561
                                                                      -4.211
                                                                               -3.860
                                                                                        -3.509
                                                                                                 -3.158
                                                                                                          -2.807
                                                                                                                   -2.456
                                                                                                                            -2.105
                                                                                                                                     -1.754
                                                                                                                                              -1.404
                                                                                                                                                       -1.053
                                                                                                                                                                -0.702
                                                                                                                                                                         -0.351
                                                                                                                                                                                  0.000
                                                                                                                                                                                          0.351
                                                                                                                                                                                                  0.702
                                                                                                                                                                                                          1.053
                                                                                                                                                                                                                  1.404
                                                                                                                                                                                                                          1.754
                                                                                                                                                                                                                                  2.105
                                                                                                                                                                                                                                          2.456
                                                                                                                                                                                                                                                  2.807
                                                                                                                                                                                                                                                          3.158
                                                                                                                                                                                                                                                                  3.509
                                                                                                                                                                                                                                                                          3.860
                                                                                                                                                                                                                                                                                  4.211
                                                                                                                                                                                                                                                                                          4.561
                                                                                                                                                                                                                                                                                                  4.912
                                                                                                                                                                                                                                                                                                          5.263
                                                                                                                                                                                                                                                                                                                  5.614
                                                                                                                                                                                                                                                                                                                          5.965
                                                                                                                                                                                                                                                                                                                                  6.316
                                                                                                                                                                                                                                                                                                                                          6.667




                    Figure 1 - Sample Frequency Distribution of Pointing Error (1σ = 1.6666 deg, 3σ = 5.0)



Table 1 shows the percentage of time that pointing error would be less than a given value.
The 1σ and 3σ values are highlighted.




                                                                                                                                                                                                  3
DC\781749.1


                                                                        ViaSat, Inc. Reply Comments
                                                                                            Exhibit A
                                                                                 IB Docket No. 05-20
                                                                                Filed August 3, 2005

For example, a 3σ value of 0.2º means that 99.7% of the time the error in either the
azimuth or elevation axis will be less than 0.2º and that 68.3% of the time it will be less
than 0.0666º.

The percentage of time under the normal curve must always add up to 100%. So for
example in the 0.2º case, 20% of the time the error will be 0.0169º or less and 80% of the
time it will be greater than 0.0169. Similarly if 80% of the time, pointing error is less
than 0.0854º, and 20% of the time it is greater than 0.0169º then 60% of the time it must
be between 0.0854º and 0.0169º.


              Percentage     0.2º       0.5º        1.0º      5.0º     10.0º
    σ           of time      (3σ)       (3σ)        (3σ)      (3σ)      (3σ)
 0.2534        20.00%      0.0169º    0.0422º     0.0845º   0.4223º   0.8447º
 0.3854        30.00%      0.0257º    0.0642º     0.1285º   0.6423º   1.2847º
 0.5245        40.00%      0.0350º    0.0874º     0.1748º   0.8742º   1.7483º
 0.6745        50.00%      0.0450º    0.1124º     0.2248º   1.1242º   2.2483º
 0.8417        60.00%      0.0561º    0.1403º     0.2806º   1.4028º   2.8057º
 1.0000        68.27%      0.0667º    0.1667º     0.3333º   1.6667º   3.3333º
 1.0365        70.00%      0.0691º    0.1728º     0.3455º   1.7275º   3.4550º
 1.2816        80.00%      0.0854º    0.2136º     0.4272º   2.1360º   4.2720º
 1.6450        90.00%      0.1097º    0.2742º     0.5483º   2.7417º   5.4833º
 1.9600        95.00%      0.1307º    0.3267º     0.6533º   3.2667º   6.5333º
 2.2420        97.50%      0.1495º    0.3737º     0.7473º   3.7367º   7.4733º
 2.5760        99.00%      0.1717º    0.4293º     0.8587º   4.2933º   8.5867º
 2.8100        99.50%      0.1873º    0.4683º     0.9367º   4.6833º   9.3667º
 3.0000        99.73%      0.2000º    0.5000º     1.0000º   5.0000º   10.0000º
 3.3000        99.90%      0.2200º    0.5500º     1.1000º   5.5000º   11.0000º
 3.9000        99.99%      0.2600º    0.6500º     1.3000º   6.5000º   13.0000º

                     Table 1 – Degrees of Pointing Error vs. Percentage of Time



The magnitude of error calculations in Table 1 above take into account the direction of
the error – either azimuth or elevation. Thus, the magnitude of the combined error vector
is:
Total _ Error =     Az _ Error 2 + El _ Error 2

See Figure 2.

i.e., if the error in the azimuth axis is 0.2º at the same time it is 0.2º in the elevation axis
the total error would be 0.28º.




                                                  4
DC\781749.1


                                                                   ViaSat, Inc. Reply Comments
                                                                                       Exhibit A
                                                                            IB Docket No. 05-20
                                                                           Filed August 3, 2005




                             Figure 2 – Resultant Pointing Error



AES Terminal Locations
The simulation uses a ±10º range across the geostationary arc and includes satellite
locations from 85º West longitude to 105º West longitude. The analysis described in this
document assumes random AES locations in order to simulate mobile AES terminals.
The simulator generates for each iteration a random latitude and longitude within the
geographic boundaries of CONUS for the AES location.


How The Simulation Works
During a simulation run, the simulator calculates for each iteration the look angle from
the new AES location to each 0.2° increment, or “location of interest” along the
geosynchronous arc from 85º WL to 105º WL. The simulator creates a “data bin” for
each location of interest, into which the off-axis gain measurements for such location of
interest are collected.

Next, the program generates a random pointing error value for azimuth and elevation
based on the standard deviation assumption input. The azimuth and elevation error
components are added together to determine the total error offset angle and magnitude.
For each location of interest along the orbital arc, the resultant change in off-axis gain
over a properly pointed antenna is calculated and added to the data bin for that location of
interest.



                                             5
DC\781749.1


                                                                              ViaSat, Inc. Reply Comments
                                                                                                  Exhibit A
                                                                                       IB Docket No. 05-20
                                                                                      Filed August 3, 2005

The simulator calculates multiple iterations of this process until the desired number of
iterations has been reached. The simulations in this summary are based on 1 million
iterations.2 At the conclusion of the simulation run, each data bin contains the sum of all
the off-axis gain from each AES terminal in the direction of that particular location of
interest. The simulator compiles the output for each data bin in a file available for
review.


Geocentric angle versus Topocentric angle
The spacing of satellites along the geostationary arc is nominally every 2º along the
equator. That is, the angle between two satellites as seen from the center of the earth, or
geocentric, is 2º. The angle between two satellites from the perspective of the AES
terminal operating on or above the surface of the earth is the topocentric angle. The
topocentric angle between two satellites from the perspective of an AES terminal will
always be greater than the geocentric angle. The actual angle as observed by the AES
depends upon the location of the AES terminal. When AES terminals are allowed to
move about within the simulation, each terminal will have a slightly different topocentric
angle to the geostationary arc depending upon its location.

The simulation results in the charts below are based on the topocentric angle. Therefore,
the data points are plotted over +/- 12.1 degrees, which represents the average topocentric
angle across the U.S. for +/- 10 degrees of geocentric angle.


Results of Pointing Error Simulation
The charts in Figures 3 and 4 below illustrate the baseline off-axis EIRP density of the
AES terminals used for the simulation. Figure 3 shows the reference antenna pattern
from a single centrally located antenna, as plotted across the geographic arc versus the
current 25.209 mask. This is to establish a baseline off-axis EIRP density profile across
the geographic arc from 85º WL to 105º WL. The antenna off-axis gain in this case does
not meet the requirements of 25.209; thus, the antenna input power density is reduced to
meet the intent of 25.209 and 25.134 and the proposed FCC off-axis EIRP density mask.
A second plot on the chart shows the antenna pattern amplitude reduced by lowering the
input power density via direct sequence spread spectrum (DSSS) to just meet the mask.
This pattern represents the input power density reduction required by a single transmitter
to meet the mask limits.

Because the ViaSat AMSS network uses CDMA, the input power density of individual
AES antennas is further reduced so that the aggregate off-axis EIRP density of all AES
terminals in the network complies with the mask. The greater the number of
simultaneously active terminals in the network, the further each terminal’s input power

2
  The simulation results for iterations greater than 100 converge quickly, and thus, the difference between
the network aggregate patterns plotted for a simulation based on 100 iterations and a simulation based on 1
million iterations is small.

                                                     6
DC\781749.1


                                                                                                                                                                                     ViaSat, Inc. Reply Comments
                                                                                                                                                                                                         Exhibit A
                                                                                                                                                                                              IB Docket No. 05-20
                                                                                                                                                                                             Filed August 3, 2005

density must be reduced. A third plot in Figure 3 shows the gain plot reduced an
additional 20 dB, simulating in this case that the AES is one terminal out of a network of
100 technically identical CDMA terminals.

                       40




                       30
                                                                                                                                                                                          FCC 25.209 Mask


                       20


                                                                                                                                                                                          Single E.S. No Pointing
                                                                                                                                                                                          Error
 Off-Axis Gain (dBi)




                       10



                                                                                                                                                                                          Single E.S. No Pointing
                        0                                                                                                                                                                 Error, Input Pwr Density
                                                                                                                                                                                          reduced by delta dB to
                                                                                                                                                                                          meet off-axis EIRP Mask


                       -10                                                                                                                                                                Single E.S. No Pointing
                                                                                                                                                                                          Error, Input Pwr Density
                                                                                                                                                                                          reduced by additional 20
                                                                                                                                                                                          dB
                       -20




                       -30
                             12.10

                                     10.88

                                             9.66

                                                    8.45

                                                           7.24

                                                                   6.03

                                                                          4.82

                                                                                 3.61

                                                                                        2.41

                                                                                               1.20

                                                                                                      0.00

                                                                                                             1.20

                                                                                                                    2.41

                                                                                                                           3.61

                                                                                                                                  4.82

                                                                                                                                         6.03

                                                                                                                                                7.24

                                                                                                                                                       8.45

                                                                                                                                                              9.66

                                                                                                                                                                     10.88

                                                                                                                                                                             12.10


                                                                  Average U.S. Earth Station θ Across +/- 10º of GEO Arc


                                                           Figure 3 - Representative Antenna Pattern (no pointing error)




                                                                                                                              7
DC\781749.1


                                                                                                                                                                                     ViaSat, Inc. Reply Comments
                                                                                                                                                                                                         Exhibit A
                                                                                                                                                                                              IB Docket No. 05-20
                                                                                                                                                                                             Filed August 3, 2005

Figure 4 illustrates a baseline plot of network aggregate off-axis gain for a large
population of perfectly pointed AES terminals transmitting from random locations. The
patterns in Figure 4 appear smoother than those in Figure 3 due to the averaging of the
varying topocentric angles across the satellite arc for different terminal locations. The
patterns in Figure 4 serve as the baseline off-axis gain pattern reference to which the
results of the pointing error simulation should be compared.

                       30


                                                                                                                                                                                        FCC 25.209 Mask


                       20




                       10
 Off-Axis Gain (dBi)




                                                                                                                                                                                        Network Aggregate of
                                                                                                                                                                                        Composite Random U.S.
                                                                                                                                                                                        E.S. Locations, Each
                        0                                                                                                                                                               operating with Input Pwr
                                                                                                                                                                                        Density reduced by delta
                                                                                                                                                                                        + 20 dB. No Pointing
                                                                                                                                                                                        Error


                       -10

                                                                                                                                                                                        Single E.S. (Composite of
                                                                                                                                                                                        Random U.S. E.S.
                                                                                                                                                                                        Locations), No Pointing
                       -20                                                                                                                                                              Error, E.S. Input Pwr
                                                                                                                                                                                        Density reduced by delta
                                                                                                                                                                                        + 20 dB from Network
                                                                                                                                                                                        Aggregate


                       -30
                             12.10

                                     10.88

                                             9.66

                                                    8.45

                                                           7.24

                                                                   6.03

                                                                          4.82

                                                                                 3.61

                                                                                        2.41

                                                                                               1.20

                                                                                                      0.00

                                                                                                             1.20

                                                                                                                    2.41

                                                                                                                           3.61

                                                                                                                                  4.82

                                                                                                                                         6.03

                                                                                                                                                7.24

                                                                                                                                                       8.45

                                                                                                                                                              9.66

                                                                                                                                                                     10.88

                                                                                                                                                                             12.10




                                                                  Average U.S. Earth Station θ Across +/- 10º of GEO Arc


                                                           Figure 4 - Reference Antenna Pattern for Composite Locations



As illustrated in Figure 4, the effect of a single AES terminal in the 100 node CDMA
network described above with its antenna mispointed by 0.2º, 0.5º, 1.0º, 5.0º, or even 10º
would be minimal. As seen from the pattern of the individual antenna, even when
shifting the antenna pattern fully to the right or left side of the plot, the level of
interference generated by this single terminal is well below the mask and too low to cause
harmful interference into adjacent satellites.

In a CDMA system, the larger the number of AES terminals transmitting simultaneously
co-frequency, the smaller the individual contribution of each AES will be to the network
aggregate power density. This reduction of power into individual antennas further lowers
the likelihood that any given terminal on its own can cause interference into an adjacent
system. Conversely, a conventional VSAT terminal not using CDMA, and operating at
the limits of the mask, could easily exceed the mask and cause interference by a small
shift of the antenna pattern to the right or left. In this case, much tighter pointing
accuracy would be required to prevent harmful interference into adjacent satellites.

                                                                                                                                  8
DC\781749.1


                                                                                                                                                                                     ViaSat, Inc. Reply Comments
                                                                                                                                                                                                         Exhibit A
                                                                                                                                                                                              IB Docket No. 05-20
                                                                                                                                                                                             Filed August 3, 2005

Figure 5 shows several AES terminals at random locations with random antenna
mispointing. The simulation generating these results assumes a 1.666° standard deviation
(3σ = 5.0º) input for the pointing error. Figure 5 also includes the baseline reference
network aggregate plot, plus the composite off-axis plot resulting from one million
iterations (each iteration simulates a single AES terminal at a random location with
random error). As illustrated in this chart, the pointing error across the network of
terminals increases the composite off-axis EIRP density at 3.61º by only 0.5 dB.


                       30
                                                                                                                                                                                       FCC 25.209 Mask




                                                                                                                                                                                       Network Aggregate of Composite Random
                                                                                                                                                                                       U.S. E.S. Locations, Each operating with
                       20                                                                                                                                                              Input Pwr Density reduced by delta + 20 dB.
                                                                                                                                                                                       No Pointing Error


                                                                                                                                                                                       Single E.S. (Composite of Random U.S.
                                                                                                                                                                                       E.S. Locations), No Pointing Error, E.S.
                                                                                                                                                                                       Input Pwr Density reduced by delta + 20 dB
                                                                                                                                                                                       from Network Aggregate
                       10
                                                                                                                                                                                       E.S. 1
 Off-Axis Gain (dBi)




                                                                                                                                                                                       E.S. 2
                        0


                                                                                                                                                                                       E.S. 3




                       -10
                                                                                                                                                                                       E.S. 4




                                                                                                                                                                                       E.S. 5
                       -20


                                                                                                                                                                                       Composite of 1 Million Random E.S.
                                                                                                                                                                                       Locations, Each with Random Pointing
                                                                                                                                                                                       Error (Az & El) of 5º (3 σ)


                       -30
                             12.10

                                     10.88




                                                                                                                                                                     10.88

                                                                                                                                                                             12.10
                                             9.66

                                                    8.45

                                                           7.24

                                                                   6.03

                                                                          4.82

                                                                                 3.61

                                                                                        2.41

                                                                                               1.20

                                                                                                      0.00

                                                                                                             1.20

                                                                                                                    2.41

                                                                                                                           3.61

                                                                                                                                  4.82

                                                                                                                                         6.03

                                                                                                                                                7.24

                                                                                                                                                       8.45

                                                                                                                                                              9.66




                                                                  Average U.S. Earth Station θ Across +/- 10º of GEO Arc


                                                                                                Figure 5 – Results for 5º (3σ)

Figures 6 - 10 show the baseline reference plot compared to the composite off-axis gain
profiles for one million iterations (randomly located AES terminals with random antenna
mispointing) at 3σ values of 0.2º, 0.5º, 1.0º, 5º, and 10º. As shown in Figures 6-8, for
pointing accuracy assumptions up to 1.0º there is no appreciable change in the network
aggregate off-axis gain profile seen by the observers along the geostationary arc – the
reference plot and the pointing error plot are virtually indistinguishable. For pointing
accuracy assumptions of 5º and 10º, the network aggregate off-axis gain profile only
exceeds the mask by 0.5 to 1.35 dB, and is only slightly higher than the baseline off-axis
profile.




                                                                                                                              9
DC\781749.1


                                                                                                                                                                     ViaSat, Inc. Reply Comments
                                                                                                                                                                                         Exhibit A
                                                                                                                                                                              IB Docket No. 05-20
                                                                                                                                                                             Filed August 3, 2005


 30


 25


 20


 15                                                                                                                                                                             Composite
                                                                                                                                                                                Reference



                                                                                                                                                                                0.2º (3 σ) Pointing
 10                                                                                                                                                                             Error Case



                                                                                                                                                                                FCC 25.209 Mask
   5


   0


  -5


 -10
       12.10
               10.88
                       9.66
                              8.45
                                      7.24
                                              6.03
                                                       4.82
                                                              3.61
                                                                      2.41
                                                                              1.20
                                                                                     0.00
                                                                                               1.20
                                                                                                       2.41
                                                                                                              3.61
                                                                                                                     4.82
                                                                                                                            6.03
                                                                                                                                   7.24
                                                                                                                                           8.45
                                                                                                                                                    9.66
                                                                                                                                                             10.88
                                                                                                                                                                      12.10
                                                                             Figure 6 - Results for 0.2º (3σ)


  30


  25


  20


  15                                                                                                                                                                   Composite
                                                                                                                                                                       Reference


                                                                                                                                                                       0.5º (3 σ) Pointing
  10                                                                                                                                                                   Error Case


                                                                                                                                                                       FCC 25.209 Mask


   5


   0


  -5


 -10
       12.10
               10.88
                       9.66
                              8.45
                                     7.24
                                             6.03
                                                     4.82
                                                            3.61
                                                                   2.41
                                                                          1.20
                                                                                 0.00
                                                                                        1.20
                                                                                                2.41
                                                                                                       3.61
                                                                                                              4.82
                                                                                                                     6.03
                                                                                                                            7.24
                                                                                                                                   8.45
                                                                                                                                          9.66
                                                                                                                                                  10.88
                                                                                                                                                           12.10




                                                                             Figure 7 - Results for 0.5º (3σ)




                                                                                                          10
DC\781749.1


                                                                                                                                                        ViaSat, Inc. Reply Comments
                                                                                                                                                                            Exhibit A
                                                                                                                                                                 IB Docket No. 05-20
                                                                                                                                                                Filed August 3, 2005


 30


 25


 20


 15                                                                                                                                                              Composite
                                                                                                                                                                 Reference



                                                                                                                                                                 1º (3 σ) Pointing
 10                                                                                                                                                              Error Case



                                                                                                                                                                 FCC 25.209 Mask

   5


   0


  -5


 -10
       12.10
               10.88
                       9.66
                              8.45
                                     7.24
                                            6.03
                                                   4.82
                                                          3.61
                                                                 2.41
                                                                        1.20
                                                                               0.00
                                                                                      1.20
                                                                                             2.41
                                                                                                    3.61
                                                                                                           4.82
                                                                                                                  6.03
                                                                                                                         7.24
                                                                                                                                8.45
                                                                                                                                        9.66
                                                                                                                                                10.88
                                                                                                                                                         12.10
                                                                        Figure 8 - Results for 1.0º (3σ)


 30


 25


 20
                                                                                                                                                                 Composite
                                                                                                                                                                 Reference
 15


 10                                                                                                                                                              5º (3 σ) Pointing
                                                                                                                                                                 Error Case



   5
                                                                                                                                                                 FCC 25.209 Mask


   0


  -5


 -10
       12.10
               10.88
                       9.66
                              8.45
                                     7.24
                                            6.03
                                                   4.82
                                                          3.61
                                                                 2.41
                                                                        1.20
                                                                               0.00
                                                                                      1.20
                                                                                             2.41
                                                                                                    3.61
                                                                                                           4.82
                                                                                                                  6.03
                                                                                                                         7.24
                                                                                                                                8.45
                                                                                                                                       9.66
                                                                                                                                               10.88
                                                                                                                                                        12.10




                                                                        Figure 9 - Result for 5.0º (3σ)




                                                                                                    11
DC\781749.1


                                                                                                                                                      ViaSat, Inc. Reply Comments
                                                                                                                                                                          Exhibit A
                                                                                                                                                               IB Docket No. 05-20
                                                                                                                                                              Filed August 3, 2005


 30


 25


 20
                                                                                                                                                              FCC 25.209 Mask


 15
                                                                                                                                                              Composite
                                                                                                                                                              Reference

 10
                                                                                                                                                              10º (3 σ) Pointing
                                                                                                                                                              Error Case

   5


   0


  -5


 -10
       12.10
               10.88
                       9.66
                              8.45
                                     7.24
                                            6.03
                                                   4.82
                                                          3.61
                                                                 2.41
                                                                        1.20
                                                                               0.00
                                                                                      1.20
                                                                                             2.41
                                                                                                    3.61
                                                                                                           4.82
                                                                                                                  6.03
                                                                                                                         7.24
                                                                                                                                8.45
                                                                                                                                       9.66
                                                                                                                                              10.88
                                                                                                                                                      12.10
                                                                    Figure 10 - Result for 10.0º (3σ)




Conclusion
The simulation shows that because the pointing error in these examples is random and
dynamic in nature, and because the network is comprised of a large number of terminals
using CDMA, the network aggregate off-axis EIRP density is only slightly increased
even when significant pointing errors are present on individual AES terminals. The
transient nature of these errors are such that violation of the mask would only occur for
very short periods – even in a system not employing dynamic power control / congestion
control.

The allowances in the proposed contention exceedance table would capture such
momentary increases in aggregate off-axis EIRP density resulting from pointing errors.
AMSS network operators using dynamic power control / congestion control are able to
reduce network aggregate off-axis EIRP density to levels that comply with the off-axis
EIRP density limits, as adjusted by the allowances in the contention table. Therefore, a
separate pointing error limit for these systems is unnecessary.




                                                                                                    12
DC\781749.1





Document Created: 2007-07-18 15:51:25
Document Modified: 2007-07-18 15:51:25

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