Attachment Exhibit A

This document pretains to SES-LIC-20180123-00055 for License on a Satellite Earth Station filing.

IBFS_SESLIC2018012300055_1329530

                                         EXHIBIT A

                       Application for Ka band Aeronautical Antenna

       By this application, Viasat, Inc. (“Viasat”) requests blanket authority to operate two
transmit/receive earth station antenna models mounted on aircraft to provide service in
the United States using the ViaSat-2 satellite: (i) the Mantarray M40 antenna, which the
Commission has already authorized to operate with Viasat’s other spacecraft,1 and (ii) the
Global Mantarray GM40 antenna, which is a variation of the Mantarray M40 that is
optimized for the ViaSat-2 satellite architecture.

       Grant of this application would promote the public interest by enabling the
provision of expanded broadband service to passengers and crew on board commercial
and private aircraft using the ViaSat-2 satellite, which is expected to commence commercial
service during the first quarter of 2018. In granting access for satellite to additional
spectrum in the Spectrum Frontiers proceeding, the Commission cited comments from
major U.S. airlines that are Viasat customers “argu[ing] that as demand for in-flight
broadband grows, airlines and their satellite broadband partners will need access to more
spectrum to meet consumer demand.”2

             1. Frequencies, Satellite Points of Communication and Geographic Area of
                Operation

       The earth stations will operate using the 17.7-18.3 GHz, 18.3-18.8 GHz and 19.7-
20.2 GHz portions of the Ka band for downlinks, and 28.35-28.6 GHz and 29.5-30 GHz for
uplinks. The Commission’s Ka-band band plan designates the 18.3-18.8 GHz, 19.7-20.2
GHz, 28.35-28.6 GHz and 29.5-30 GHz portions of the Ka band for GSO FSS on a primary
basis. The 17.8-18.3 GHz band segment has been allocated on a secondary basis for FSS
downlinks.3 The 17.7-17.8 GHz band segment is allocated on a co-primary basis to the
terrestrial fixed service and BSS feeder links in the Earth-to-space direction.4 Thus,




1See Viasat, Inc., File No. SES-LIC-20120427-00404, Call Sign E120075 (granted July 17,
2013).
2Use of Spectrum Bands Above 24 GHz for Mobile Radio Services, GN Docket No. 14-177,
Second Report and Order, FCC 17-152, at ¶ 188 (rel. Nov. 22, 2017); see also American
Airlines Ex Parte Presentation, GN Docket No. 14-177, et al., at 1 (Nov. 9, 2017); JetBlue
Airways, Ex Parte Presentation, GN Docket No. 14-177, et al., at 1 (Nov. 9, 2017).
3See Update to Parts 2 and 25 Concerning Non-Geostationary, Fixed-Satellite Service Systems
and Related Matters, Report and Order, 32 FCC Rcd 7809, ¶ 7 (2017) (“NGSO Order”).
4   47 C.F.R. § 2.106 n.US271.


consistent with the waiver already granted for market access for ViaSat-2,5 Viasat requests
a waiver to receive satellite downlink communications in the 17.7-17.8 GHz band segment.

        These earth stations will communicate with the ViaSat-2 satellite at the 69.9º W.L.
orbital location. The Commission has granted U.S. market access for ViaSat-2, which is
operated under the authority of the United Kingdom, to use these frequency bands.6

      The earth stations will operate throughout the coverage area of the ViaSat-2 satellite
and can be operated with each of the gateway earth stations for ViaSat-2.7

             2. Operation on Mobile Platforms

       The earth stations will be mounted on commercial and private aircraft and will be
used to provide two-way, in-flight broadband communications, including Internet access,
and will be operated while in flight and at fixed locations while on the ground. The
Commission is considering the adoption of rules that would authorize earth stations in
motion in Ka-band frequencies. In commencing that proceeding, the Commission
acknowledges that it is now well-established in the industry and in the Commission’s
precedent that GSO FSS spectrum can be used for earth stations on mobile platforms
without adversely changing the operating environment created by a traditional FSS earth
station.8 Based on the Commission’s tentative conclusion that FSS earth stations in motion
(“ESIMs”) would be no more interfering than operations in a fixed installation, the
Commission proposes to adopt a footnote to the U.S. Table to recognize the operation of
ESIMs as an application of the FSS with primary status.9

       The earth stations proposed by this application would operate as an application of
the FSS and would be no more interfering than a fixed terminal using the same antennas.
ViaSat-2’s authorized downlink operations in the 17.7-18.3 GHz, 18.3-18.8 GHz, and 19.7-
20.2 GHz band segments are unaffected by the operation of the proposed earth stations. As
demonstrated below and in the technical attachments to this application, the proposed
operations would be compatible with the operations of other GSO systems in the 28.35-
28.6 GHz and 29.5-30 GHz band segments, and also with NGSO systems. In accordance


5Viasat, Inc., File No. SAT-MOD-20160527-00053, Att. To Grant at ¶ 11 (granted Jan. 12,
2017).
6Viasat, Inc., Call Sign S2902, File Nos. SAT-LOI-20130319-00040 (granted Dec. 12, 2013);
SAT-MOD-20141105-00121; SAT-AMD-20150105-00002 (granted Apr. 15, 2015); SAT-
MOD-20160527-00053 (granted Jan. 12, 2017) (“ViaSat-2 Authorization”).
7   See 47 C.F.R. § 25.115(e).
8See Amendment of Parts 2 and 25 of the Commission’s Rules to Facilitate the Use of Earth
Stations in Motion Communicating with Geostationary Orbit Space Stations in Frequency
Bands Allocated to the Fixed Satellite Service, IB Docket No. 17-95, Notice of Proposed
Rulemaking, FCC 17-56, ¶ 53 (rel. May 19, 2017).
9   Id.
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with the requirements in Section 25.220 for the operation of earth stations at non-routine
power levels, Viasat is in the process of coordinating exceedances in the off-axis EIRP
density envelope in certain limited scenarios in the direction of the GSO arc with the one
GSO satellite operator that potentially could be impacted by the operation of the proposed
antennas at certain skew angles. Therefore, to the extent the Commission adopts the
proposed ESIM rules that would treat such operations as an application of the FSS with
primary status in the 18.3-18.8 GHz, 19.7-20.2 GHz, 28.35-28.6 GHz and 29.5-30 GHz band
segments, Viasat requests that the proposed earth stations be authorized on that basis. In
the meantime, to the extent necessary and out of an abundance of caution, Viasat seeks a
waiver of the U.S. Table, and the Commission’s Ka-band band plan, to operate mobile earth
stations in frequencies allocated for FSS. The Commission has granted such waivers to
allow Viasat to operate aeronautical earth stations, including one of the models included
here, with Viasat’s other spacecraft,10 and has granted authority to other licensees to
operate earth stations on mobile platforms in the Ka band.11

          3. Antenna Performance and Compatibility with GSO FSS Operations

        The attached Technical Description in Attachment 1 describes the antenna
specifications, network architecture, and antenna pointing mechanism for the GM40 and
M40 antennas. The previously-authorized M40 antenna and the new GM40 antenna share
the same antenna patterns, which are attached hereto as Exhibit B. The antenna patterns
provided are in accordance with Section 25.115(g)(1), except that patterns were only able
to be generated to +/- 80 degrees, rather than +/- 180 degrees for the co-polarized EIRP
density in the plane tangent to the GSO arc in Section 25.115(g)(1)(i). The near-field range
available for obtaining measurement data for the patterns was limited to 80 degrees.
However, Viasat has developed simulated data for the antennas for off-axis angels out to
+/- 180 degrees and found no exceedances beyond 80 degrees. Viasat thus requests a
limited waiver to provide measured patterns to 80 degrees rather than 180 degrees.12

        This application is consistent with the existing regulatory framework for the Ka
band. The GM40 and M40 antennas comply with the PFD levels in Section 25.138(a)(6). As
illustrated by the antenna patterns in Exhibit B, the GM40 and M40 antennas comply with
the EIRP spectral density limits in Section 25.138(a) in the GSO plane, but exceed to a

10See Viasat, Inc., File No. SES-MOD-20160108-00029, Call Sign E120075 (granted June 29,
2016).
11See, e.g., ISAT US Inc., File No. SES-LIC-20141030-00832, Call Sign E140114 (granted Aug.
11, 2015) (granting waiver for aeronautical earth stations at 19.7-20.2 GHz and 29.5-30
GHz); ISAT US Inc., File No. SES-LIC-20140224-00098, Call Sign E140029 (granted Sept. 29,
2015) (granting waiver for maritime earth stations at 19.7-20.2 GHz and 29.5-30 GHz); see
also O3b Limited, File No. SES-MSC-20151021-00760 (granted Jan. 29, 2016) (granting a
waiver to provide service to 30 foreign-flagged ships using earth stations at 27.6-28.35
GHz).
12See, e.g., Viasat, Inc., File No. SES-MOD-20160108-00029, Call Sign E120075, Condition
90261 (granted June 29, 2016).
                                             3


limited degree the Section 25.138(a)(2) limits in the elevation plane. Specifically, the
antenna patterns show off-axis exceedances for the main lobe in the elevation plane. In
order to avoid a scenario where the main-beam exceedances would impact the GSO arc,
Viasat previously has accepted a condition for the M40 antenna that transmissions would
cease if the antenna-to-GSO skew angle exceeds 60 degrees and the off-axis EIRP spectral
density emissions risk harmful interference to a GSO space station.13 Viasat also agrees to
inhibit transmissions from the M40 and GM40 antennas communicating with ViaSat-2 in
any cases where the skew angles exceed 60 degrees and the off-axis EIRP spectral density
emissions from operation at such angle risk harmful interference to a GSO space station.

        The antenna patterns also show off-axis exceedances for four grating lobes along the
elevation axis. Exhibit B includes plots of the off-axis EIRP spectral density at a 25-degree
skew cut, which illustrates the location and magnitude of the exceedances of these grating
lobes. As illustrated in Figure 2 of Attachment 1, the grating lobes are located well outside
of the GSO arc and could only intersect the GSO arc when the earth station is skewed by
approximately 25 degrees relative to the GSO arc. The supplemental table required by
Section 25.115(g)(1)(viii) detailing the off-axis EIRP density levels that exceed the Section
25.138 envelope is included in a spreadsheet attached as Exhibit D.

        Because the grating lobes occur well outside of the GSO arc, they would intersect the
GSO arc only when the aircraft is traveling within certain geographic locations in which the
GSO arc appears skewed with respect to the local horizon of the antenna, or when the
aircraft is banking at certain angles while in flight. Due to the high speeds at which aircraft
travel, any intersection of a grating lobe with the GSO arc likely would be fleeting.
Moreover, due to the large off-axis angles from the main lobe where these grating lobes
occur, the level of any actual impact to any GSO satellite is extremely low.

        In accordance with Section 25.138(b), Viasat will comply with the coordination
requirements in Section 25.220 with respect to the exceedances of the off-axis EIRP density
envelope in Section 25.138(a) that potentially could impact other GSO networks. Section
25.220 requires coordination of non-conforming earth station operations “with all adjacent
satellite networks . . . within 6º of orbital separation.” However, in the case of the proposed
earth stations, the off-axis EIRP density toward the satellites +/- 6 degrees from ViaSat-2
will not be exceeded in any operating scenario. The only GSO satellites that could
potentially be impacted are those located at off-axis angles where the grating lobes could
radiate toward the GSO arc when the earth stations are operated in certain geographic
locations and at certain skew angles. Moreover, the satellite networks at these off-axis
locations potentially could be impacted only if they have overlapping coverage with ViaSat-
2. As explained in Attachment 1, DirecTV’s satellites operating in the range of 99º W.L. to
103º W.L. are the only networks that are potentially impacted by the grating lobes. Viasat
is coordinating the proposed operations with DirecTV.



13See Viasat, Inc., File No. SES-LIC-20120427-00404, Call Sign E120075, Condition 90097
(granted July 17, 2013).
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             4.        Compatibility with NGSO FSS Operations

       In the 28.35-28.6 GHz and 29.5-30 GHz band segments, the Commission’s band plan
allows NGSO FSS operations on a secondary basis. GSO FSS operations are primary in this
band, and as discussed above, the Commission is contemplating rules allowing ESIMs on a
primary basis as an application of the FSS. However, to the extent necessary and out of an
abundance of caution, Viasat has requested a waiver for the operation of ESIMs while the
adoption of Ka-band ESIM rules is pending and, in connection with that request, provides a
demonstration showing that the proposed ESIM operations are compatible with NGSO FSS
operations in the 28.35-28.6 GHz and 29.5-30 GHz uplink band segments.

       The Technical Description in Attachment 1 includes an analysis of the off-axis EIRP
density in the plane perpendicular to the GSO with respect to the NGSO FSS systems in the
Commission’s Ka-band processing round. Based on simulations conducted using the
technical characteristics of Viasat’s proposed earth stations under typical operating
conditions and the information in the NGSO FSS applications, the proposed operations are
unlikely to cause harmful interference into NGSO systems.

             5. Compatibility with Terrestrial Operations and BSS

        Viasat requests authority for receive operations using the proposed earth stations
from the ViaSat-2 satellite in the 17.7-18.3 GHz band segment. The U.S. Table allocates the
17.7-18.3 GHz band segment on a primary basis for fixed services. In the 17.8-18.3 GHz
portion of this band segment, the Commission recently adopted a secondary FSS
allocation.14 The 17.7-17.8 GHz portion of the band segment is allocated to FSS on a co-
primary basis, but this FSS allocation is limited by footnote US271 to broadcasting-satellite
service feeder links in the Earth-to-space direction.15

       In seeking market access for ViaSat-2, Viasat demonstrated that its FSS downlinks in
the 17.7-18.3 GHz band segment are compatible with primary fixed service operations and
neighboring BSS operations.16 More specifically, Viasat demonstrated that downlink
transmissions from ViaSat-2 will be within the power-flux density limits at the earth’s
surface set forth in Article 21 of the ITU Radio Regulations and17 would not cause harmful
interference into primary fixed service operations throughout the 17.7-18.3 GHz band
segment.

      Because the 17.7-17.8 GHz band segment is not allocated for the FSS downlinks
proposed in this application, Viasat requests a waiver with respect to this band segment.

14   See NGSO Order at ¶ 7.
15   47 C.F.R. § 2.106 n.US271.
16See Viasat, Inc., File No. SAT-MOD-20160527-00053, Call Sign S2902, Technical Annex at
7-10 (filed May 27, 2016).
17ViaSat-2 Authorization, File No. SAT-MOD-20160527-00053, Att. to Grant at ¶ 12
(granted Jan. 12, 2017).
                                              5


The Commission granted a waiver of the U.S. Table to authorize ViaSat-2 for U.S. market
access based on a showing that the ViaSat-2 downlinks at 17.7-17.8 GHz would not cause
harmful interference into primary fixed service operations or neighboring BSS spacecraft.
A corresponding waiver to allow the proposed earth stations to receive ViaSat-2 downlinks
at 17.7-17.8 GHz would have no impact on the authorized RF environment. To the extent
necessary, Viasat seeks a corresponding waiver to allow the proposed earth stations to
receive signals from ViaSat-2 at 17.7-17.8 GHz. As a non-conforming user of this band
segment, Viasat accepts the risk of interference from conforming spectrum uses.

        In addition, to the extent necessary to authorize the operation of the proposed earth
stations at 17.7-18.3 GHz without specifying their locations, Viasat seeks a waiver of
Section 25.115(e) of the Commission’s rules.18 Licensing multiple earth stations through a
single authorization serves the public interest by reducing administrative costs and delays
and by accelerating system deployment, and thereby facilitating the delivery of expanded
services to end users. The Commission has previously issued licenses for GSO earth
stations in segments of the Ka band other than those identified in Section 25.115(e)
without specifying the locations of the earth stations in advance.19 Therefore, grant of this
waiver request would be consistent with Commission precedent.

             6. Control Point

       The control point for all earth stations will be Viasat’s network operations center
(NOC) located at 349 Inverness Drive South, Englewood, Colorado 80112, and can be
contacted 24/7 at (720) 493-7300. This single point of contact will have the capability of
shutting down any of the earth stations operated within the network, which can occur
through communications with the appropriate ViaSat-2 gateway.

             7. Radiation Hazard Analysis

        The radiation hazard analysis in Exhibit C covers both antenna models. As
demonstrated by the results of the analysis, operation of the proposed terminals will not
result in exceedance of the maximum permissible exposure limits (MPE) in an
Occupational/Controlled Environment.




18   See 47 C.F.R. § 25.115(e).
19 See, e.g., Viasat, Inc., File No. SES-LIC-20170401-00357, Call Sign E170088 (granted Nov.
9, 2017) (authorizing large numbers of GSO earth stations at 17.7-18.3 GHz to
communicate with ViaSat-2).
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Document Created: 0650-04-27 00:00:00
Document Modified: 0650-04-27 00:00:00

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