Attachment TEMPO april 10 1997

TEMPO april 10 1997

COMMENT submitted by TEMPO

Comments

1997-04-10

This document pretains to SAT-STA-19960904-00109 for Special Temporal Authority on a Satellite Space Stations filing.

IBFS_SATSTA1996090400109_1158967

                                                                                  ORIGINAL
                                 WILEY, REIN & FIELDING
                                                1776 k STREET, N. W.

                                            WASHINGTON, D. C. 20006

                                                 (202) 429—7000



                                                                                          FACSIMILE
whiten‘s DIRECT DIAL NUMBER                     Apl”ll 10, 1997                        (202) 429—7049




  (202) $28—4948


  Thomas S. Tycz
  Chief, Satellite and Radiocommunication Division
   International Bureau
  Federal Communications Commission
  2000 M Street, N.W.
   Washington, D.C. 20554

                        Re:    EchoStar Satellite Corporation
                              Directsat Corporation
                              Request for Special Temporary Authority
                              FCC File Nos. 155—SAT—STA—96, 156—SAT—STA—96

  Dear Mr. Tycz:

          TEMPO Satellite, Inc. ("TEMPO"), through its counsel, submits these comments on the
  Technical Annex filed by EchoStar Satellite Corporation ("EchoStar") on March 28, 1997 in
  response to your letter of inquiry regarding the above captioned request for special temporary
  authority ("STA").‘ EchoStar was instructed to supply a technical showing "demonstrating that
  harmful interference will not be caused to other potentially affected satellite systems and U.S.
  permittees," or, alternatively, to obtain the consent of affected satellite operators."




   ‘ Letter from Thomas S. Tycz, Chief, Satellite and Radiocommunication Division, International
  Bureau, to Pantelis Michalopoulos, counsel to EchoStar Satellite Corporation and Directsat
  Corporation, dated Feb. 26, 1997.

  * Id.


Thomas S. Tycz
April 10, 1997
Page 2


       As the Commission has been advised, TEMPO has had discussions with EchoStar
regarding its request to reposition USABSS—3 and USABSS—4 to 119.05° W.L. and 118.95°
W.L., respectively. In this regard, TEMPO has indicated that it has no objection to EchoStar‘s
request to relocate USABSS—4 to 118.95° W.L. Relocating USABSS—4 alleviates some of the
problems that are inherent with the continuous coordination of co—located satellites. Thus, the
FCC should promptly authorize EchoStar to relocate USABSS—4 at least as far west as 118.95°
W.L., and preferably to 119.1° W.L.

       TEMPO does not believe, however, that the Technical Annex filed by EchoStar is
adequate to demonstrate that relocation of USABSS—3 to 119.05° W.L. will not result in harmful
interference to TEMPO‘s system at 118.8° W.L. In particular, as explained in the attached
Technical Statement of TEMPO, EchoStar‘s Technical Annex contains a number of critical
errors and omissions.

         First, EchoStar‘s interference calculations do not conform to the format specified in
Appendix 30A of the International Telecommunication Union ("ITU") Radio Regulations and
fail to evaluate critical factors that may exacerbate the potential for interference. For example,
EchoStar concludes that there is no potential for interference assuming it uses a maximum clear
sky EIRP of 87.4 dBW and TEMPO uses a clear sky EIRP of 83.34 dBW. However, the
maximum licensed EIRP levels for EchoStar and TEMPO are 95 dBW and 80 dBW,
respectively. As noted in the attached Technical Statement, EchoStar‘s interference formula,
using licensed EIRP levels and correcting for the inaccurate cross—polarization value in
EchoStar‘s Technical Annex, would yield a carrier to interference level ("C/I") that is 17.7 dB
above TEMPO‘s noise floor. Even if EchoStar operates with the lower EIRP of 87.4 dBW
suggested in its Technical Annex, the C/I level would still be 10.1 dB above TEMPO‘s noise
floor.

       In addition, other factors neglected by EchoStar must be considered to assess fully the
potential for harmful interference into TEMPO‘s system. For example, EchoStar‘s analysis fails
to make an allowance for naturally occurring satellite drift, which could result in only 0.1° of
physical separation between USABSS—3 and TEMPO‘s satellite.‘ EchoStar also has failed to
make an allowance for antenna mispointing, which must be considered in a worst case analysis
of interference pursuant to ITU Appendix 30A.


* TEMPO‘s satellite has an east—west station keeping of 0.1° and USABSS—3 has an east—west
station keeping of 0.05°. As a result, in order to determine if relocating USABSS—3 to 119.05°
W.L. could result in interference to TEMPO, a worst case spacing of 0.15° must be included in
any calculations.


Thomas S. Tycz
April 10, 1997
Page 3


       Second, EchoStar‘s analysis fails to consider the potential for interference from its
tracking carriers in its channels 1 and 2 into TEMPO‘s authorized telemetry operations. As
noted in the Technical Statement, the combination of EchoStar‘s tracking carriers and service
carriers could create intermodulation products that could interfere with TEMPO‘s telemetry
operations."
        Third, TEMPO has learned that Telesat Canada intends to locate an FSS satellite at
118.7° W.L., which would be operated in an inclined orbit, possibly as early as May 1997.5
EchoStar‘s Technical Annex does not consider the significant impact that location of an FSS
satellite just 0.1° away from TEMPO‘s and Directsat‘s authorized slot would have on the ability
to coordinate EchoStar‘s proposed operations with TEMPO‘s system.*

       Thus, TEMPO submits that EchoStar‘s Technical Annex fails to demonstrate that
EchoStar‘s proposed operations would not cause harmful interference into TEMPO‘s system.
This inadequacy is underscored by EchoStar‘s own long—standing position that a serious potential
for harmful interference exists between USABSS—3‘s operations at its existing authorized
position at 119.2° W.L. and TEMPO‘s system at 118.8° W.L. EchoStar has twice opposed
applications of TEMPO and its affiliate, Western Tele—Communications, Inc. ("WTCI"), for FCC
authorizations on the grounds that even the presently required 0.4° spacing may be insufficient to
prevent interference between EchoStar‘s and TEMPO‘s satellites.

       For example, as early as 1994, EchoStar argued that "interference at numerous
frequencies may occur" if TEMPO and EchoStar operate 0.4° apart.‘ In 1996, EchoStar repeated


* Because EchoStar‘s channel 2 tracking carrier and TEMPO‘s telemetry carrier are co—polarized,
the proposed relocation of USABSS—4 (with channel 2 service) to 118.95° does not eliminate the
potential for that satellite to interfere with TEMPO‘s operations.

* TEMPO understands that EchoStar has been informed of Telesat‘s intention.

° Telesat has proposed that TEMPO move its satellite to 118.95° W.L. in order to provide
Telesat‘s satellite with a deadband of 0.15°. As the Commission is aware, TEMPO was required
to design the shaped reflector for its satellite to serve Alaska while suppressing the signal
towards Siberia. Thus, it is unclear whether TEMPO could move its satellite to the West without
causing unauthorized transmissions into Siberia.

* See Letter from David K. Moskowitz, Vice President and General Counsel, EchoStar Satellite
Corporation, to William F. Caton, Acting Secretary, Federal Communications Commission, at
 10, dated Sept. 30, 1994. EchoStar indicated that 0.4° of spacing is insufficient between
                                                                                       (Continued...)


Thomas S. Tycz
April 10, 1997
Page 4


this argument in a petition to deny WTCI‘s earth station application because of EchoStar‘s
"serious interference concerns.‘""" EchoStar argued that even with 0.4° of separation, "EchoStar‘s
uppermost channel (21) is so close to TEMPO‘s lowermost channel (22) that TEMPO‘s
operations could easily cause interference . . .‘

        Moreover, as TEMPO has previously indicated, EchoStar acknowledged inits November
1995 technical submissions to the Commission that its system would cause "excessive
interference" to DBS systems operating at 119° W.L.‘* EchoStar disregarded the severity of this
interference, however, by incorrectly assuming that it is authorized to operate all 32 channels at
119° W.L. and thus the interference would be into its own system.‘



       (...Continued)
USABSS—3 and TEMPO‘s satellite because of the potential for both satellites to drift towards
each other. Taking the potential for drift into account, EchoStar stated that interference may
result at numerous frequencies. Id.
8




9


DRED/L.964t5(Oct 18, 1996). _
i     iti           i      formation                     inicati            Per:        e
Interference
 Includig Considerations, at unnumbered page 2, included
attachment Minor
             Conditions, Modification
Authority,
 Launch    FCC File No. 15—SAT—MP/LA—96 (Nov. 13, 1995) ("EchoStar Request for
Launch Authority"), also included as an attachment to Letter from Pantelis Michalopoulos,
Steptoe & Johnson LLP, to Giselle Gomez, Satellite Engineering Branch, FCC, dated Nov. 3,
1995 ("November 3rd Letter"); see also Western Tele—Communications, Inc.Opposition
toD
Petition eny, FCC File No. 1725—DSE—P/L—96, at 10 (Oct. 28, 1996).

‘ See Qutput Results From ‘MSPACE‘ Program for the Modified Input Data for the Beam
(ReducedEchoStar), at unnumbered pages 3—4, included as Attachment 3
to EchoStar Request for Launch Authority, also included as an attachment to November 3rd
Letter (disclosing excessive interference to channels 22—32 at 119° W.L., but indicating that
EchoStar‘s satellite would be the satellite operating channels 22—32); see also EchoStar DBS
TechnicalI
  Satel ite, nput, at 17 (Aug. 1994), included as an attachment to EchoStar Request for
Authority (excluding TEMPO‘s authorized channels at 119° W.L. from a list of
                                                                                     (Continued...)


Thomas S. Tycz
April 10, 1997
Page 5


       In light of EchoStar‘s past statements of concern, the Commission should view
EchoStar‘s Technical Annex in support of its request for STA with skepticism. Indeed, TEMPO
has shown that the annex is based on erroncous assumptions and fails to consider key factors that
could contribute to interference. Accordingly, EchoStar‘s showing is wholly inadequate to
demonstrate that the proposed operation of USABSS—3 from 119.05° W.L. would not cause
harmful interference to TEMPO‘s system at 118.8° W.L.

          Thank you for your attention to this matter. If you have any questions, please contact this
office.


                                                Rcspcctfullwmi-tted,




Enclosure

cc:       Kim Baum, Satellite and Radiocommunication
          Division, International Bureau, FCC
          Pantelis Michalopoulos, counsel to EchoStar
          Satellite Corporation and Directsat Corporation




          (...Continued)
authorized systems between 101.2° W.L. and 148.2° W.L. and incorrectly indicating that
EchoStar would be the sole operator at 119° W.L.).


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               TECHNICAL            STATEMENT         OF    TRMPO    SATELLI’I'E,      INC


      The following is an analysis of the Technical Annex filed by
      Echostar/Directsat on March 28, 1997.                          Echostar was directed
      to show that their system will not interfere into Tempo‘s
      system or other BSS satellites.                        For the reasons explained in
      the followihg analysis, Echostar has failed to satisfy this
      obligation.


      Facts         Important          to       the   Analysis


      A.        Authorized            nocations,           Polarization,           Channels,      and
      Station—keeping


      Echostar is authorizged to operate it‘s satellite USABSS—3 at
      119.2° WL using odd channels 1—21 with right hand—circular

       (RHC) polarization.                  Directsat‘s satellite USABSS—4 is
      authorized to operate at a location of 118.8° WL using even

      channels 2—20 with left—hand—circular (LHC) pola:iéation.
      ERchostar/Direcatsat are authorized to use +/— 0.05° R—W
      station—keeping.



      Tempo‘s satellite USABSS—~7 is authorized to operate at 118.8"°

      WL with even and odd channels 22—32 inclusive with LHC
      polarization on even chamnnels and RHC polarization on odd
      channels. Tempo is authorized to use +/— 0.10° E—W station—

      keeping.



      B.       TTU BSS          Plan for Feedaer             links    in the        17.3—17.8      GHz
      band          in Region 2


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      The BSS plan for feeder links to BSS satellites is defined in
      Appendix 30A to Orb 88 of the ITU radio regulations.                         The
      Feeder link is the seqment between the uplink earth station
      on the ground and the associated receiving satellite space
      station.


      Appendix. 30A and Technical                      Characteristics méx 3


      Annex 3 to Appendix 30A contains theprogédures and
      calcularions to be used to deteminé.} J.f v]:_g%apcsled changes to
      the plan will cause harmful interference.                      The Region 2
      technical characteristics are contained within Section 4 of
      Annex 3. Article 9 to Appendix 30A contains the plan tables
      for Region 2 that define each channel, the various beams,
      orbital locations, and polarization.                   These sections include
      all the necessary parameters to properly determine the
      porential for interference.


      Plan for Feeder links in the 17.3—17.8 GHz band in
      Region 2           using haam USAEHOON4                           i


      The satellites operated by Echostar, Directsat and Tempo
      share the cluster centered at 119° WL. The ITU Radio
      Requlations include a diagram that shows the geometry for
      clusters of the plan‘s BSS satellites. See ITU Radio
      Reqgulations Appendix 30A¥ Fiqure 9 on page 245.                       Allowances
       for E—W station—keeping,                  satellite spacing between cross—
      polarized satellites, feeder link antenna mis—pointing, and
      the pattern of the reference antenna is also shown.



      The plan defines the applicable beam for the cluster at 119°

      WL as USAEHOO4.                This has an orbit of 119.2° with polarization
      RHC for odd channels 1 to 31.                    The beam USAFEHOO4 also has an


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      orbit of 118.8° for the even channels 2 to 32 with
      polarization LHC.                Therefore,   the plan specifies a separation
      of 0.4° between cross—polarized channels in a Cluster.                       See

      ITU Radio Requlations section 4.:.13 of Annex 3.


      Uplink EIRP is defined in all beams and channels as a maximum
      level of 87.4 a@BW at the ground.                The plan also reduires a
      minimum antenna size of 5 meters, with m%spointing of the
      antenna +/— 0.1° maximum with mispoihéifié%allowanée’of 1;§B or
      less.



      Tempo and Echostar/Directsat have filed characteristics with
      the FCC for Appendix 30A on their receiving space stations
      and feeder link earth stations.                 These parameters include
      antenna patterns, service area, known feeder link earth
      station parameters, typical feeder link earth station
      parameters, service areas and test points.


      These and the other parsameters in the plan should be used to
      determine potential interference with the applicable test
      points for each DBS system over the ‘applicable service area.


      ¢.        Echostar/Directgzat            Proposed Change        in Satellite
      Locations and Reduction in the Orbital Spacing

      Echostar and Directsat propose to change their orhiftal
      locations, therehy reducing the separation between Echostar‘s
      satellite and Tempo‘s satellite.                  Echostar proposes to
      operate it‘s satellite USABSS—3 at 119.05° WL using odd
      channels 1—21 with RHC polarization. Directsat proposes to
      operate USABSS—4 at 118.95"° WL with even channels 2—20 with

      LIHC polarization.               Tempo‘s satellite USABSS—7 would remain at


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      118.8° WL using even and odd channels 32—32 inclusive with LHC

      polarization on even channels and RHC polarization on odd
      channels.


      Orbltal spacing on odd channels between Echostar and aven

      whannels on Tempo would, thersafors, be reduced to 0.25° from

      the Region Z% plan‘s requirement of 0.40° separation



     D.        Evaluatlion of               the     Calculutiéfi‘£5§nab           and
      Parametars             contained in the Technical Annex by
      Rchostar



      Echostar‘s Technical Annex evaluated the interference
     potential into Tempo only on the basis of EIRP and cross—
      polarization isolation, without regard for consi&eration of
      all variables specified in Annex 3 of the Region 2 plan.                                     In
      fact,         the analysis only includes values for EIRP,                    cross—
      polaization iselation, and a value for a bandwidth factor. To
      compound the problem,                      the analysis uses incorrect values for
      EIRP and cross—polarization.                      Also. the bandwidth factor is
      not recognized in the plan.


      Additionally, Echostar‘s calculation refers to a level of
      carrier—to—interference C/I, but does not compare this C/I
      level to the satellite station receiver input,                             aé requirsa in
      the plan. Appendix 30A section 1.7 of Annex 3. This
      reference level is required to evaluate it for interference.


      Rchostar used the following formula in it‘s Technical Amnnex:



               C/ITfemps = ELIRPTempo — EIRPrEchostar + XPD(O)               + Foverlap


Armmivoad   a4eui    T OM i1 ELCEUOUMMUNICALTLUNG                 13044883890
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      Echostar‘s formula definitions include errors as well.


      XPD(O) The cross—polarigzed isolation of the transmitting
      antemnna is a factor of cross—polarization, but the value is
      not equal to 30 dB, as Echostar states. This should be
      calculated as follows:


      Using the formulas for Fiqgure 6 on page 234 of Appendlx 3OA,
      with the antenna 0.235° off—axis, the cross-polarlzatlon '
      ilsolation = 27.0 dB.. Note that in it‘s Technlcal Aannex,
      Echostar refers to the ITU pattern defined in Figure 6 as
      it‘s uplink antenna pattern.


      Secondly, the cross—polarization isolation of the satellite
      receiving antenna must be included.                       Tempo‘s satellite
      receive antenna provides 30 daB cross—polariz:ation isolation.


      The combined isolation of the two antennas in the feeder link



      = 10 log (1/((log—1(—27/10}))+({log—1i(—30/10})}}) This combined
      isolation equals an amount of only 25.3 dB and this should be
      used in calculations.


      EIRP          factors used in the Echostar Calculations


      RLREYempo            The EIRP clear—sky licenged by Tempo for it‘s known
      feeder link earth stations and the EIRP for typical feeder
      link earth stations with Tempo‘s service area has been
      clearly provided in it‘s Appendix 30A filing or in the earth
      station license(s).                       For the known feeder link earth station
      in Littleton,               Colorado,         the EIRP is an amount of 80.0 dBW and
      a monopulse tracking antenmna of 13.im is used.                           For typical
      earth stations within Tempo‘s service area, as defined in the


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      Appendix 30A filing, the EIRP is an amount of up to 87.4 dBW,
      using a 5m or larger antenna without tracking.                    It is
       important to noate that these levels are consistent with the
       FCC rules under CFR 47 part 25.204 d.              This specifies the
       lowest power level that will provide the required signal
       cquality be used.


       For a typical feeder link station at the eadge of Tempo‘s
       service area, such as in Anchorage, Alaska, the G/T in the
       Tempo satellite is reduced 6 dB to a level of —4 daB/k.                     This
       station also has higher path losses . Theéefore, to maintain
       the required siqgnal quality from this station,                  the EIRP would
       be increaged to 87.4 dBW, the plan maximum.


       EIRPuchostar             The EIRP clear—sky licensed by Echostar is
       provided in it‘s earth station license at a level of 95.0
       daBW.          It is important to note that this level is in excess of
       the power level that will provide the required signal
       cquality.           See FCC rules under CFR 47 part 25.204 d.


       In it‘s latest ITU filing dated November 13, 1995 Echostar
       indicated an EIRP substantlally lower, an amount of 75.6 dBW
       clear—sky for it‘s service. This parameter is consistent with
       CFR 47 part 25,.204 d and e.


       In the Technical Annex, however,              Echostar indicated a new
       clear—sky RIRP of 87.4 dBW                                  ‘


       Foverlap         The plan for Region 2 does not recognize the use of a
       bandwidth factor such as the one utilized by Echostar,
       thereforse it is not sppropriate to include it.


       Calculation format of Feeder Link Upiink Thermal C/N


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      As noted previously, Echostar‘s calculation did not reference
      the C/I to the satellite receive system as required.                        The
      caloulation for uplink thermal C/N is as follows:



      Uplink thermal C/N (dB)                   EIRP at feeder link site (dB)
      —Dispersion loss in path to satellité (a@B/m*"3)})                     —Isotropic
      Area at uplink frequency (dB—m*"2)                —Noise Bandwidath of 24 MHz
      channel (dB—Hz) —~Boltzsmann‘s Constant (dB/K—Hz)}) +G/T of
      satellite for uplink location (dB) fihntenna mispointing (dB) .


      Uplink thermal for Littleton, Colorado = 80.0 —162.5 —46.3
      —73.8 —(—228.68) +2.0 —0.1 = 27.9 aB.

      Uplink thermal for Anchorage, Alaska = §7.4 —163.0 —46.3
      —73.8 —(~—2%8.6)}           —4.0 —1.0 = 27.9 aB.



      E.        Evaluation of             the   formula provided by Echostar
      uging          the   Revised        Parameters   above


      The Echostar interference potential into Tempo is
      siqnificantly higher than Echostar‘s caculations would lead
      us to beliave, hased on their formula.


      Using the licensed EIRP of Tempo‘s system in Littleton,
      Colorado and the licensed EIRP of Rchostar‘s system in
      Cheyenne, Wyoming, plus the correct cross—polarized isolation
      the value of C/I = 80.0 —95.0 +2325.2 = 10.3 dB C/I.                       This
      level is 17.7 dB above Tempo‘s noise floor.                        This is 19.8 dB
      from the objective of 30 dB C/I claimed by Echostar in the
      Technical Annex.


      Using the licensed EIRP of Tempo‘s system in Littleton,
      Colorado and the EIRP of 87.4 dBW proposed by Echostar in the
      Technical Annex, plus the correct cross—polarigzed isolation,


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      the value of C/f = 80.0 —87.4 +25.2 = 17.8 dB C/I.                          This
      level is 10.1 dB above Tempo‘s noise floeor.                        This is 12.2 dB
      from the objective of 30 dB C/I claimed by Echostar in the
      Technical Annex.


      Calculation presented                     by   Echastar   evaluated       at     a
      fringe Tempo earth station in aAnchorage,                               Alaska


      A calculation based on the plan parameters with EIRP for
      Tempo’s fringe sarth station in Anchorage, Alaska,                         compared
      to the EIRP proposed in the Technical Annex by Echostar
      follows. This calculation uses the corrected cross—polarized
      isolation. — An adjustment for the satellite G/T, equal to the
      amount of +2.0 dB/K effective at the interfering earth
      station location and a value of —4.0 dB/K effective in
      Anchorage, equals a reduction in the C/I ratio of —6.0 aB.


      The value of C/I to the uplink from Anchorage = 8§7.4 —~87.4
      +25.2 —6,.0 = 19.2 dB C/I. This level is 8.7 dB above Tempo‘s
      noise floor. This is10.8 dB from the objective of 30 aB C/I
      claimed by-Echostar in the Technical Annéx.                         Note that Tempo
      cannot raise the EIRP in this confiquration, as was suggested
      by Echostar in the Technical Annex, since it already uses the
      plan maximum.'


      Summary regarding                    the Adequacy    of    the     Calculations


      Note that these calculations do not account for all worst
       case analysis recquirements in the plan.                     Addition of these
       could be expected to further reduce the isolation.                            Also note
       the calculations above do not include the benefit of off—axis
       antenna isolation based on orbital spacing between the
       systems .        The calculations also do not include the benefits


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       of Echostar using similar EIRP levels to that planned for
       Tempo.


       In summary,         the calculations herein show the inadequacy of
       the calculations provided in Echostar‘s Technical Annex.


       E.   Additional Facts Applicable to the Analysis of
       Echostar/Directsat and Tempo



       Other factors affect the potential of interference into Tempo
       from Echostar, especially considering the reduced spacing
       proposed. Other factors that concern the location of
       Directsat‘s satellite must also be evaluated


       1.     TTAC usgsed by Temps and the Trackung carrier in Echostar‘s
       channel 1——Reduced spacing between Echostar‘s satellite and
       Tempo‘s satellite also reduces the isolation between
       Echostar‘s channel 1 and                  Tempo‘s Tracking, Telemetry and
       control       (TTAC) that is cross—polarized with LHC fiolarization
       at 12201—12204 MHz.                  Tempo is concerned about intermodulation
       products that may fall into Tempo‘s TTAC from mixing of
       Echostars‘s tracking carrier with the service carrier in
       transponder 1.              Tempo‘s TTPAC has a minimum EIRP worst case of
       +3 dBW with LHC palarization at thefedgerof—coverage.


       2.     TTAC used by Tempo and the tracking carrier in
       Directsat‘s channel 2——Mixing of the tracking carrier in
       Directsat‘s channel 2 with the service carrier in channel 2
       in the LHC polarized satellite may interfere with the Tempo
       TTAC telemetry with LHC polarization at 12201—12204 MHz. This
       is still potentially a problem, even thdugh Directsat‘s
       satellite is proposed to move West from Tempo‘s (118§.8° WL to


arit=iu~gi0   i4.iug   oFfOMi1GLGCUMMUNIUGALIUNS                 (EREECERCET]    T=73?f?    P.1/12   som=g07




       118.95° WL),. because Directsat‘s uplink and downlink are co—

       polarized with Tempo‘s LHC TTAC.


       3.      Channel 30 used by Directsat interfering with Tempo‘s
       channel 22——The potential of Echostar‘s channel 20
        interfering into Tempo‘s channel 22 is significant if
       Echostar uses the very high EIRP proposed and licensed.                             The
       plan requires this channel also be evaluated.


        4.     Station—keeping between systems--Theffiaordination that
       will be required on an on—going basis, necessary between
       Echostar‘s operator Loral Skynet.                    and Tempo‘s operator GK
       Americom, will be increased if Directsat‘s satellite and
       Tempo‘s satellite will have overlaping E—W station—keeping
       deadbands.             Echostar and Directsat have indicated to the FPCC
        they will use +/— 0.05° E—W station—keeping. Tempo will use

        +/= 0.10° E—W station—keeping.


       Telesat Canada has made a recent request to place Anik Cl and
        a future Anik F, or move an existing Anik BE series hybrid
        satellite, to 118.7° WLh.                  The Anik C1 satellite would operate

        inclined up to 2Adegrees N—S (4 degrees peak—~to—peak) .
        Inclination of this satellite will require more E—W spacing.
        Telesat has requested Tempo to use 118 .95° WL and

        Directsat/Echostar to use orbits as far West of this as
       possible (119.1° and 119.2° WL). It is clear that some
        isolation from this satellite may be necessary.



        Tempo has designed it‘s shapad transmit reflectors for 118.8°

        WL to suppress Siberia and cover Alaska,                     in accordance to a
        request from the FCC, fully in accordance with Appendix 30 of
        the Orb 85 plan.                 Tempo is uncertain how much movement West


                                                       10


ArR~iu=gi   i4104   rCOMiGRLECUMMUNIGATIUNS                  13034863890    T—?3?   P.12/12   Job—807




      can be made in it‘s satellite from 118 .8"° WL for this reason.

      This complicates the orbital coordination issues between
      Tempo and Echostar even further.



                      o     the          lysg i a



      Echostar‘s calculation is not in conformance with the
      calculation format spec1f1ed in Appendix 30A (Orb 88)                 to the
      ITU regulations.               In Appendix 30A, the petentlal of _
      interference is evaluated on the bas;s ofan OBPM (overall
      equivalent protection margin)} as defined in Annex 3.                 The
      calculations provided by Echostar in the Technical Annex
      filed March 28, 1997 have been shown herein to be inadequate.
      Additionally, Tempo has shown that other unresolved issues
      exist that are affected by the orbital locations of USABSS—3
      and USABSS—4 as well.




      Siqnatura                   TMeC.._t4/16 /47
               Gary        Q%éiue, Pirector,        Satellite Serv1ces,
               TCLI        chnology Ventures,         Inc for Tempo Satellite,   Inc.
               4100 E. Dry Creek Road,              Littleton, CO 80132




                                                     11



Document Created: 2016-11-16 16:59:33
Document Modified: 2016-11-16 16:59:33

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