Attachment Technical Analysis

This document pretains to SES-MOD-20160108-00029 for Modification on a Satellite Earth Station filing.

IBFS_SESMOD2016010800029_1121018

                                       Technical Analysis

ViaSat submits the following showing to demonstrate that the operation of the aeronautical earth
station under Call Sign E120075 in the 28.1-28.35 GHz band segment will not cause harmful
interference to existing or future LMDS stations.

The antenna of the earth station is installed on a fuselage mount on top of an aircraft using an
approved mounting method that includes a faring adaptor ring and a radome to protect the
antenna from the high wind forces in flight.

Locating the antenna on the top of the aircraft fuselage provides blockage of the signal toward
the ground from the fuselage of the aircraft, the wings and horizontal stabilizers, and the faring
mounting ring for the radome. The attenuation from blockage varies with respect to the
downward angle to the LMDS station on the ground and in this analysis is conservatively
estimated as 20 dB, even though the blockage value would increase to higher values as the
downward angle toward the LMDS user station increases when the aircraft gets closer to the
LMDS site.

ViaSat conducted a technical analysis to determine the potential level of an interfering signal
received from an aircraft earth station at a LMDS station, assuming operation at both 10,000 ft
and at 35,000 ft. Because no sharing criteria exist, ViaSat relied on research available in
technical papers discussing LMDS systems and link budgets, 1 and also obtained LMDS
equipment specifications from a major LMDS equipment manufacturer. 2

Based on the available research, ViaSat selected a ΔT/T of 6% as the basis for calculating the
threshold I/N ratio of -12.2 dB, which corresponds to an effective increase to the LMDS
receiver’s noise floor of 0.27 dB. As detailed below, even under a worst-case analysis (direct
azimuth alignment), the resulting ΔT/T would be well under 1%. 3

Notably, the potential interference case presented in this analysis is based on the same
assumptions for LMDS operational parameters and interference thresholds that ViaSat utilized in
its applications for sixteen earth stations at fixed locations that operate in the 28.1-28.35 GHz
frequencies, all of which were approved by the Commission,4 and all of which have been

1
       Robert Duhamel, “Local Multipoint Distribution Service (LMDS) Cell Sizing and
       Availability,” IEEE P802.16 Broadband Wireless Access Working Group (June 9, 1999),
       available at http://wirelessman.org/sysreq/contributions/80216sc-99_17.pdf.
2
       DragonWave Packet Microwave Systems, Product Link:
       http://www.dragonwaveinc.com/products-wireless-ethernet.asp.
3
       These levels are used to illustrate are the lack of any impact on LMDS from the proposed
       aeronautical earth stations; they are not assumed to be, and should not be construed as, an
       admission about what level of unwanted emissions would conceivably constitute
       “harmful interference” into an LMDS facility.
4
       The following secondary earth station authorizations were granted October 21, 2011
       based on showings on compatibility with LMDS operations in the 28.1-28.35 GHz band
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operating for almost four years without any reports of interference with respect to LMDS
operations.

The analysis considered both hub-type and user-type LMDS stations. The higher antenna gain
and better receiving performance of the user-type LMDS stations make these stations more
sensitive than the hub-type stations, and thus, more susceptible to potential interference.

Table 1 and Table 2 consider the worst-case scenario, which results when the earth station and
the LMDS station are directly aligned in the azimuth. This occurs when the LMDS hub-type
station is located directly between the aircraft and the LMDS user-type station and when the
aircraft is north east of the two LMDS stations as depicted in Figure 1 and Figure 5. In this case,
the LMDS user-type station’s antenna is pointing directly towards the antenna on the aircraft in
the horizontal, or azimuth, plane. However, due to the difference in elevation between the
stations, there is always some misalignment of the LMDS user-type station’s antenna with the
earth station antenna on the aircraft in the elevation plane. In other words, the earth station
antenna points up toward the satellite while the LMDS user-type station antenna points along the
ground toward the LMDS hub-type station, which results in less unwanted energy being received
by the LMDS station than if they were on the same elevation plane.

Because the worst-case analysis (direct azimuth alignment) does not present a problem for the
LMDS user-type station, it also does not present a problem for the LMDS-hub-type stations;
only the results of the analysis of the LMDS user stations are presented here.

The analysis assumes the LMDS user terminal has the characteristics listed in the technical
specifications provided for sample LMDS equipment.




       segment: ViaSat, Inc., File Nos. SES-LIC-20110211-00150 (E110015); SES-LIC-
       20110228-00212 (Call Sign E110026); File Nos. SES-LIC-20110318-00318 (Call Sign
       E110033); SES-LIC-20110318-00323 (Call Sign E110036); SES-LIC-20110328-00373
       (Call Sign E110043); SES-LIC-20110328-00374 (Call Sign E110044); SES-LIC-
       20110328-00375 (Call Sign E110045); SES-LIC-20110328-00376 (Call Sign E110046);
       SES-LIC-20110328-00378 (Call Sign E110047); SES-LIC-20110328-00379 (Call Sign
       E110048); SES-LIC-20110328-00380 (Call Sign E110049); SES-LIC-20110328-00381
       (Call Sign E110050); SES-LIC-20110328-00382 (Call Sign E110051); SES-LIC-
       20110328-00383 (Call Sign E110052); SES-LIC-20110418-00474 (Call Sign E110064);
       SES-LIC-20110419-00488 (Call Sign E110065).
                                                 2


     Table 1 System Parameters and Results for Direct Azimuth Alignment at 35,000 ft

The results in Table 1 for an aeronautical earth station operating at 35,000 ft indicate that, in a
direct azimuth alignment case, the undesired signal from the aeronautical station would be
received at 45 dB below the thermal noise floor of the LMDS user terminal and thus, well below
the I/N threshold of -12.2 dB. In the case of operation at 10,000 ft, in a direct azimuth alignment
case, the undesired signal would be received 24 dB below the thermal noise floor of the LMDS
user terminal and still well below the I/N threshold. A direct azimuth alignment case represents
the worst-case interference scenario, and even that worst-case scenario is likely to occur only on
a fleeting basis, given the speed at which aircraft typically operate at these altitudes. Given the
large margin under the thermal noise floor in each of these scenarios, ViaSat’s proposed
operations would not cause harmful interference to any LMDS users.




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     Table 2 System Parameters and Results for Direct Azimuth Alignment at 10,000 ft

ViaSat conducted simulations using Visualyse software to perform an area analysis to verify the
analytical results in the tables above. The Visualyse simulations determine the level of unwanted
energy received by an LMDS user terminal at all locations surrounding the user terminal given
the LMDS hub location. The location of the LMDS hub terminal with respect to the LMDS user
terminal drives the pointing direction of the user terminal.

The Visualyse software does not have a parameter to enter airframe blockage toward the ground.
To simulate airframe blockage during the area analysis, the input power to the antenna was
adjusted downward by static value of 20 dB, even though the blockage value would increase to
higher values as the downward angle toward the LMDS user station increases when the aircraft
gets closer to the LMDS site. However, even without the full blockage effect included in the
area analysis, the results still indicate an acceptable I/N at areas near the LMDS user terminal.

In the area analysis, the aeronautical earth station is moved in small steps to each location within
the area, and the analysis is performed in successive iterations with the results recorded
                                                 4


internally within Visualyse. Using these recorded results, Visualyse generates the figures shown
below to illustrate the contour boundaries for various I/N levels for the LMDS system. The
results compare well with the value in Table 1 and indicate a worst case I/N of -45 dB within the
area analysis region during operation at 35,000 ft. When operating at 10,000 ft, a worst case I/N
of -22 dB was observed.

These results are consistent with the values in Table 1 and Table 2 above and indicate an
acceptable I/N at areas near the LMDS user terminal in all cases.

The following figures represent various alignments of the aeronautical earth station to the LMDS
hub and user terminal that were evaluated. In most cases, there will be no alignment at all that
needs to be considered as a potential interference case. For instance, (i) Figure 1 depicts the case
where the LMDS hub terminal is North East of the LMDS user terminal and the user terminal
pointing most directly towards the aeronautical earth station is more likely to receive unwanted
energy than when facing other directions, (ii) Figures 2, 3 and 4 depict cases where the LMDS
user terminal and the aeronautical earth station simply are not aligned in the azimuth plane.




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Figure 1: Aeronautical Earth Station at 35,000 ft - LMDS Hub NE of UT




                                 6


Figure 2: Aeronautical Earth Station at 35,000 ft - LMDS Hub NE of UT




                                 7


Figure 3 Aeronautical Earth Station at 35,000 ft – LMDS Hub SW of UT




                                 8


Figure 4 Aeronautical Earth Station at 35,000 ft – LMDS Hub SE of UT




                                 9


Figure 5 Aeronautical Earth Station at 10,000 ft – LMDS Hub NE of UT




                                10


Figure 6 Aeronautical Earth Station at 10,000 ft – LMDS Hub NW of UT




                                11


Figure 7 Aeronautical Earth Station at 10,000 ft – LMDS Hub SW of UT




                                12


Figure 8 Aeronautical Earth Station at 10,000 ft – LMDS Hub SE of UT




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Document Created: 2016-01-08 09:56:38
Document Modified: 2016-01-08 09:56:38

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