Attachment ASC-9 4m Product Des

ASC-9 4m Product Des

SUPPLEMENT submitted by Ryan N. Terry

Product Description

2015-12-21

This document pretains to SES-LIC-20151016-00712 for License on a Satellite Earth Station filing.

IBFS_SESLIC2015101600712_1119423

         9.4M KA ESA
EXTENDED PRODUCT DESCRIPTION


                 ASC Signal

       1120 Jupiter Road, Suite 102
          Plano, TX 75074-3521

          Phone: 214-291-7608
           Fax: 214-291-7655




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1.1       Antenna Subsystem

1.1.1 9.4m Antenna Subsystem

The ASC Signal 9.4 meter antenna was designed and introduced to the satellite
communications industry over 10 years ago. It has been in production ever since primarily
filling the requirements of the C-band to K-band satellite communications market. Prompted
by demanding commercial and military requirements, ASC Signal designed and introduced a
series of high precision mount designs specifically meant to address large aperture, Ka-Band
Gateway earth station applications. The 9.4m antenna design combined with the extended
azimuth dual drive precision mount and patented 3 axis subreflector tracker (SRT) technology
provide an extremely versatile and reliable gateway antenna solution. Knowing that the
ultimate goal of any Ka-band gateway terminal is maximum link availability, the 9.4m design
provides the operator with the industry’s best feature set available to combat the unique
challenges of Ka-band operation.

         Precision stretch formed reflector skins
         Thermally matched all-aluminum reflector construction
         Specially optimized reflector heater systems
         Extended azimuth/hi wind dual drive mount with 26 bit high precision encoders
         Patented (U.S. patent 6,943,750) 3-axis SRT tracking system with adaptive thermal
          compensation
         NGC 6-axis antenna control with redundant positioning/tracking systems
         All forms of pointing/tracking algorithms available:
               o Ephemeris (INTELSAT, NORAD)
               o Step Track with patented 3 point peaking
               o SmartTrack (Model Track)
               o Monopulse

The primary satellite tracking function is accomplished via small mechanical movements of
the subreflector tracking (SRT) assembly. This tracking scheme provides precision satellite
tracking over a +/- 0.25 degree range while the main pedestal is in a static/fixed condition.
This approach increases operational life and extends time between routine maintenance
intervals. The mount motion is primarily utilized to reposition the antenna over >200 degree
azimuth range but can also be used as a backup tracking system in case of SRT failure. The
antenna control system (based on the ASC Signal NGC controller) commands both the SRT
system and the pedestal mount motor drives.

The 9.4m SRT also incorporates a thermal compensation feature that is unique in the
industry. Substantial data is available that shows thermally induced reflector distortions
dramatically impact the antenna performance for large high frequency structures like the
9.4m. Reflector and mount distortions induced by the sun and anti-ice heater operation will
alter beam pointing angles and reduce antenna gain (de-focusing). Beam deflections will
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automatically be negated while in step track mode. However, the ASC Signal SRT also
incorporates a precision z-axis drive mechanism that adaptively re-focuses the antenna
system and maintains optimal performance through all weather and anti-ice events.

1.1.2 Antenna RF Description and Performance
The 9.4m optical design has been optimized for high efficiency Ka-band performance and
providing compliance to all applicable regulatory requirements. The 9.4 Meter Ka-Band
antenna is fully compliant (as a minimum) with the following referenced Regulatory Agency
specifications:

      Federal Communications Commission Rules and Regulations, Title 47, C.F.R. Part
       25.209, as amended.
      ITU-R, S.580-5 and S.465-5 Recommendations for Pattern Performance for 2 degree
       satellite spacing, as amended

Specifically, the proposed antenna complies with the radiation pattern envelope (RPE)
performance for 1 - 180 degrees angles as per ITU-R, S.580-5, S.465-5, and FCC part 25:


Transmit pattern curve
                     29-25 LOG  dBi (1º    20)
                     -3.5 dBi (20<   26.3)
                     32-25 LOG  dBi (26.3<   48)
                     -10 dBi ( > 48)

Transmit pattern sidelobe excursions

                     No excursions for 1º   7
                     3dB max excursions for  > 7
                     10% max integr. excursions for 7<   180


Examples of transmit and receive band antenna patterns are shown on the following pages:




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FIGURE 1 ANTENNA PATTERN AT 19.25 GHZ, NARROW CUT




 FIGURE 2 ANTENNA PATTERN AT 19.25 GHZ, WIDE CUT




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FIGURE 3 ANTENNA PATTERN AT 28.35 GHZ, NARROW CUT




 FIGURE 4 ANTENNA PATTERN AT 28.75 GHZ, WIDE CUT




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The 9.4m antenna proposed is supplied with a wideband 4-port feed that supports the entire
operational bandwidth of the satellite system as well as provides access to all polarizations.
The complete RF performance data sheet for the 9.4m Ka-band antenna is given in the
attached feed Specification (represented in Table 1 below);




                                TABLE 1 RF-4CPWWKA-94-206




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1.1.3 Unique 9.4m Features

The 9.4m incorporates a industry unique very reliable, low maintenance, low cost and low
power consumption tracking mechanism that exploits the fact that next generation Ka-Band
spot beam satellites must maintain their orbital positions within a small orbital box. For these
satellites, accurate station keeping is a necessity in order to keep the multiple tiny spot beams
from wandering about, which would cause cross-beam interference and beam edge level
degradation.

The ASC Signal Subreflector Tracking (SRT) technology exploits the small orbital box size, by
positioning the antenna’s main beam constantly toward the satellite by using small controlled
movements of the subreflector. This technique can be used when the satellite’s AZ/EL
pointing angles don’t migrate “off axis” from the antenna’s mechanical axis by more than
three antenna beam widths during tracking. For a 9.4M, at 29 GHz, that translates to ± 0.22
degrees. With the tracking scan angle limited to within this range, there are negligible scan
losses, and the cross polarization isolation and the off axis radiation pattern envelope
performance remain within all regulatory compliance specifications.

It is important to note that should SRT mechanism fail, the tracking controller in the ASC
proposed system will automatically default back to pedestal drive motion to continue with
the tracking operation.




                        FIGURE 5 KA-BAND GATEWAY ANTENNA WITH 3-AXIS SRT
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The ASC Signal 3-axis SRT assembly depicted in Figure 6 above can efficiently track through
beam deflections AND adaptively compensate for antenna de-focusing due to antenna
heating from de-ice and solar exposure.




                FIGURE 6 MEASURED REFLECTOR DISTORTIONS DUE TO THERMAL LOADING

Figure 7 shows actual measured data (infrared photo left, surface distortions right) of a
reflector during afternoon sun induced heating. The vertical scale on the distortion plot is
approximately 3 mm peak to peak.




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                     FIGURE 7 EFFECT OF 3-AXIS SRT THERMAL COMPENSATION

Fig 8 shows the antenna performance impact of the 3-axis SRT at Ka-Band. The plot shows an
antenna pattern (in black) distorted by sun induced thermal distortions. There is evidence of
both a mechanical bias (beam steer) and reflector de-focusing. With the 3-axis tracking
engaged (blue), the antenna performance is much improved. Without the adaptive
refocusing, these results indicate an uplink (30 GHz) loss in the order of 1 dB or more would
occur. A complete description of the 9.4m capabilities along with a complete report on
measured distortion and SRT tracking compensation data is available upon request.




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1.1.4 Mechanical Description and Performance
The extended azimuth galvanized pedestal mount assembly provides antenna positioning
ranges that easily comply with the most program operational requirements. The mount
incorporates variable speed dual drives in both axes that provide the necessary stiffness to
maintain accurate antenna pointing in high wind conditions.

The 9.4m antenna mechanical design is based on time proven, fielded technology. Established
finite element modeling methods backed up by decades of installation experience form the
basis of this optimized construction. A similar gateway antenna construction is shown figure
9. Table 3 is a list of some of the key features and performance specifications of the 9.4m
antenna and pedestal construction.


Optical Design              Symmetric Gregorian Dual Reflector
Reflector Panels            Precision stretch formed aluminum
Backstructure               Precision thermally matched aluminum
                            Stress-free 2 piece rib construction
                            Precision eccentric cam adjustment

Reflector Segments          20
Mount Type                  Pedestal, Hot dip galvanized steel
Travel Range (continuous)
                                 o
  Azimuth                   >200
                             o      o
  Elevation                 0 to 90
Hub/enclosure dimensions
  Depth                     46”
  Diameter                  84”
                               o       o
Operating Temperature       -40 to 125 F
Seismic                     Richter 8.3 or Grade 11
Wind Loading, Survival      125 MPH any position


              TABLE 2 9.4M EARTH STATION ANTENNA                         FIGURE 8 ASC GATEWAY ESA



The pedestal position drive system incorporates dual opposing gear motors with brakes for
precision antibacklash motion and high strength antenna hold performance. The elevation
drive consists of mechanically linked dual jack screws for structural stability and low backlash
characteristics. The ability to manually reposition the antenna with a handcrank is available
for both axes. A close up of the Azimuth drive system is shown in Figure 10.




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                               FIGURE 9 VIEW OF AZIMUTH DRIVE

All ASC antenna constructions utilize galvanized steel, stainless steel and painted aluminum
components for superior corrosion resistance and durability. The large maintenance platform
provides substantial room for multiple personnel during troubleshooting and maintenance
operations and allows access to the antenna hub enclosure even when the antenna is
positioned at zenith.

Swept antenna volume drawings shown in Fig. A2.8 and A2.9 incorporate several additional
features proposed for the configuration. Note the platform stairway and hub enclosure
access door.

ASC also supplies foundation loading requirements and typical foundation drawings. An
example foundation specification in shown in Fig. A2.10.

For the typical configuration, ASC has added several features specifically requested. The
outline drawing shown in Fig. A2.7 depicts an access ladder and hub rollup door.

1.1.5 Hub Integration

Figures A2.5 and A2.6 show preliminary internal hub layouts with the following major
electronics:

       Transmit Power Amplifier subsystem
       Low Noise Amplifier subsystem
       Transmit Block Upconverter subsystem
       Receive Block Down Converter subsystem
       Ka/L band frequency converters for Signal Monitoring, Tx Carrier Monitoring and
        Monopulse Tracking
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Other ancillary components listed below will be strategically positioned inside the Hub:

       10 MHz (passive) distribution subsystem (splitters)
       Tracking LNB, Plate and Block Down Converter
       Signal monitoring RF switch matrix and L-band relay switches

Several access points, space for CFE (Noise Source), test panels and power outlets for testing
by the Customer’s technical staff will be provided.

Placement of the major subsystem and components is optimized to meet the following
objectives:

    1. Shortest possible path length for RF connections to minimize loss, with priority given
       to traffic signal paths, followed by monitoring signal paths
    2. Logical grouping
    3. Accessibility for maintenance and testing

All internal Hub cable connections, i.e. L-band signals (for traffic, signal monitoring and
tracking), 10 MHz reference distribution cables, data communication for control and
management (coax, multiconductor or fiber optic) will use internal jumper cables. These will
interface at one or more Cable Interconnect Panels inside the hub with the outside IFL cables.
The latter are routed through cable access openings below the door, which are weather
protected using rubber boots.


1.1.6 Antenna Tracking System

1.1.6.1 Summary
The 9.4m antenna design, when combined with the extended azimuth precision dual drive
mount and ASC Signal’s patented 3-axis subreflector tracker (SRT) technology, provides an
extremely versatile and reliable overall gateway antenna solution. The tracking system block
diagram shows the basic tracking system (Monopulse) needed for this configuration. This
industry unique setup lends itself to also be used to track satellite motions by a variety of
other methods. The ASC Signal NGC controller allows for all traditional tracking methods
including, but not limited to:

       Ephemeris track (INTELSAT, NORAD, etc)
       Step Track with patented 3 point peaking
       SmartTrack (Predictive Model Track)
       Traditional Monopulse track


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The following diagram shows a simplified schematic diagram of the tracking control system.

                                                                                                                    Heat




                                                                                                                                      Wind
                                                                                                                  SRT



                                          Comm                         TE21 Mode
                                   LNA               OMT
                                                                        Coupler


                                                                                                                   Not Seen

                                          Error
                                   LNA                                Comparator                                 Encoder

                                                                                                                   Seen
                                                              Antenna Feed
         Down        Down
       Converter                         10 MHz                                                         Motor
                   Converter
                                                                                                        Drive
                                                                                            Position             CMD

    Comm IF             Error IF                                                                                           CMD
                                                                                                       NGC-ODU
                                                                                                                           Position

                                                                             Error Vector
                                                  Tracking Receiver                                    NGC-IDU
                                                                             Signal Level

                                    Comm IF



                                     ASC Signal SRT based Monopulse Block Diagram


                                         FIGURE 10 TRACKING SYSTEM CONTROL

As shown in the block diagram, the ASC Signal tracking system can be used to operate the
traditional mount motion drives, AND/OR our patented 3-axis subreflector tracking (SRT)
subsystem using a single control system.

The SRT provides a fast, extremely accurate antenna beam steering system, and importantly
allows for tracking with significantly reduced mechanical drive wear and maintenance (since
the main reflector does not need to move for most corrective tracking steps. Due to the
much lesser mass being moved as compared to the mass of the entire reflector system, the
SRT consumes far less power – approximately 75W during motion and less than 25W when
holding position.

Most importantly this SRT configuration delivers an inherent redundant tracking system
feature. The system normally operates with SRT movements, falls back to the conventional
main dish alternative upon equipment fault.
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In addition to the above redundancy from the antenna mechanics, the NGC also will be
configured to offer redundancy in the electronics, as described in the following.


1.1.7 Antenna Control System Architecture

1.1.7.1 Indoor Antenna Control System Equipment

The ASC NGC indoor unit (NGC-IDU) is a standard ASC Signal product, offered to and used
with a variety of options by our customers.

For some proposals Monopulse Tracking implementation, the indoor equipment for the
antenna control system will consist of:

      Two (2) NGC-IDU units, configured as a 1:1 redundant pair with automatic reversion,
       with separate optical fiber links to the NGC-ODU equipment. Each NGC-IDU would be
       equipped with all necessary software licenses to support all tracking modes (steptrack,
       predictive track, monopulse).

      Two (2) monopulse-capable tracking receivers, paired with NGC-IDU units. The
       primary tracking receiver would be configured for monopulse. Which receiver is used
       would depend on which NGC-IDU was active. The monopulse tracking receiver is
       connected to a monopulse tracking plate in the hub.

A Cisco Catalyst 2960 switch will be supplied for interconnecting the antenna control system
equipment.

The indoor equipment will be linked to the outdoor equipment using optical fiber (for the
antenna control IDU-to-ODU units) and coaxial cable (for the tracking receiver to tracking
plate interface).

The M&C system will interface to the control system using the NGC-IDU’s SNMP agent. This
will include proxy control of the tracking receiver and other equipment attached to the
Antenna Control System.

In addition to tracking, the NGC-IDU will also provide the following basic functions:

      Position designate pointing, and jog functions for all five major axes.
      Display of look angles to a default resolution of 0.001°, with optional resolution to
       0.0001°.


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      Tracking logs including storage of pointing angles every one second to analyze the
       performance of the monopulse tracking system. Note this requires an optional larger
       storage card system.

The redundant NGC-IDUs will be configured in an NGC Cluster with the NGC Accessory
Controller. This configuration will allow the NGC-IDUs to share configuration information; the
backup NGC-IDU will therefore not need to be separately managed. This also allows sharing
some operational information, such as signal strength indications and fault statuses.

1.1.7.2 Outdoor Antenna Control System Equipment
Outdoor equipment in the NGC architecture includes all motor drive electronics, axis
transducers, and limit switches. All axes have both soft and hard movement limits.

The outdoor equipment will consist of:

      The NGC-ODU for the extended azimuth mount, which consists of several small
       electronics enclosures interconnected by the NGC Bus. These enclosures will include
       the following electronic components:
      Two (2) MC-7 master control boards, each mated via fiber connection to an NGC-IDU.
      One (1) elevation drive interface, which consists of a Yaskawa V1000-based variable
       frequency drive, control electronics, a 26-bit Heidenhain ROC 426 optical encoder for
       the main elevation drive, and the mechanical limit switch package. Dual motors are
       not necessary in elevation because gravity bias tends to remove backlash from the
       axis. The motorization of elevation will be jackscrew-based.
      One (1) azimuth drive interface, which consists of two Yaskawa G7-based variable
       frequency drives, control electronics, a 26-bit Heidenhain ROC 426 optical encoder for
       the main elevation drive, and the mechanical limit switch package. The azimuth drive
       uses two AC motors and uses electrical preload (counter-torque) to remove backlash
       from the axis. The motors will be connected through spur-and-bull-gear to the
       azimuth axis.
      One (1) three axis SRT drive interface, which can move the SRT in the azimuth (X),
       elevation (Y), and focus (Z) axis. (The ability of the SRT to refocus the antenna is
       significant as thermal distortions include shallowing/deepening of focus.)
      For the Main GW, one (1) monopulse tracking plate, which takes the delta signal from
       the feed and combines it with the sum signal at calibrated phase delays (under control
       of the tracking receiver) to construct a synchronously amplitude modulated beacon
       signal. The tracking receiver demodulates this signal to recover the delta amplitude.
      For the Main GW, one (1) tracking down-converter.

The outdoor motorization control system (pedestal positioner and SRT) proposed is
substantially identical to one delivered to multiple US sites in the 2010-2012 time period. The
NGC-ODU provided will be a standard ASC Signal product available to any customer, and is
not expected to be a custom design.
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1.1.7.3 Antenna Control System Redundancy

With respect to system antenna control, the proposed architecture of the overall Dual
Gateway implementation offers multiple redundancy protection levels at several points:

      Spatial diversity. The backup gateway supplies a redundant system.
      Equipment redundancy, i.e., tracking receiver, NGC-IDUs, the fiber links to the NGC-
       ODUs and an electronics module in the ODUs.

ASC Signal proposes the following to be non-redundant:

      The backup antenna control system will not be equipped with a monopulse tracking
       plate. ASC Signal believes the combination of a backup gateway and steptrack is
       adequate for all reasonable scenarios if repair of the monopulse tracking system is
       required.
      The main reflector motorization subsystem will not be redundant, nor is the SRT, since
       they effectively back up each other for a geostationary satellite.


1.1.7.4 Evaluation of Tracking Modes of Operation
The following is in response to the RFP requirement for evaluating different tracking modes.

The NGC will be capable of operating in the following tracking modes:

   i. Monopulse tracking where the tracking receiver continuously supplies a pointing error
      to the control system without depointing the main beam. This is accomplished by
      receiving a “delta” output from a specially constructed feed assembly and multiplexing
      that onto the “sum” signal using phase delays to electronically steer the receive beam.
      Algorithmically this is the simplest tracking approach: the NGC will develop a new
      commanded angle based on the pointing error added to the current position, and drive
      toward that angle. Because the system has two degrees of freedom for each axis, the
      NGC must allocate the commanded azimuth and elevation to main reflector and SRT
      commands, which is done by the NGC-ODU. The SRT is normally moved preferentially
      unless the movement exceeds a user-defined circular limit, in which case the system
      simultaneously moves both subreflector and main dish to smoothly re-center the SRT.
      The effect is that the control system minimizes the delta channel (“null seeking”) as the
      main optimization criterion for tracking. The drawbacks to monopulse tracking are:

           (a) the complex receiver electronics necessary to analyze the delta channel from
               the TE21 mode coupler, and


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       (b) sensitivity to asymmetry in the reflector that distorts the shape of the “delta”
           pattern versus the “sum” pattern. Large Ka-band antennas in particular,
           because of the short wavelength, are subject to significant pattern
           asymmetries due to solar heating. Under some clear-sky conditions, this effect
           may make monopulse tracking performance less than desired. In these cases
           the customer should fall back to step track.

  Note that monopulse tracking cannot focus the Z axis of the SRT. This process must be
  done through an occasional step track process.

ii. Step track¸ where through small depointings of the receive beam, and measurement of
    the resulting signal loss, peak signal angles are empirically derived. This approach is
    well-understood and universal.

  The main drawback to step track for this application is that de-pointing the receive
  beam enough to make for a measureable loss will cause a significant loss in the
  transmit uplink. Smaller step sizes reduce the loss but they also decrease the RMS
  accuracy due to the lack of resolution in the signal strength. Since the customer
  requires a 0.3dB max drop (10% of beamwidth), a very small step size (5%) coupled
  with very long integration times (10-15s) will be required to get reasonable
  performance. This makes it suitable as a fallback or emergency tracking approach but
  for normal operation it will have trouble meeting the desired performance.

iii. Orbital prediction or “SmarTrack”, where step track is used to construct a
     mathematical model of the motion of the satellite which is constrained by
     astrodynamics. Once the model is built, it is used to predict the motion of satellite, and
     therefore the antenna.

  The problem with orbital prediction is it was developed to solve a different problem
  than the one presented by most large-aperture Ka-band systems. It assumes that the
  orbital motion of the satellite is the only significant variable in the beam angle. For
  well-station-kept satellites (i < 0.1°) the motion due to astrodynamics is comparable in
  magnitude to a completely uncorrelated but non-random beam deformation due to
  thermal distortion of the main reflector under solar load. Since the orbital models all
  assume that pointing feedback noise is just noise, and since they assume that the
  filtered pointing angles correspond to true look angles of satellites in Keplerian orbits,
  the existence of non-random noise makes the orbital prediction process inaccurate.
  ASC Signal’s experience is that no orbital-derivation algorithm is useful for low-
  inclination Ka-band satellites with large apertures due to these factors.

iv. Ephemeris Predictive track (NORAD/Intelsat elements), where an authoritative set of
    Keplerian ephemeris parameters is used to predict look angles.

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      These approaches all suffer from the same issues as orbital prediction, due to the same
      combination of circumstances as mentioned above.


The following tables show typical performance tracking analysis results of the 9.4m antenna
operating in Ka-band for three different tracking methods, using both the SRT and mount
motion tracking scenarios under both calm and moderate wind conditions for various
frequencies.     One of the three methods, “Memory” track, covers ephemeris (NORAD,
Intelsat, etc), and predictive track where there is no direct beacon reception feedback
required.

Results are provided both in angular tracking error as well as predicted signal tracking losses
in both the downlink and uplink. The half power beamwidths for 30 GHz transmit and 20 GHz
receive frequencies are 0.072 deg and 0.108 deg respectively.

Each table gives a predicted RMS and a calculated expected peak error based on worst-case
assumptions. Peak errors would be transient, RMS errors will be normally present.

For step track in calm conditions, the predicted performance for the main reflector is 0.15dB
RMS downlink and 0.33dB RMS uplink loss. The majority of the loss is caused by the step track
motion.

For monopulse tracking with the main reflector improvements to about 0.010dB/0.030dB are
achieved. This assumes that there is no significant thermal distortion of the main reflector
causing asymmetries which would introduce tracking errors to the monopulse mode. When
the environmental control system detects significant temperature gradients across the dish, it
may be necessary to switch to step track to resume peak-based pointing rather than null-
based pointing.

In windy conditions the RMS tracking losses for steptrack increase to 0.19dB and 0.43dB.
Note the sharp increases in peak error caused by deflection. Memory track is even worse due
to the lack of control system feedback to implement counter measures to unobservable
structural wind-up caused by wind force.

In clear skies, SRT tracking for steptrack improves the performance slightly due to the
increased accuracy of the subreflector positioner.




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                           Weather              Calm Clear Sky Conditions              Operational Winds 44.7 gusting to 55.9
     STEP TRACK                                                                                        mph
9.4 m Performance Ka-                   Mount Motion                                    Mount Motion
                                                                        SRT                                       SRT
        band              Dist Type        Drives                                          Drives
                                        RMS      Peak           RMS            Peak     RMS       Peak      RMS        Peak

Feedback Quantization      Constant    0.0004       0.0007     0.0000         0.0000   0.0004    0.0007     0.0000    0.0000
Deadband                   Constant    0.0017       0.0030     0.0006         0.0010   0.0017    0.0030     0.0006    0.0010
Tracking Lag              Sinusoidal   0.0031       0.0044     0.0031         0.0044   0.0031    0.0044     0.0031    0.0044
Scintillation Noise        Gaussian    0.0033       0.0098     0.0033         0.0098   0.0033    0.0098     0.0033    0.0098
Wind Induced Error         Gaussian    0.0013       0.0039     0.0013         0.0039   0.0013    0.0039     0.0013    0.0039
Variable Tracking Error     Mixed      0.005        0.010      0.005           0.010   0.005     0.010      0.005     0.010

Gust Deflection           Gaussian      0.000       0.000       0.000         0.000    0.007      0.020     0.007      0.020

Total Variable Error       Mixed        0.005       0.010       0.005         0.010    0.008      0.021     0.008      0.021

Scan Loss                 Absolute      0.011       0.011       0.011         0.011    0.011      0.011     0.011      0.011

Total Angular Error deg                 0.012       0.015       0.012         0.014    0.014      0.023     0.013      0.023

DL Signal Loss dB                        0.15        0.22       0.14           0.21     0.19      0.57       0.19      0.56
% of HPBW                               11.0%       13.6%      10.9%          13.4%    12.6%     21.7%      12.5%     21.7%

UL Signal Loss dB                        0.33        0.50       0.32           0.48     0.43      1.27       0.42      1.27
% of HPBW                               16.5%       20.4%       16.4          20.0%    18.9%     32.6%      18.7%     32.5%


                                     TABLE 3 STEP TRACK SYSTEM PERFORMANCE


                           Weather              Calm Clear Sky Conditions              Operational Winds 44.7 gusting to 55.9
    MEMORY TRACK                                                                                       mph
 9.4 m Performance Ka-                  Mount Motion                                    Mount Motion
                                                                        SRT                                       SRT
         band             Dist Type        Drives                                          Drives
                                        RMS      Peak           RMS           Peak      RMS       Peak      RMS         Peak

Feedback Quantization     Constant     0.0004      0.0007      0.0000         0.0000   0.0004    0.0007    0.0000     0.0000
Feedback Repeat.          Gaussian     0.0033      0.0100      0.0003         0.0010   0.0033    0.0100    0.0003     0.0010
Deadband                  Constant     0.0017      0.0030      0.0006         0.0010   0.0017    0.0030    0.0006     0.0010
Prediction Error          Gaussian     0.0023      0.0069      0.0023         0.0069   0.0023    0.0069    0.0023     0.0069

Total Tracking Error       Mixed        0.004       0.012      0.002          0.007    0.004     0.012      0.002      0.007

Wind Deflection           Gaussian      0.000       0.000      0.000          0.000    0.018     0.054      0.018      0.054

Total Angular Error deg                 0.004       0.012      0.002          0.007    0.019     0.055      0.018      0.055

DL Signal Loss dB                       0.02         0.15       0.01          0.05      0.36      3.18       0.34      3.09
% of HPBW                               4.1%        11.0%       2.2%          6.4%     17.3%     51.5%      16.9%     50.8%

UL Signal Loss Db                       0.05         0.33       0.01          0.11      0.81      7.16       0.77      6.96
% of HPBW                               6.2%        16.6%       3.4%          9.7%     25.9%     77.3%      25.4%     76.2%


                                TABLE 4 MEMORY TRACK SYSTEM PERFORMANCE

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                           Weather             Calm Clear Sky Conditions              Operational Winds 44.7 gusting to 55.9
     MONOPULSE                                                                                        mph
9.4 m Performance Ka-                   Mount Motion                                   Mount Motion
                                                                       SRT                                       SRT
        band              Dist Type        Drives                                         Drives
                                        RMS      Peak          RMS            Peak     RMS       Peak      RMS        Peak

Feedback Quantization      Constant    0.0004     0.0007      0.0000         0.0000   0.0004    0.0007    0.0000     0.0000
Deadband                   Constant    0.0017     0.0030      0.0006         0.0010   0.0017    0.0030    0.0006     0.0010
Tracking Lag              Sinusoidal   0.0023     0.0032      0.0023         0.0032   0.0023    0.0032    0.0023     0.0032

Variable Tracking Error    Mixed       0.003       0.004       0.002         0.003    0.003     0.004      0.002      0.003

Gust Deflection           Gaussian     0.000       0.000      0.0000         0.0000   0.007     0.020      0.007      0.020

Total Variable Error       Mixed       0.003       0.004       0.002         0.003    0.007     0.018      0.007      0.018

Bias Error                Absolute     0.002       0.002       0.002         0.002    0.002     0.002      0.002      0.002

Total Angular Error deg                0.004       0.005       0.003         0.004    0.007     0.019      0.007      0.019

DL Signal Loss dB                      0.01        0.02        0.01          0.02     0.06       0.36      0.05       0.36
% of HPBW                              3.3%        4.6%        3.0%          3.7%     6.9%      17.3%      6.7%      17.3%

UL Signal Loss dB                      0.03        0.06        0.02          0.04      0.13      0.81       0.12      0.81
% of HPBW                              5.0%        6.8%        4.4%          5.6%     10.4%     25.9%      10.1%     25.9%

                                   TABLE 5 MONOPULSE SYSTEM PERFORMANCE

1.1.8 Environmental Controls
1.1.8.1 Dehydration Subsystem

The dehydration subsystem will use the ETI ADH NETCOM automatic dehydrator. This
automatic dehydrator supplies low pressure dry air to keep waveguide and coaxial cable dry.
“Snap On” type air leakage valves will be implemented along with quick release couplings
Norgren Series 233 with type G ¼ connection for monitoring and testing the system. For
easier management, operation, and maintainability this unit will be housed in an outdoor
rated unit mounted on the antenna pedestal and will incorporate an Ethernet interface for
integration to the M&C System.

1.1.8.2 Plenum Based Environmental Management

To help manage thermal distortion the 9.4m antenna subsystem can be integrated with a
reflector enclosing plenum system. Normally reserved for colder climates with significant
snowfall, this system has been designed to “manage” ambient temperature within the
plenum behind the reflector by monitoring multiple points behind the reflector sense
temperature differentials and responding as needed. These techniques result in a more
uniform ambient temperature around the reflector. This management results in more
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improved performance of the reflector. ASC Signal has conducted extensive measurements
both characterizing and optimizing plenum systems for Ka band ESA applications. A full
measurement report on this activity is available upon request.

1.1.8.3 Anti Dew Systems

The 9.4m antenna subsystem also incorporates a feed anti-dew system designed to ensure
the external surface of the feed window does not experience any dew-point condensation
which could otherwise completely attenuate operational emissions.

1.1.8.4 Rain Diverter

ASC also uses rain deviator (feed blower) for rain events. Triggered by seninsing the presence
of rain the system is designed to target a high velocity stream of air around the feed horn to
vaporize any moisture near the vicinity of the feed horn window before. While this cannot
mitigate far field attenuation in the path due to moisture, localized moisture around the feed
no longer has the chance to hit the feed window surface and otherwise degrade the signals.

1.1.9 Hub air conditioning

As required dual air conditioning system will be installed to control the antenna hub
temperature. The antenna hub will be sealed from leakage and insulated accordingly. The
TWT exhaust will be connected to louvers ported out of the hub, venting excessive the heat
from the hub and enabling more efficient operation. The air conditioning units will be sized
sufficiently so that each individual air conditioning unit will be able to appropriately cool the
equipment, hence the system, is redundant in respect that both are operable however in the
vent of failure of a single unit the overall cooling operation will not be hampered. In addition,
in the unlikely event both units fail the fan vent systems will activate for cooling the hub
equipment.




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1.2    G/T Analysis
A detailed analysis of the Gateway G/T has been performed. The detailed worksheet appear
in Appendix C, and are summarized in the Table below. Ka Band G/T analysis is differs from
Ku or C Band analysis due to monotonically increasing noise temperature with frequency due
to the atmospheric absorption characteristics. This phenomenon is presented in the
antenna’s noise temperature Table of values below.

                                                 Antenna Temp (K)
                     ELEVATION
                                                       FREQ (GHz)
                     ANGLE (deg)       20.2               20.7      21.2
                         5°            172                184       195
                         10°           141                150       159
                         20°           120                124       128
                         30°           107                 11       112
                         40°           104                106       108
                         50°           101                102       104
                                   TABLE 6 9.4M NOISE TABLE

The G/T is degraded by tracking error, wind deflection and optical deformation and at Ka
Band it is very important to consider solar defocusing. All antennas, no matter their design,
are affected by solar defocusing to some extent. ASC has carefully characterized this
degradation and has devised an industry unique form of mitigating this inherent gain
reduction characteristic by adding a “Z-Axis” to the optics which effectively corrects the
effects of solar optical distortion. Without the “Z-Axis” correction, an antenna can and does
lose up to 1.4 dB of receive gain (even extremely robust structural designed antennas) in the
presence of intense solar radiation. The ASC SRT Z-Axis correction reduces the solar
defocusing affect to less than 0.25 dB! This is a critical element to consider when analyzing
overall Gateway Terminal performance both at Transmit and Receive.

The following Table summarizes the G/T calculated for three various environmental
conditions and for three separate hardware configurations. The three configurations are: (1)
SRT Step Track, (2) SRT Mono Pulse, and (3) Mono Pulse Mount Motion. The three
environmental conditions are: (1) Ideal Conditions, i.e., no wind and no sun, (2) Solar Defocus
and no wind, and (3) Solar Defocus and wind simultaneously. The take-a-way from this data is
simply that Mono Pulse tracking buys very little return for its complexity and cost and by
mitigating the solar defocusing rather substantial gains are made. The data in the data is a
little more meaningful when see graphically as illustrated in the following chart.

The proposed antenna and tracking system design affords a cost effective and less complex
engineering solution that achieves a G/T within a small variance from the specification!

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                                         CONFIGURATION                          G/T (dB/K)
                      SRT Mono Pulse ideal condx                                  38.66
                      Mount Motion Mono Pulse ideal condx                         38.66
                      3-axis SRT ideal condx                                      38.53
                      SRT Mono Pulse Solar Defocus                                38.41
                      3-axis SRT Solar Defocus                                    38.28
                      SRT Mono Pulse Solar and Wind                               38.24
                      3-axis SRT Solar and Wind                                   38.11
                      Mount Motion Mono Pulse Solar Defocus                       37.26
                      Mount Motion Mono Pulse Solar and Wind                      37.09

                                                   TABLE 7 G/T TABLE




                      G/T Variances versus Antenna Configuration
             38.50


             38.00


             37.50
G/T (dB/K)




             37.00


             36.50


             36.00


             35.50
                     SRT Mono Mount 3-axis SRT SRT Mono 3-axis SRT SRT Mono 3-axis SRT Mount   Mount
                     Pulse ideal Motion      ideal  Pulse   Solar    Pulse Solar and Motion Motion
                       condx      Mono      condx   Solar  Defocus Solar and Wind       Mono   Mono
                                Pulse ideal        Defocus           Wind               Pulse   Pulse
                                  condx                                                 Solar Solar and
                                                                                       Defocus  Wind

                                       FIGURE 11 G/T CONFIGURATION VARIANCE



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G/T CALCULATIONS                                                          38.24    dB/K

SRT Step Track Antenna Parameters
  Antenna Type                                                              9.4    M
  Antenna Efficiency                                                        53     %
  Solar Defocusing with 3-axis SRT                                         0.25    dB
  RMS Pointing Error Winds 45MPH gusts to 65MPH                            0.18    dB
  Effective Operational Antenna Gain @ Op Freq & Environ Condx             63.0    dBi
  Antenna Noise Temp @ Op EL & Op Freq & Atmos water vapor =7.5 g/m^3     124.0    K
  Combiner VSWR                                                             1.3    :1
  Antenna Op Elevation Angle                                               20.0    °
  Op Frequency                                                            20700    MHz
  Analysis Ambient Temperature                                              23     C

LNA/LNB Subsystem
  Feed to Plate W/G Loss + Filter                                         0.438    dB
  1:2 LNA Switch Plate w/cplr Loss                                        0.26     dB
  LNA Temperature @ 23 C                                                   100     K
  LNA Gain @ 23 C                                                           50     dB
  LNA Input VSWR                                                          1.25     :1
  LNA Output +1 dB Comp Pt                                                  10     dBm

System Analysis
Net System Gains
   Antenna                                                                63.0     dBi
   W/G Connection                                                         -0.44    dB
   W/G Switch                                                             -0.26    dB
   LNA Mismatch                                                           -0.05    dB
   Net Gain                                                               62.24    dBi
Net System Noise (Referenced at LNA Input)
   Ambient Temperature                                                       23    °C
   LNA                                                                      100    K
   Antenna                                                                104.29   K
   TRF                                                                     26.42   K
   W/G Switch                                                              16.99   K
   LNA Reflec. Noise                                                       3.61    K
   RF Cable/CPLR Loss                                                      0.00    K
   1:2 Switch Loss                                                         0.00    K
   BDC                                                                     0.22    K
   100 M IFL                                                               0.01    K
   Net System Temp                                                        251.53   K

             TABLE 8 SAMPLE G/T CALCULATION MONOPULSE SRT WITH SOLAR DEFOCUSING
                             and 45 MPH Wind gusting to 60 MPH




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ANNEX 2: DRAWINGS




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A2.5 -   EXAMPLE HUB CONFIGURATION #1




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A2.6 -   EXAMPLE HUB CONFIGURATION #2




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A2.7 -           3-D ANTENNA MODEL


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A2.8 -   ANTENNA MOUNT, AZIMUTH SWEPT VOLUME


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A2.9 -   ANTENNA MOUNT ELEVATION SWEPT VOLUME

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A2.10 -   SAMPLE FOUNDATION DRAWING

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A2.11 -   EXAMPLE FOUNDATION DRAWING

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Document Created: 2015-12-21 14:20:24
Document Modified: 2015-12-21 14:20:24

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