Attachment Technical Analysis

This document pretains to SES-LFS-20151020-00734 for License to use Foreign Satellite (earth) on a Satellite Earth Station filing.

IBFS_SESLFS2015102000734_1111281

USN Support of Proba-V in North Pole Alaska


Universal Space Network (USN) has been contracted to provide additional
ground station support for the Proba-V mission from the USN North Pole Alaska
ground station. This support is receive only. USN maintains an array of large
aperture tracking antennas at this station. USN is supporting the Proba-V
downlink today under an FCC Special Temporary Authority (STA) and is
pursuing a receive only license for the life of the mission.

Universal Space Network
Address: 1465 Bradway Road, North Pole, Alaska 99705
Phone number: 907‐490‐3064
Latitude: 64° 48’ 16.61” North
Longitude: 147° 30’ 0.87” West
Altitude:146 meters MSL


About Proba-V

Proba-V is a vegetation imaging satellite launched by the European Space
Agency. The spacecraft is norad ID = 39159 and registered by France with the
ITU.


                                              Proba-V satellite
                                              The Proba-V satellite may only be
                                              slightly larger than a washing
                                              machine, but it is tasked with a full-
                                              scale mission. This miniature
                                              satellite is designed to map land
                                              cover and vegetation growth across
                                              the entire globe every two days.
                                              Over the last decade 'Proba' has
                                              become synonymous with small
                                              high-performance satellites,
                                              designed around innovation. The
two previous satellites in the series were demonstration missions to give
promising technologies an early chance to fly in space. They were overseen by
ESA’s Directorate of Technical and Quality Management. Although designed as
a demonstration mission, the success of the first Proba satellite led to it being
operated as an Earth observation Third Party Mission. Proba-1 carries a high-
resolution imaging spectrometer.




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                            Vegetation swath
                            Proba-V, however is different from the outset: this new
                            mission will start serving as an operational Earth
                            observation mission as soon as its six-month
                            commissioning phase is complete, supplying data to an
                            existing – and eagerly waiting – international user
                            community. The 'V' stands for Vegetation – a lighter
                            but fully functional redesign of the ‘Vegetation’ imaging
                            instrument previously flown on France’s full-sized Spot-
                            4 and Spot-5 satellites.

Launched on 7 May 2013, Proba-V has been designed to continue the supply of
this much needed imagery for applications such as climate impact assessments,
water resource management, agricultural monitoring and food security estimates.


Analysis

Proba-V is an NGSO space station in an 820 Km altitude orbit at an inclination of
98.7°. Due to the NGSO type orbit its antenna pattern impinging upon the earth
is dynamic. This analysis is intended to show how the RF pattern impinges upon
the ground station area in North Pole Alaska and surrounding areas.

Figure 1 below shows the total passes calculated for a typical day that are visible
from USN’s Alaska ground station. Note that not all 10 passes each day will be
supported, typically only two each day will be taken.

Proba-V
1 39159U 13021A   15097.16845750 .00000099 00000-0 63656-4 0 9990
2 39159 098.6652 177.8153 0004362 164.1357 195.9962 14.22868732 99540




Figure 1 - USN Alaska coverage of Proba-V on a typical day 7 April 2015



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USN Alaska possible passes for Proba-V on a typical day

Pass     Start Time (UTCG)           Stop Time (UTCG)

  1      7   Apr   2015   01:03:26   7   Apr   2015   01:13:43
  2      7   Apr   2015   02:42:29   7   Apr   2015   02:51:26
  3      7   Apr   2015   04:20:21   7   Apr   2015   04:30:12
  4      7   Apr   2015   05:58:09   7   Apr   2015   06:09:58
  5      7   Apr   2015   07:37:15   7   Apr   2015   07:50:08
  6      7   Apr   2015   09:18:33   7   Apr   2015   09:30:13
  7      7   Apr   2015   11:03:30   7   Apr   2015   11:09:09
  8      7   Apr   2015   19:41:24   7   Apr   2015   19:51:14
  9      7   Apr   2015   21:21:14   7   Apr   2015   21:33:53
 10      7   Apr   2015   23:01:25   7   Apr   2015   23:13:54


Downlink RF Specifications

Proba-V’s downlink consist of a highly filtered OQPSK with symbol rate of
84.8Msps. 98% of the energy is contained within a 100MHz bandwidth and thus
the emission designator is 100M0G2D. The center frequency is 8090.0 MHz,
and polarization is RHCP.

Figure 2 below represents the spacecraft transmit antenna’s beam pattern. The
colour red indicates the dominant polarization of RHCP, while the blue indicates
LHCP. Theta of 0 is the boresight of the antenna that is nadir pointing towards
earth. The antenna is rated at a +3.0 dBi gain maximum and typically for any
visible satellite pass the worst case gain is approximately -1.0 dBi since the edge
of the antenna pattern is not visible due to the combination of orbital altitude and
the earth’s curvature.




Figure 2 – Static spacecraft antenna pattern


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During a direct overhead pass taken at USN Alaska, the space station impinges
a dynamic pattern on the earth as shown in figure 3. Note the blue grid in the
figure represents radio frequency impingement on the earth during this direct
overhead pass. Figure 4 shows the nominal flux density delta power impinging
in the area as the space station is directly overhead. Note that the yellow
shaded area is in the 0 to +1 dBi contour of the pattern and the red shaded area
is in the 0 to +3 dBi contour of the pattern.




Figure 3 – Overhead pass RF impingement on earth




Figure 4 – RF flux density delta power at moment of overhead



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Power Flux Density (PDF) impinging on the Earth

The Flux density is calculated as:

                                               )
         Where       is the distance from spacecraft to the ground.
         Where         is the Effective Isotropic Radiated Power of the Spacecraft.

Data from the spacecraft vendor indicates that the maximum EIRP of Proba-V is
13.0 dBW (10.0 effective watt transmit power into a +3 dBi antenna). The
altitude (and thus the closest distance to earth during an overhead pass) is = 820
Km. Converting 13.0 dBW to scalar watts = 19.95 watts transmitted at 8090 MHz

Therefor:
                           .               ∗       ,               )

PDF = 2.361 x 10-12 Watts/meter2
Or
PDF = 2.361 x 10-13 mW/cm2
Or
PDF = -116.3 dBW/meter2
Or
PDF = -160.2 dBW/meter2/4KHz worse case (using occupied BW = 100MHz)

Table 1 shows the PDF versus the incident angle as seen from ground.
   Incidence Angle              PDF
                           (dBW/m2/4KHz)
           0                   -163.2
           5                   -161.7
           10                  -160.7
           15                  -160.5
           20                  -160.2
           25                  -160.2
           30                  -160.3
           35                  -160.7
           40                  -161.2
           45                  -162.2
           50                  -162.7
           55                  -163.1
           60                  -163.2
           65                  -163.2
           70                  -162.4
           75                  -162.2
           80                  -161.7
           85                  -161.5
           90                  -161.4



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Figure 5 shows the compliance of PDF on the earth surface with NTIA and ITU
specifications. Note this shows the worst case PDF on an overhead pass at the
closest possible distance of spacecraft to ground. Most Proba-V passes will
produce a lower PFD.




Figure 5 – Proba-V PDF incident on the earth’s surface




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Proba-V ITU Registration




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Document Created: 2015-05-08 10:16:13
Document Modified: 2015-05-08 10:16:13

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