ITU-R S 1899-2012 Protection criteria and interference assessment methods for non-GSO inter-satellite links in the 23 183-23 377 GHz band with respect to the space research service.pdf

《ITU-R S 1899-2012 Protection criteria and interference assessment methods for non-GSO inter-satellite links in the 23 183-23 377 GHz band with respect to the space research service.pdf》由会员分享，可在线阅读，更多相关《ITU-R S 1899-2012 Protection criteria and interference assessment methods for non-GSO inter-satellite links in the 23 183-23 377 GHz band with respect to the space research service.pdf（7页珍藏版）》请在麦多课文档分享上搜索。

1、 Recommendation ITU-R S.1899(01/2012)Protection criteria and interference assessment methods for non-GSO inter-satellite links in the 23.183-23.377 GHz band with respect to the space research serviceS SeriesFixed-satellite servicesii Rec. ITU-R S.1899 Foreword The role of the Radiocommunication Sect

2、or is to ensure the rational, equitable, efficient and economical use of the radio-frequency spectrum by all radiocommunication services, including satellite services, and carry out studies without limit of frequency range on the basis of which Recommendations are adopted. The regulatory and policy

3、functions of the Radiocommunication Sector are performed by World and Regional Radiocommunication Conferences and Radiocommunication Assemblies supported by Study Groups. Policy on Intellectual Property Right (IPR) ITU-R policy on IPR is described in the Common Patent Policy for ITU-T/ITU-R/ISO/IEC

4、referenced in Annex 1 of Resolution ITU-R 1. Forms to be used for the submission of patent statements and licensing declarations by patent holders are available from http:/www.itu.int/ITU-R/go/patents/en where the Guidelines for Implementation of the Common Patent Policy for ITU-T/ITU-R/ISO/IEC and

5、the ITU-R patent information database can also be found. Series of ITU-R Recommendations (Also available online at http:/www.itu.int/publ/R-REC/en) Series Title BO Satellite delivery BR Recording for production, archival and play-out; film for television BS Broadcasting service (sound) BT Broadcasti

6、ng service (television) F Fixed service M Mobile, radiodetermination, amateur and related satellite services P Radiowave propagation RA Radio astronomy RS Remote sensing systems S Fixed-satellite service SA Space applications and meteorology SF Frequency sharing and coordination between fixed-satell

7、ite and fixed service systems SM Spectrum management SNG Satellite news gathering TF Time signals and frequency standards emissions V Vocabulary and related subjects Note: This ITU-R Recommendation was approved in English under the procedure detailed in Resolution ITU-R 1. Electronic Publication Gen

8、eva, 2012 ITU 2012 All rights reserved. No part of this publication may be reproduced, by any means whatsoever, without written permission of ITU. Rec. ITU-R S.1899 1 RECOMMENDATION ITU-R S.1899 Protection criteria and interference assessment methods for non-GSO inter-satellite links in the 23.183-2

9、3.377 GHz band with respect to the space research service (2012) Scope Links in the inter-satellite service (ISS) are used by some systems to interconnect two or more non-GSO satellites together. This Recommendation presents protection criteria and interference assessment methods for such non-GSO IS

10、S links in the 23.183-23.377 GHz band with respect to the space research service (SRS). The ITU Radiocommunication Assembly, considering a) that the band 22.55-23.55 GHz is allocated on a co-primary basis to the inter-satellite, fixed and mobile services; b) that ISS links of non-GSO systems connect

11、 satellites providing service in other mobile satellite and fixed satellite bands; c) that the band is also shared by systems in the fixed service and other ISS links connecting satellites in the space research service; d) that methods exist for analysing the interference from other systems operatin

12、g in the band allocated to non-GSO ISS links; e) that some operational non-GSO systems use ISS links, recommends 1 that the aggregated unwanted emission levels in the band 23.183-23.377 GHz due to earth stations in the space research service operating in the band 22.55-23.15 GHz should not exceed a

13、power density of 155 dBW/MHz at the input to a non-GSO ISS satellite receiver, for a fraction of time greater than 102per cent (0.01%); 2 that the factors described in Annex 2 should be used to evaluate unwanted emission levels into the non-GSO system from space research service systems in the alloc

14、ation; 3 that the following Note should be considered as part of this Recommendation. NOTE A type of system that requires protection and operates in the band 23.183-23.377 GHz is described in Annex 1. 2 Rec. ITU-R S.1899 Annex 1 General system characteristics of an operational non-GSO system using i

15、nter-satellite links in the range 23.183-23.377 GHz At least one non-GSO satellite communication system uses the ISS links in the 22.55-23.55 GHz band. The major characteristics of an operating constellation are presented in Table A. Its orbital configuration is described in Table B. Due to the cros

16、s-linked nature of the satellite constellation in providing end-to-end services, the channel usage and loading distribution is non-uniform and difficult to characterize at any given time and location. TABLE A System specifications System parameter Value Number of satellite planes 6 Number of satelli

17、tes per plane 11 Nominal altitude (km) 780 Orbit type Circular polar (inclination angle of 86.5) Orbital period (min) 100 Frequency range (GHz) 23.183-23.377 Necessary bandwidth for 8 channels 8 19 MHz channels (total bandwidth 194 MHz) The necessary bandwidth for one channel is 19 MHz The channel s

18、pacing equals 25 MHz Satellite system noise temperature (K) 877 Peak transmitter power (per 19 MHz channel) (dBW) 3 Antenna gain (one antenna per channel) (dBi) 36.6 e.i.r.p. (one single 19 MHz channel) (dBW) 39.6 Rec. ITU-R S.1899 3 TABLE B Argument of latitude for satellites in the system in Table

19、 A Plane 1 Right ascending node = 0 Plane 2 Right ascending node = 31.6 Plane 3 Right ascending node = 63.2 Satellite Arg. of latitude (degrees) Satellite Arg. of latitude (degrees) Satellite Arg. of latitude (degrees) 1 100.8 12 83.1 23 98.2 2 68.0 13 50.4 24 65.43 35.3 14 17.7 25 32.7 4 2.6 15 344

20、.9 26 360.05 329.9 16 312.2 27 327.3 6 297.1 17 279.5 28 294.57 264.4 18 246.7 29 261.8 8 231.7 19 214.0 30 229.19 199.0 20 181.3 31 196.4 10 166.2 21 148.6 32 163.611 133.5 22 115.8 33 130.9 Plane 4 Right ascending node = 94.8 Plane 5 Right ascending node = 126.4 Plane 6 Right ascending node = 22.1

21、 Satellite Arg. of latitude (degrees) Satellite Arg. of latitude (degrees) Satellite Arg. of latitude (degrees) 34 80.5 45 95.6 56 77.9 35 47.8 46 62.9 57 45.236 15.1 47 30.1 58 12.5 37 342.3 48 357.4 59 339.738 309.6 49 324.7 60 307.0 39 276.9 50 291.9 61 274.340 244.1 51 259.2 62 241.5 41 211.4 52

22、 226.5 63 208.842 178.7 53 193.8 64 176.1 43 146.0 54 161.0 65 143.444 113.2 55 128.3 66 110.6 4 Rec. ITU-R S.1899 Annex 2 Factors in protection criteria 1 Potential sources of interference The ISS shares the allocation 22.55-23.55 GHz with the fixed and mobile co-primary services. The addition of s

23、ervices such as the space research service opens the possibility of additional sources of interference and prompts the interest in establishing protection criteria for the ISS. 2 Protection criteria For studies of out-of-band interference from proposed SRS uplinks operating in 22.55-23.15 GHz into t

24、he non-GSO system described in Annex 1 that uses inter-satellite links (ISL) operating in the 23.183-23.377 GHz band, the protection criteria of I/N = 16 dB not to be exceeded more than 0.01% of the time at the input to each ISL receiver taking into account the aggregated effect of all SRS earth sta

25、tions in operation in the 22.55-23.15 GHz band would be used. An I/N = 16 dB corresponds to an I0= 155 dB(W/MHz), derived from the system noise temperature given in Table A. Recognizing that this non-GSO system shares its ISS spectrum with other services, the above criterion does not apply now or in

26、 the future to the existing service sharing arrangements for systems operating in the part of the allocation in which the ISL of this system operate. The protection criterion in Recommendation ITU-R SA.1155 applies to the existing systems with which this system shares spectrum. Furthermore, the shar

27、ing studies between SRS uplinks and non-GSO-non-GSO ISS links operating co-frequency in the band 22.55-23.15 GHz should apply the value of I/N = 10 dB not to be exceeded more than 0.1% per link as set forth in Recommendation ITU-R SA.1155. 3 Antenna pattern In discussing the antenna pattern that sho

28、uld be used to represent the non-GSO system ISS receiving antenna in SRS interference studies two possibilities were initially considered. On the one hand, a preference was expressed for the pattern in Recommendation ITU-R F.1245 for compatibility studies with dynamic interference configurations, wh

29、ereas on the other hand it was considered that the antenna pattern in Recommendation ITU-R S.672 was more appropriate when considering interference from a single interference source. It was noted that neither pattern may, in itself, serve as fully appropriate to use in the analyses of ISS antennas f

30、or use in interference studies. It was also noted that, in determining the statistical behaviour of interference, it would be more appropriate to consider antenna patterns that reflect the oscillatory shape of real radiation patterns. This type of pattern is usually considered in situations involvin

31、g multiple interference entries or in situations where the interference off-axis arrival angle at the victim receiving antenna varies in time, which is the case in question. In consideration of the above, it was concluded that a pattern that lies between the patterns in Recommendations ITU-R F.1245

32、and ITU-R S.672 and that reflects the oscillatory shape of real antenna radiation patterns would most appropriately model the ISS antenna. Rec. ITU-R S.1899 5 Therefore, the following pattern should be used for modelling the non-GSO system ISS antenna in carrying out such unwanted emission level stu

33、dies: +=degrees1804.38; )(3degrees4.381.6;)(log256.36degrees1.61.3; )(17degrees1.30; 37.36)(2FFFGbwhere: += )1()58.2(23sinlog10)(2bF with b= 1.2 and = 0.999 4 Method There are several appropriate methods for analysing interference from an SRS earth station into the ISS links of the subject non-GSO s

34、ystem. These include either analytical or dynamic computer simulation methodologies. In conducting such analyses it is necessary to consider the rapid movements of the non-GSO satellites crossing through narrow SRS uplink beams, as well as movements of the inter-planar cross link antennas of such no

35、n-GSO satellites relative to SRS earth station antenna pointing. Thus, the use of dynamic computer simulations is an appropriate method to determine the potential interference to these non-GSO satellites operating in the ISS. In addition, the analytical method in Recommendation ITU-R S.1529 is an al

36、ternative appropriate method to determine the potential interference to the ISS links of these non-GSO satellites, recognizing that the Recommendation ITU-R S.1529 method may have to be adapted, verified and validated to consider scenarios involving SRS satellite operations in non-Earth orbits. Simu

37、lation parameters, such as the time interval between samples and total simulation times, should be chosen to guarantee reliable results. The results obtained from different methods should be compared to assess reliability. In this sense, comparison with results from the analytical method contained in Recommendation ITU-R S.1529 would be a useful technique. In particular, it can be very useful in situations involving very low probability events. _