ITU-R RS 1279-1997 SPECTRUM SHARING BETWEEN SPACEBORNE PASSIVE SENSORS AND INTER-SATELLITE LINKS IN THE RANGE 50 2-59 3 GHz《星载无源传感器和星间链路在50 2-59 3 GHz内的频谱共享》.pdf

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1、 Rec. ITU-R RS.1279 1 RECOMMENDATION ITU-R RS.1279*, *SPECTRUM SHARING BETWEEN SPACEBORNE PASSIVE SENSORS AND INTER-SATELLITE LINKS IN THE RANGE 50.2-59.3 GHz (Question ITU-R 216/7) (1997) Rec. ITU-R RS.1279 The ITU Radiocommunication Assembly, considering a) that weather forecasting is an increasin

2、gly important tool which is essential to all human economic activities, and is also playing a predominant role in early identification and warnings of potentially dangerous phenomena; b) that atmospheric temperature is essential data needed for weather forecasting on a global basis; c) that the oxyg

3、en absorption band consisting of several absorption lines between 50 and 65 GHz represents a unique natural resource for remote temperature profile sensing in the atmosphere, not available in any other frequency band; d) that all-weather atmospheric temperature profiles can only be obtained on a glo

4、bal basis with sufficient accuracy through three-dimensional microwave passive measurements from low-Earth orbiting (LEO) space platforms in the unique frequency band around 60 GHz where absorption by atmospheric oxygen is taking place; e) that these passive measurements are extremely vulnerable to

5、interference because the natural variability of the atmosphere makes it impossible to recognize and to filter out measurements contaminated by interference; f) that contaminated passive sensor measurements can have a dramatic, adverse impact on climate studies and the quality of weather predictions;

6、 g) that non-geostationary-satellite orbit (non-GSO) networks providing fixed-satellite services (FSS) and mobile-satellite services are being developed which plan to employ large numbers of inter-satellite links (ISL) near 60 GHz; h) that geostationary-satellite orbit (GSO) networks providing FSS a

7、nd mobile-satellite services are being developed which plan to employ ISLs near 60 GHz; j) that the 54.25-58.2 GHz frequency band is shared on a co-primary basis by the Earth exploration-satellite service (passive) (EESS), the Space Research (passive) service, and the inter-satellite service (ISS);

8、k) that item 1.9.4.3 of Resolution 718 (WRC-95) (Agenda for the 1997 World Radiocommunication Conference) is to consider “the existing frequency allocations near 60 GHz and, if necessary, their re-allocation, with a view to protecting the Earth exploration-satellite (passive) service systems operati

9、ng in the unique oxygen absorption frequency range from about 50 GHz to about 70 GHz”; l) that Recommendation ITU-R RS.1029 contains interference protection criteria for passive sensors in bands near 60 GHz; m) that studies conducted in the band 54.25-58.2 GHz have shown that the ISLs in an non-GSO

10、network can cause interference to the passive sensors well in excess of these protection criteria (see Annex 1); n) that studies conducted in the band 54.25-58.2 GHz have shown that ISLs in GSO networks can share the band with passive sensors with suitable restrictions on the power flux density (pfd

11、) produced by GSO satellites at the sensor orbital altitude (see Annex 2), recognizing a) the need to protect existing and planned ISS systems in the band 56.9-57 GHz, _ *This Recommendation should be brought to the attention of Radiocommunication Study Group 4. *Radiocommunication Study Group 7 mad

12、e editorial amendments to this Recommendation. 2 Rec. ITU-R RS.1279 recommends 1 that, in view of considering c) and m), passive sensors and ISLs of non-GSO networks should operate in separate bands in the range 50.2-59.3 GHz; 2 that, in view of considering n), passive sensors and ISLs of GSO networ

13、ks can share bands in the range 50.2-59.3 GHz provided that the pfd at all altitudes from zero to 1 000 km above the Earths surface produced by emissions from a space station in the ISS does not exceed 147 dB(W/(m2 100 MHz). ANNEX 1 Results of the non-GSO interference study 1 Introduction The EESS i

14、ncludes spaceborne passive sensors which measure temperatures of various atmospheric layers in several frequency bands within the oxygen absorption bands near 60 GHz. Depending on the frequency, measurements in the 60 GHz band can be substantially protected from interference from terrestrial emissio

15、ns. Frequency bands near 60 GHz are also attractive for ISL of a non-GSO communications system. Unfortunately these ISLs introduce potential interference to spaceborne passive sensor measurements, which are not attenuated by oxygen absorption. Table 1 describes the non-GSO and sensor satellite orbit

16、s, and Table 2 describes the non-GSO transmission and sensor satellite reception characteristics used in the study. All antennas were modelled using Recommendation ITU-R S.672, with _10 dBi minimum gain. TABLE 1 non-GSO and sensor satellite orbit characteristics TABLE 2 non-GSO and sensor satellite

17、characteristics Orbital parameter non-GSO satellite Sensor Altitude (km) 700 833 Inclination (degrees) 98.16 98.7 Period (min.) 98.8 101.5 Eccentricity 0.0 0.0 Number of orbital planes 21 2 Number of satellites per plane 40 1 Ascending nodes Spaced 9.5 starting at 0 N.A. Parameter non-GSO satellite

18、Advanced microwave sounding unit (AMSU) sensor Pushbroom sensor Carrier frequencies (GHz) 56 and 59 56 56 Bandwidth per channel (MHz) 1 000 400 100 Power in each band (dBW) 7.4 N.A. N.A. Peak antenna gain (dBi) 48 36 45 Rec. ITU-R RS.1279 3 2 Interference from non-GSO satellites To determine whether

19、 interference from even a single non-GSO satellite can exceed the interference threshold of the sensor, three fixed geometries are considered. Figure 1 illustrates the geometries considered. Configuration 1: The potential interference path may be through the antenna main lobes of the sensor and the

20、antenna side lobes of one (or several) inter-satellite transmitter. Configuration 2: The interference path may be through the antenna side lobes of the sensor and the antenna main lobe of one (or several) inter-satellite transmitter. Configuration 3: During “cold space calibration”, main lobe-to-far

21、 lobe and main lobe-to-main lobe interferences paths are possible, as well as various intermediate combinations. 1279-01Anon-GSOnon-GSOEESSorbit tracknon-GSO visibility circle from EESS orbitEESS(850 km)Configuration 1non-GSO in sensor FOV,main-lobe to side-lobeA: FOV ( 50 renadir)Configuration 3Cal

22、ibration sequencemain-lobe to main-lobeor main-lobe to side-lobeSphere containingnon-GSO(700 km)Configuration 2non-GSO at horizon of sensor,side-lobe to main-lobeFIGURE 1Geometry of EESS-non-GSO satellite mutual visibilitiesFIGURE 1279-01 Table 3 gives the results of the static evaluation for the th

23、ree configurations assuming a pushbroom sensor. The importance of the relative positions of the EESS orbit and of the interfering non-GSO ascending nodes is illustrated by the considerable variation in the duration of interference and of the intervals between interference events. The shortest durati

24、ons and intervals apply to the case where ascending nodes of the two systems are about 180 apart. Recommendation ITU-R RS.1029 cites an interference threshold of 166 dB(W/100 MHz) for a pushbroom sensor. This is the interference threshold used in Table 3. 3 Interference statistics A computer simulat

25、ion was used to model the dynamic interaction of the non-GSO constellation and the spaceborne sensor in order to determine how often, and by how much, the sensor interference threshold is exceeded. The simulation considers interference to an advanced microwave sounding unit (AMSU) sensor rather than

26、 a pushbroom sensor because spectrum sharing is less likely to be feasible when a pushbroom sensor is used than when an AMSU sensor is used. All of the non-GSO ISLs are assumed to be transmitting continuously, and the sensor is assumed to be making measurements continuously. The results of the dynam

27、ic analysis are summarized in Fig. 2. 4 Rec. ITU-R RS.1279 TABLE 3 Interference levels and durations 1279-020 45 90 135 180 225 270 315 36013121110987654FIGURE 2Dependence of threshold exceedance on sensor ascending nodeAscending node of passive sensor (degrees)Threshold exceedance(%time)FIGURE 1279

28、-02 Each point in Fig. 2 represents the result of a simulation performed for a given ascending node of the AMSU sensor spacecraft orbit. The per cent of time that the interference level exceeds the sensor interference threshold is plotted as a function of the given AMSU ascending node. In general, f

29、or the runs represented by the points along the “top” of the curve envelope, the AMSU node was coincident with an ascending node of an non-GSO plane (e.g. 0, 66.5, . 180.5, and 190). The runs represented by the data points defining the “bottom” of the envelope correspond to AMSU orbit nodes placed i

30、n between the non-GSO planes. It should be noted that the AMSU ascending nodes between 0 and 50 were selected in arbitrary steps rather than exactly coincident with non-GSO nodes. In contrast, above 50, the AMSU orbit ascending nodes were selected to be either coincident with or half-way in between

31、two non-GSO nodes. There are more co-channel, cross-plane, ISL pointed in the direction of the AMSU sensor at 180.5 than at 0, resulting in a higher percentage of interference if the AMSU node is at 180.5. The AMSU interference threshold is 157 dB(W/400 MHz). This is the threshold assumed in Fig. 2.

32、 The calibration mode was not modelled in the simulation. Had it been modelled, Fig. 2 would have exhibited more severe interference. Interference is considered to be excessive whenever the sensor threshold is exceeded more than 0.01% of the time. Level above interf. threshold (dB) Duration of a sin

33、gle interference event (s) Interval between successive events (min) Configuration 1 18.5-31 1-75 1-81 Configuration 2 7-10 10-665 1-81 Configuration 3 7-65 2-138 1-81 Rec. ITU-R RS.1279 5 Assuming that a threshold exceedance of x% of the time corresponds to a contamination of x% of the measurement c

34、ells scanned by the sensor, Fig. 2 shows that the spatial interference criteria of Recommendation ITU-R RS.1029 are violated at all of the ascending nodes that were examined. 4 Conclusion The results in Fig. 2 demonstrate that the interference levels introduced by the ISLs of the non-GSO constellati

35、on assumed here exceed the sensor interference threshold at least 4% of the time and as much as 13% of the time. The amount of threshold exceedance depends on the ascending node of the sensor satellite relative to those of the non-GSO constellation. ANNEX 2 Results of the GSO interference study 1 In

36、troduction When the difference in longitude between two GSO satellites communicating on an ISL is sufficiently small, there will be no interference to the sensor satellites because the link does not penetrate the orbit spheres of the sensor satellites. A parametric analysis was done to determine the

37、 maximum pfd produced by an ISL at the altitude of a sensor satellite that would not cause the sensor interference threshold to be exceeded for either the scan or the calibration mode. For both modes the maximum pfds were obtained analytically. For the calibration mode simulations were performed to

38、determine the interference statistics. These statistics depend on the GSO satellite longitude separation. The separation was reduced from its maximum value of 162.6 (the separation at which the GSO-GSO link grazes the Earth) until the interference level dropped below the sensor interference threshol

39、d. Potential GSO systems have transmit and receive antenna gains ranging from 45 to 60 dBi, bandwidths ranging from 90 MHz to 1 GHz, and receive system noise temperatures of approximately 650 K. The simulations that were carried out consider antenna gains of 45, 50, 55 and 60 dBi, and a bandwidth of

40、 1 GHz. Antenna patterns from Recommendation ITU-R S.672 are assumed for the ISL antennas. The GSO satellite transmit power was adjusted throughout the simulations to achieve an ISL Eb/N0of 12 dB. Table 4 summarizes the assumed microwave sensor characteristics. TABLE 4 Microwave pushbroom sensor cha

41、racteristics 2 Results of the study In its Earth-viewing mode the sensor (assumed to be a pushbroom sensor) receives interference through its antenna side lobes, which are assumed to have a gain of 14 dBi. To avoid exceeding the interference threshold while the sensor is in the Earth-viewing mode, t

42、he pfd produced at altitudes of 1 000 km or less above the Earths surface from a single ISL transmission should not exceed _97 dB(W/(m2 100 MHz). A one dB allowance for interference from multiple ISLs reduces the allowable pfd to 98 dB(W/(m2 100 MHz). Sensor interference threshold 166 dB(W/100 MHz)

43、Maximum antenna gain 45 dBi 14 dBi back lobes Calibration antenna gain 35 dBi Field of view +48.5 from nadir Altitude 1 000 km Inclination Sun synchronous (100.1 for 1 000 km altitude) Centre frequency 56 GHz 6 Rec. ITU-R RS.1279 In its calibration mode the sensor can receive interference through it

44、s antenna main beam. Potential interference is therefore much more severe in the calibration mode. The level and duration of interference events are variable, requiring dynamic simulation. Simulation with AMSU sensors reveals that for 45 dBi GSO satellite antennas, the sensor interference threshold

45、is exceeded approximately 5% of the time at large separations of the GSO satellites (near 160). Interference is negligible for separations less than 70. The duration of interference events varies from 0.2 to 21.5 min. On the other hand, for 60 dBi GSO satellite antennas, the sensor interference thre

46、shold is exceeded only 0.14% of the time for longitudinal separations more than 160, with negligible interference for separations less than 160. The duration of interference events varies from 0.1 to 4.1 min. Simulation with pushbroom sensors would have revealed even more interference. Pushbroom sen

47、sors have fixed antennas for sensing toward the Earth. The cold calibration antenna will be a separate antenna aimed toward the cold sky. The dynamic analysis performed for the AMSU sensor would provide similar results for the pushbroom antenna because of the similar orientations. The durations of t

48、he interference periods would be a function of the gain of the calibration antenna. Pfd limits for GSO inter-satellite systems must be sufficient to protect both present and future systems. The present AMSU sensor has an antenna gain of 36 dBi, an effective aperture of 21 dB/m2at 58 GHz, and a sensi

49、tivity of _161 dBW. Allowing 3 dB for multiple interferers, it needs a pfd limit of 143 dB(W/(m2 100 MHz) to prevent interference to the sensor if it points towards the GSO. Planned scanning antenna systems will have a 3 dB higher antenna gain and therefore need a pfd limit of 146 dB(W/(m2 100 MHz). The pushbroom sensor has a sensitivity of 166 dB(W/100 MHz). As shown in Table 5, it can be protected from interference with a 147 dB(W/(m2 100 MHz) limit when pointing at the GSO if its calibrating antenna gain does not exceed 35 d