• Acta Optica Sinica
  • Vol. 40, Issue 7, 0728001 (2020)
Bowen Guan1、2, Ning An2、*, Cunbo Fan2、3, Chengzhi Liu2、3, Guanyu Wen2, Jian Gao2, Haitao Zhang2, and Shuzhuo Miao1、2
Author Affiliations
  • 1University of Chinese Academy of Sciences, Beijing 100049, China
  • 2Changchun Observatory, National Astronomical Observatories, Chinese Academy of Sciences, Jilin, Changchun 130117, China
  • 3Key Laboratory of Space Object and Debris Observation, Purple Mountain Observatory, Chinese Academy of Sciences, Jiangsu, Nanjing 210008, China
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    DOI: 10.3788/AOS202040.0728001 Cite this Article Set citation alerts
    Bowen Guan, Ning An, Cunbo Fan, Chengzhi Liu, Guanyu Wen, Jian Gao, Haitao Zhang, Shuzhuo Miao. Satellite Signature Effects Based on the Retroreflector Uneven Distribution Model[J]. Acta Optica Sinica, 2020, 40(7): 0728001 Copy Citation Text show less
    Actual image of Lageos-1
    Fig. 1. Actual image of Lageos-1
    Reflection intensity distribution of retroreflectors in Lageos-1 with the incident angle from the north pole of satellite. (a) CoM model; (b) RUD model; (c) experiment results[12]
    Fig. 2. Reflection intensity distribution of retroreflectors in Lageos-1 with the incident angle from the north pole of satellite. (a) CoM model; (b) RUD model; (c) experiment results[12]
    Retroreflectors distribution at 70.151° latitude inLageos-1
    Fig. 3. Retroreflectors distribution at 70.151° latitude inLageos-1
    Reflected intensity of each retroreflector at 70.151° latitude in Lageos-1 with the incident angle from the north pole of satellite. (a) CoM model; (b) RUD model
    Fig. 4. Reflected intensity of each retroreflector at 70.151° latitude in Lageos-1 with the incident angle from the north pole of satellite. (a) CoM model; (b) RUD model
    Reflected intensity distribution in Lageos-1 with different laser incident angles simulated by RUD model. (a) (0°,67.5°); (b) (0°,45°); (c) (0°,22.5°); (d) (0°,0°)
    Fig. 5. Reflected intensity distribution in Lageos-1 with different laser incident angles simulated by RUD model. (a) (0°,67.5°); (b) (0°,45°); (c) (0°,22.5°); (d) (0°,0°)
    Echo signal residual distributions of Lageos-1 in SLR. (a) CoM model; (b) RUD model; (c)(d) experiment results obtained at Changchun observation
    Fig. 6. Echo signal residual distributions of Lageos-1 in SLR. (a) CoM model; (b) RUD model; (c)(d) experiment results obtained at Changchun observation
    CoM curves of Lageos-1 with changing of the laser incident angle from (0°,0°) to (0°,90°) simulated by RUD model
    Fig. 7. CoM curves of Lageos-1 with changing of the laser incident angle from (0°,0°) to (0°,90°) simulated by RUD model
    Ring numberNumber of cubesLatitude /(°)Angle between cubes /(°)
    1324.86511.250
    23213.25211.250
    33122.98211.613
    43131.23111.613
    52740.96113.333
    62350.69115.652
    71860.42130.000
    81270.15130.000
    9679.88160.000
    10190.000360.000
    Table 1. Retroreflectors distribution in Lageos-1
    ParameterValue
    Quantum efficiency of SPAD ηq0.2
    Single pulse laser energy emitted by laser E /mJ1
    Full width at half maximum τFWHM /ps50
    Efficiency of laser emission optical system Kt0.7
    Effective area of the receiving telescope Ar /m20.251
    Receiving efficiency of telescope Kr0.5
    Atmospheric transmittance (sunny weather) T0.8
    Divergence angle of emitting laser beam θt/(″)10
    Table 2. Parameters of SLR system in Changchun station
    Bowen Guan, Ning An, Cunbo Fan, Chengzhi Liu, Guanyu Wen, Jian Gao, Haitao Zhang, Shuzhuo Miao. Satellite Signature Effects Based on the Retroreflector Uneven Distribution Model[J]. Acta Optica Sinica, 2020, 40(7): 0728001
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