• Acta Optica Sinica
  • Vol. 39, Issue 6, 0628003 (2019)
Junfeng Xie1、2, Fan Mo1、*, Huai Wang1, Xiang Li1、2, and Hong Zhu1
Author Affiliations
  • 1 Land Satellite Remote Sensing Application Center, Ministry of Natural Resources, Beijing 100048, China
  • 2 School of Surveying and Geographical Science, Liaoning Technical University, Fuxin, Liaoning 123000, China
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    DOI: 10.3788/AOS201939.0628003 Cite this Article Set citation alerts
    Junfeng Xie, Fan Mo, Huai Wang, Xiang Li, Hong Zhu. Jitter Detection of ZY3-02 Satellite Platform Using Phase-Correlation Registration Based on Symmetrical Energy Distribution[J]. Acta Optica Sinica, 2019, 39(6): 0628003 Copy Citation Text show less
    Schematic of multi-spectral camera imaging on ZY3-02 satellite
    Fig. 1. Schematic of multi-spectral camera imaging on ZY3-02 satellite
    Installation relation among CCDs at different spectral bands in multi-spectral camera
    Fig. 2. Installation relation among CCDs at different spectral bands in multi-spectral camera
    Schematic of energy peak calculation
    Fig. 3. Schematic of energy peak calculation
    Schematic of jitter detection of satellite platform. (a) b-band camera scanned ground point O at moment t1; (b) a-band camera scanned ground point O at moment t2
    Fig. 4. Schematic of jitter detection of satellite platform. (a) b-band camera scanned ground point O at moment t1; (b) a-band camera scanned ground point O at moment t2
    Images of registration error acquired form simulation data. (a) PC; (b) PF; (c) SC; (d) SF; (e) SVD; (f) UP
    Fig. 5. Images of registration error acquired form simulation data. (a) PC; (b) PF; (c) SC; (d) SF; (e) SVD; (f) UP
    Jitter curves detected from on-orbit data using different algorithms
    Fig. 6. Jitter curves detected from on-orbit data using different algorithms
    Experimental scheme
    Fig. 7. Experimental scheme
    Parallax images between blue and green spectra. (a) Track 718; (b) track 1379; (c) track 11229; (d) track 11365
    Fig. 8. Parallax images between blue and green spectra. (a) Track 718; (b) track 1379; (c) track 11229; (d) track 11365
    Satellite attitude data verify platform jitter. (a) Track 718; (b) track 1379; (c) track 11229; (d) track 11365
    Fig. 9. Satellite attitude data verify platform jitter. (a) Track 718; (b) track 1379; (c) track 11229; (d) track 11365
    Satellite or sensorLaunch yearFrequencya /HzAmplitudeb /m
    ISS[22-23]19930.01-300.00-
    ETS-VI[13]19940.39-250.00-
    MOC-NA[3]19961-4≈15
    ASTER[4,24-25]19991.5-1.66-7
    QuickBird [4]20011.0, 4.32.5, 0.1
    SPOT 5[4]2002≈0.003≈20
    ALSat-1[26]20020.5-
    Nigeria Sat[26]20030.5-
    UK-DMC[26]20030.6-
    MEX-HRSC[27-28]20030.1-0.2, 1.78
    HiRISE[4,29]2005≈1.6≈1
    Beijing-1[30]20052003
    ALOS[31-32]20066-7, 60-701000, 100
    Kompsat-2[33]20062100.14
    LROC[29,34]200960.1-1.0
    Mapping Satellite-1[35]20100.105, 0.635, 4.0000.2, 0.1, 0.1
    Pleiades-HR[22]201170.9-78.40.14
    ZY3-01[5,10,12,36-37]20120.6-0.72.5-7.5
    Yaogan-26[6]2014100, 200, 3000.1, 0.1, 0.1
    aSatellite attitude jitter frequency may be detected in roll, pitch, or both; the information listed here are from either or both. bThe amplitude has been transformed from on-orbit arcsec or pixel to ground meter (from satellite to ground), which can show the influence of jitter intuitively. Amplitudes not listed in existing records and research are indicated by “-”.
    Table 1. Jitter frequency and amplitude of different satellite platforms
    AlgorithmError /pixel
    MeanRMSE
    PC-0.0070.046
    PF0.0680.088
    SC0.0320.060
    SF0.0690.089
    SVD0.1430.156
    UP-0.0780.085
    Table 2. Statistics of registration error acquired form simulation data
    Track IDFrequency /HzAmplitude /s
    7180.630.99
    13790.631.12
    112290.650.41
    113650.650.97
    Table 3. Jitter information for experimental data
    Junfeng Xie, Fan Mo, Huai Wang, Xiang Li, Hong Zhu. Jitter Detection of ZY3-02 Satellite Platform Using Phase-Correlation Registration Based on Symmetrical Energy Distribution[J]. Acta Optica Sinica, 2019, 39(6): 0628003
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