2020
DOI: 10.1049/iet-rsn.2020.0259
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Modelling and analysis of celestial Doppler difference velocimetry navigation considering solar characteristics

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Cited by 7 publications
(1 citation statement)
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“…However, this celestial Doppler difference measurement method changes the measurement model. Considering factors such as the overlap ratio of the zone of the direct and reflected solar light sources, the diffusion effect of the time difference of light arrival (TDOA), the direction of the solar rotation axis, the differential solar rotation, and the Lambert radiator, Liu Jin established a near-real solar difference deviation model [40][41][42]. However, due to the instability of the astronomical spectra, the spectral velocity estimation method of the ground station has some defects, such as low accuracy and instability, which affect velocimetry navigation.…”
Section: Introductionmentioning
confidence: 99%
“…However, this celestial Doppler difference measurement method changes the measurement model. Considering factors such as the overlap ratio of the zone of the direct and reflected solar light sources, the diffusion effect of the time difference of light arrival (TDOA), the direction of the solar rotation axis, the differential solar rotation, and the Lambert radiator, Liu Jin established a near-real solar difference deviation model [40][41][42]. However, due to the instability of the astronomical spectra, the spectral velocity estimation method of the ground station has some defects, such as low accuracy and instability, which affect velocimetry navigation.…”
Section: Introductionmentioning
confidence: 99%