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Earth, Planets and Space
Fig. 7 | Earth, Planets and Space

Fig. 7

From: Comparison of shadow models and their impact on precise orbit determination of BeiDou satellites during eclipsing phases

Fig. 7Fig. 7

a SRP acceleration variation of C10 (IGSO) in eclipse in 2019/007. b SRP acceleration variation of C14 (MEO) in eclipse in 2019/060. c SRP acceleration variation of C01 (GEO) in eclipse in 2019/069. Each figure is composed of SRP acceleration (left) and their differences (right) between other three models with regard to 3dishes. In each side of figure, including along trace direction (top), cross trace direction (middle) and radial trace direction (bottom)

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