Method for determining relative orbit elements based on inter-satellite distance
A technology of relative orbit and inter-satellite distance, applied in three-dimensional position/channel control, etc., can solve the problems of too much measurement information and low precision, and achieve the effect of improving calculation accuracy and high engineering application value
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[0124] The present invention takes the two-star formation flight system as an example for analysis. The master and slave stars are respectively distributed on two orbital planes. The orbital semi-major axis a in the orbital elements of the two orbitals is 标称 , eccentricity e 标称 , inclination i 标称 are the same, but the right ascension of ascending node Ω and the argument of latitude u are different. Take the orbital semi-major axis a 标称 =7478.137km, eccentricity e 标称 = 0, orbital inclination i 标称 =63.43°, argument of perigee ω 标称 =45°, the relative right ascension of the ascending node is ΔΩ=0.8764°, and the relative latitude angle is Δu=0.0602°. In the case of no perturbation, the configuration of the formation flight system remains unchanged at the equator and the north and south poles, and the star distance at the equator The distance between the stars is Δx at the two poles 标称 =59km, such as Figure 5 As shown, there is exactly formation angle β=30° at this moment....
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