Satellite fast high-precision extrapolation method of great-eccentricity track
An eccentricity and high-precision technology, applied in the field of satellite orbits, can solve the problem of large fitting errors of orbit extrapolation algorithms on satellites
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[0038] Such as figure 1 As shown, the specific implementation of the present invention includes the following steps:
[0039] (1) Solve the X, Y, and Z three-axis position difference between the precision orbit of the large eccentricity elliptical orbit and the two-body orbit on the ground, and then use the Chebyshev polynomial fitting method to obtain the Chebyshev polynomial coefficients;
[0040] Chebyshev polynomial fitting is to fit a function according to the given data, so that the variance sum between the function value at a given point and the given value is the smallest, and the function is composed of Chebyshev polynomials as the basis function The function.
[0041] The precise orbit refers to the actual orbit of the satellite, which is provided by ground orbit measurement. The two-body orbit refers to the ideal orbit of the satellite only under the gravitational force of the center of the target celestial body, which is obtained by theoretical calculation; the in...
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