Method for simulating solar motion
A technology for simulating the sun and the sun. It is applied in the field of simulating object motion and simulating solar motion. It can solve the problems of reducing model unreliability, increasing the pressure of satellite remote control channels, and being unable to eliminate model truncation errors. It achieves the effect of small errors and simple calculations.
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Embodiment 1
[0030] see figure 1 , the invention discloses a method for simulating solar motion, the method comprising the steps of:
[0031] Step A. Obtaining the true celestial longitude of the sun and the flat celestial longitude of the sun in the set time period. The solar true celestial longitude and the solar flat celestial longitude of the set time period can be obtained through accurate models or forecasts from authoritative departments.
[0032] Step B. Analyzing and comparing the above two sets of data to obtain the fluctuation curve of the Taiyangzhenhuang meridian relative to the Taiyangpinghuang meridian in the time period.
[0033] Step C, according to the satellite attitude determination accuracy requirements, the fluctuation curve is fitted, and the obtained solar eclipse longitude U S ; s = M 0 +k 1 d+k 2 sin(2π / 365.25d); where, M 0 is a known moment t 0 The true celestial longitude of the sun; d=t / (24*3600), t is relative to t 0 time; k 1 , k 2 is the coefficie...
Embodiment 2
[0040] In the present embodiment, the method for simulating solar motion comprises the steps:
[0041] Step A', obtain the solar true celestial longitude and the solar flat celestial longitude of each day between 0:00 on January 1, 2007 and 0:00 on January 1, 2015 through an accurate model or the forecast of an authoritative department.
[0042] Step B', analyze and compare the two sets of data, and obtain the fluctuation curve of the true yellow meridian of the sun relative to the flat yellow meridian of the sun during the time period from 0:00 on January 1, 2007 to 0:0 on January 1, 2015; the fluctuation curve Such as figure 2 shown.
[0043] Step C', according to the satellite attitude determination accuracy requirements, the fluctuation curve is fitted. The accuracy of attitude determination using satellites is required to be 0.5 degrees, and only one fitting is required. Taking the true yellow meridian at 0:0 on January 5, 2008 as the starting point, the fitting analy...
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