Sun Position (VSOP87)

Versión 1.1.1 (938 KB) por Meysam Mahooti
VSOP87 defines the analytical solutions to the motions of the solar system planets
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The main version of VSOP87 defines elliptic variables for the planets as a function of time. The VSOP data provides the following elliptic variables:
A the semi-major axis in Astronomic Units (AU where 1AU = 149597870.7km)
L the mean longitude
k = e cos π where e is the eccentricity and π is the longitude of the perihelion
h = e sin π
q = sin i/2 cos Ω where i is inclination and Ω is the longitude of the ascending node
p = sin i/2 sin Ω
The calculations are based on the time in Julian centuries after the J2000 epoch 2000-01-01 12:00:00.
T = (JDE - 2451545)/365250
References:
https://www.caglow.com/info/compute/vsop87
https://celestrak.org/SpaceData/EOP-All.txt

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Meysam Mahooti (2024). Sun Position (VSOP87) (https://www.mathworks.com/matlabcentral/fileexchange/77248-sun-position-vsop87), MATLAB Central File Exchange. Recuperado .

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Sun Position_VSOP87

Versión Publicado Notas de la versión
1.1.1

Mjday.m was modified.
1.1.0

test_SunPosition.m is modified.
1.0.0