Path: SC/Ephem
% Finds the distance to the sun and the solar flux. For moons this uses only the planetary distance. -------------------------------------------------------------------------- Form: [r, f] = PlanetaryDistanceToSun( name, jD ) -------------------------------------------------------------------------- ------ Inputs ------ name (1,:) Name of moon or planet jD (1,:) Julian date (days) ------- Outputs ------- r (1,:) Distance (au) f (1,:) Solar flux (W/m^2) --------------------------------------------------------------------------
Common: Database/Constant Common: Graphics/Plot2D Common: Time/Date2JD Math: Linear/Mag SC: Ephem/Moons SC: Ephem/PlanetPosition
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