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AgEVAShadowModel Enumeration
See Also

Description

The shadow model type.

Members

MemberValueDescription
eVAShadowModelCylindrical0Cylindrical - assumes the Sun to be at infinite distance so that all light coming from the Sun moves in a direction parallel to the Sun to satellite vector.
eVAShadowModelDualCone1Dual Cone - uses the actual size and distance of the Sun to model regions of full, partial (penumbra) and zero (umbra) sunlight. The visible fraction of the solar disk is used to compute the acceleration during penumbra.
eVAShadowModelNone2None - turns off all shadowing of the satellite.
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