SRPTabulatedAreaVector#

class ansys.stk.core.stkobjects.astrogator.SRPTabulatedAreaVector#

Bases: IComponentInfo, ICloneable

Tabulated area vector SRP propagator function.

Overview#

Properties

`atmosphere_altitude`	Get or set the atmospheric altitude for eclipse. A simple model to account for some measure of attenuation that simply increases the shape of the Earth by the defined altitude height, often taken to be 23 km. Uses Distance Dimension.
`shadow_model`	Get or set the shadow model type.
`sun_position`	Get or set the sun position computation.
`eclipsing_bodies`	Other eclipsing bodies.
`mean_flux`	Get or set the mean solar flux at 1 au (W/m^2).
`luminosity`	Get or set the luminosity of sun. Dimensionless.
`solar_force_method`	Get or set the solar force method.
`include_boundary_mitigation`	True if shadow boundary mitigation should be performed; the state of the satellite after crossing a shadow boundary will be corrected for errors possibly caused by the sudden change in SRP which occurred during the integration step.
`use_sun_central_body_file_values`	True if solar values should come from the Sun.cb file.
`solar_radius`	Get or set the solar radius value to use in eclipse calculations. Uses Distance Dimension.
`tab_area_vector_definition_file`	Full path of the tabulated area vector definition file.
`interpolation_method`	Get or set the file interpolation method.

from ansys.stk.core.stkobjects.astrogator import SRPTabulatedAreaVector

property SRPTabulatedAreaVector.atmosphere_altitude: float#: Get or set the atmospheric altitude for eclipse. A simple model to account for some measure of attenuation that simply increases the shape of the Earth by the defined altitude height, often taken to be 23 km. Uses Distance Dimension.

property SRPTabulatedAreaVector.shadow_model: ShadowModel#: Get or set the shadow model type.

property SRPTabulatedAreaVector.sun_position: SunPosition#: Get or set the sun position computation.

property SRPTabulatedAreaVector.eclipsing_bodies: CentralBodyComponentCollection#: Other eclipsing bodies.

property SRPTabulatedAreaVector.mean_flux: float#: Get or set the mean solar flux at 1 au (W/m^2).

property SRPTabulatedAreaVector.luminosity: float#: Get or set the luminosity of sun. Dimensionless.

property SRPTabulatedAreaVector.solar_force_method: SolarForceMethod#: Get or set the solar force method.

property SRPTabulatedAreaVector.include_boundary_mitigation: bool#: True if shadow boundary mitigation should be performed; the state of the satellite after crossing a shadow boundary will be corrected for errors possibly caused by the sudden change in SRP which occurred during the integration step.

property SRPTabulatedAreaVector.use_sun_central_body_file_values: bool#: True if solar values should come from the Sun.cb file.

property SRPTabulatedAreaVector.solar_radius: float#: Get or set the solar radius value to use in eclipse calculations. Uses Distance Dimension.

property SRPTabulatedAreaVector.tab_area_vector_definition_file: str#: Full path of the tabulated area vector definition file.

property SRPTabulatedAreaVector.interpolation_method: TabVecInterpolationMethod#: Get or set the file interpolation method.