grss.libgrss#
GRSS Python bindings for C++ library
Functions
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Convert cartesian state to cometary state. |
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Convert cometary state to cartesian state. |
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Calculate the difference between TAI and UTC time with TAI as the input. |
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Calculate the difference between TAI and UTC time with UTC as the input. |
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Calculate the difference between TDB and UTC time with TDB as the input. |
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Calculate the difference between TDB and UTC time with UTC as the input. |
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Calculate the inverse of a matrix using LU decomposition. |
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Propagate a simulation in parallel using OpenMP. |
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Reconstruct the state transition matrix from the flattened vector. |
Classes
The BPlaneParameters class contains parameters used for calculating the B-plane of a close approach. |
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The Body class contains the properties of an integrated or SPICE body. |
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The CloseApproachParameters class contains parameters used for calculating the close approach between two integrated or SPICE bodies. |
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The Constants class contains physical constants and conversion factors used in the GRSS orbit propagation code. |
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The Event class contains the properties of an impulsive or continuous event. |
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The ImpactParameters class contains parameters used for calculating the impact between two integrated or SPICE bodies. |
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The IntegBody class contains the properties of an integrated body. |
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The IntegrationParameters class contains parameters used in the numerical integration of the equations of motion. |
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The InterpolationParameters class contains parameters used for interpolation of the states of the integrated bodies. |
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The NongravParameters class contains constants used for calculating the non-gravitational accelerations on integrated bodies. |
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The PropSimulation class contains the orbit propagation simulation for intgrating solar system small bodies. |
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The SpiceBody class contains the properties of a SPICE body. |