Package | Description |
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org.orekit.propagation.semianalytical.dsst.forces |
This package provides force models for Draper Semi-analytical Satellite Theory (DSST).
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Modifier and Type | Method and Description |
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protected abstract double[] |
AbstractGaussianContribution.getLLimits(SpacecraftState state,
AuxiliaryElements auxiliaryElements)
Compute the limits in L, the true longitude, for integration.
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protected double[] |
DSSTAtmosphericDrag.getLLimits(SpacecraftState state,
AuxiliaryElements auxiliaryElements)
Compute the limits in L, the true longitude, for integration.
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protected double[] |
DSSTSolarRadiationPressure.getLLimits(SpacecraftState state,
AuxiliaryElements auxiliaryElements)
Compute the limits in L, the true longitude, for integration.
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double[] |
DSSTZonal.getMeanElementRate(SpacecraftState spacecraftState,
AuxiliaryElements auxiliaryElements,
double[] parameters)
Computes the mean equinoctial elements rates dai / dt.
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double[] |
AbstractGaussianContribution.getMeanElementRate(SpacecraftState state,
AuxiliaryElements auxiliaryElements,
double[] parameters)
Computes the mean equinoctial elements rates dai / dt.
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double[] |
DSSTNewtonianAttraction.getMeanElementRate(SpacecraftState state,
AuxiliaryElements auxiliaryElements,
double[] parameters)
Computes the mean equinoctial elements rates dai / dt.
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double[] |
DSSTForceModel.getMeanElementRate(SpacecraftState state,
AuxiliaryElements auxiliaryElements,
double[] parameters)
Computes the mean equinoctial elements rates dai / dt.
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double[] |
DSSTTesseral.getMeanElementRate(SpacecraftState spacecraftState,
AuxiliaryElements auxiliaryElements,
double[] parameters)
Computes the mean equinoctial elements rates dai / dt.
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double[] |
DSSTThirdBody.getMeanElementRate(SpacecraftState currentState,
AuxiliaryElements auxiliaryElements,
double[] parameters)
Computes the mean equinoctial elements rates dai / dt.
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List<ShortPeriodTerms> |
DSSTZonal.initialize(AuxiliaryElements auxiliaryElements,
PropagationType type,
double[] parameters)
Performs initialization prior to propagation for the current force model.
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List<ShortPeriodTerms> |
AbstractGaussianContribution.initialize(AuxiliaryElements auxiliaryElements,
PropagationType type,
double[] parameters)
Performs initialization prior to propagation for the current force model.
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List<ShortPeriodTerms> |
DSSTNewtonianAttraction.initialize(AuxiliaryElements auxiliaryElements,
PropagationType type,
double[] parameters)
Performs initialization prior to propagation for the current force model.
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List<ShortPeriodTerms> |
DSSTForceModel.initialize(AuxiliaryElements auxiliaryElements,
PropagationType type,
double[] parameters)
Performs initialization prior to propagation for the current force model.
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List<ShortPeriodTerms> |
DSSTTesseral.initialize(AuxiliaryElements auxiliaryElements,
PropagationType type,
double[] parameters)
Performs initialization prior to propagation for the current force model.
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List<ShortPeriodTerms> |
DSSTThirdBody.initialize(AuxiliaryElements auxiliaryElements,
PropagationType type,
double[] parameters)
Computes the highest power of the eccentricity and the highest power
of a/R3 to appear in the truncated analytical power series expansion.
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