public class IsotropicRadiationClassicalConvention extends Object implements RadiationSensitive
This model uses the classical thermo-optical coefficients Ca for absorption, Cs for specular reflection and Kd for diffuse reflection. The equation Ca + Cs + Cd = 1 always holds.
A less standard set of coefficients α = Ca for absorption and
τ = Cs/(1-Ca) for specular reflection is implemented in the sister
class IsotropicRadiationCNES95Convention.
BoxAndSolarArraySpacecraft,
IsotropicDrag,
IsotropicRadiationCNES95ConventionABSORPTION_COEFFICIENT, REFLECTION_COEFFICIENT| Constructor and Description |
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IsotropicRadiationClassicalConvention(double crossSection,
double ca,
double cs)
Simple constructor.
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| Modifier and Type | Method and Description |
|---|---|
ParameterDriver[] |
getRadiationParametersDrivers()
Get the drivers for supported parameters.
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org.hipparchus.geometry.euclidean.threed.FieldVector3D<org.hipparchus.analysis.differentiation.DerivativeStructure> |
radiationPressureAcceleration(AbsoluteDate date,
Frame frame,
org.hipparchus.geometry.euclidean.threed.FieldVector3D<org.hipparchus.analysis.differentiation.DerivativeStructure> position,
org.hipparchus.geometry.euclidean.threed.FieldRotation<org.hipparchus.analysis.differentiation.DerivativeStructure> rotation,
org.hipparchus.analysis.differentiation.DerivativeStructure mass,
org.hipparchus.geometry.euclidean.threed.FieldVector3D<org.hipparchus.analysis.differentiation.DerivativeStructure> flux)
Compute the acceleration due to radiation pressure, with state derivatives.
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org.hipparchus.geometry.euclidean.threed.Vector3D |
radiationPressureAcceleration(AbsoluteDate date,
Frame frame,
org.hipparchus.geometry.euclidean.threed.Vector3D position,
org.hipparchus.geometry.euclidean.threed.Rotation rotation,
double mass,
org.hipparchus.geometry.euclidean.threed.Vector3D flux)
Compute the acceleration due to radiation pressure.
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org.hipparchus.geometry.euclidean.threed.FieldVector3D<org.hipparchus.analysis.differentiation.DerivativeStructure> |
radiationPressureAcceleration(AbsoluteDate date,
Frame frame,
org.hipparchus.geometry.euclidean.threed.Vector3D position,
org.hipparchus.geometry.euclidean.threed.Rotation rotation,
double mass,
org.hipparchus.geometry.euclidean.threed.Vector3D flux,
String paramName)
Compute the acceleration due to radiation pressure, with parameters derivatives.
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clone, equals, finalize, getClass, hashCode, notify, notifyAll, toString, wait, wait, waitgetAbsorptionCoefficient, getRadiationParametersNames, getReflectionCoefficient, setAbsorptionCoefficient, setReflectionCoefficientpublic IsotropicRadiationClassicalConvention(double crossSection,
double ca,
double cs)
crossSection - Surface (m²)ca - absorption coefficient Ca between 0.0 an 1.0cs - specular reflection coefficient Cs between 0.0 an 1.0public ParameterDriver[] getRadiationParametersDrivers()
getRadiationParametersDrivers in interface RadiationSensitivepublic org.hipparchus.geometry.euclidean.threed.Vector3D radiationPressureAcceleration(AbsoluteDate date, Frame frame, org.hipparchus.geometry.euclidean.threed.Vector3D position, org.hipparchus.geometry.euclidean.threed.Rotation rotation, double mass, org.hipparchus.geometry.euclidean.threed.Vector3D flux)
radiationPressureAcceleration in interface RadiationSensitivedate - current dateframe - inertial reference frame for state (both orbit and attitude)position - position of spacecraft in reference framerotation - orientation (attitude) of the spacecraft with respect to reference framemass - current massflux - radiation flux in the same inertial frame as spacecraft orbitpublic org.hipparchus.geometry.euclidean.threed.FieldVector3D<org.hipparchus.analysis.differentiation.DerivativeStructure> radiationPressureAcceleration(AbsoluteDate date, Frame frame, org.hipparchus.geometry.euclidean.threed.FieldVector3D<org.hipparchus.analysis.differentiation.DerivativeStructure> position, org.hipparchus.geometry.euclidean.threed.FieldRotation<org.hipparchus.analysis.differentiation.DerivativeStructure> rotation, org.hipparchus.analysis.differentiation.DerivativeStructure mass, org.hipparchus.geometry.euclidean.threed.FieldVector3D<org.hipparchus.analysis.differentiation.DerivativeStructure> flux)
radiationPressureAcceleration in interface RadiationSensitivedate - current dateframe - inertial reference frame for state (both orbit and attitude)position - position of spacecraft in reference framerotation - orientation (attitude) of the spacecraft with respect to reference framemass - spacecraft massflux - radiation flux in the same inertial frame as spacecraft orbitpublic org.hipparchus.geometry.euclidean.threed.FieldVector3D<org.hipparchus.analysis.differentiation.DerivativeStructure> radiationPressureAcceleration(AbsoluteDate date, Frame frame, org.hipparchus.geometry.euclidean.threed.Vector3D position, org.hipparchus.geometry.euclidean.threed.Rotation rotation, double mass, org.hipparchus.geometry.euclidean.threed.Vector3D flux, String paramName) throws OrekitException
radiationPressureAcceleration in interface RadiationSensitivedate - current dateframe - inertial reference frame for state (both orbit and attitude)position - position of spacecraft in reference framerotation - orientation (attitude) of the spacecraft with respect to reference framemass - current massflux - radiation flux in the same inertial frame as spacecraft orbitparamName - name of the parameter with respect to which derivatives are requiredOrekitException - if acceleration cannot be computedCopyright © 2002-2017 CS Systèmes d'information. All rights reserved.