fr.cnes.sirius.patrius.forces.gravity.tides

Class TerrestrialTides

java.lang.Object

fr.cnes.sirius.patrius.math.parameter.Parameterizable

fr.cnes.sirius.patrius.math.parameter.JacobiansParameterizable

fr.cnes.sirius.patrius.forces.gravity.tides.AbstractTides

fr.cnes.sirius.patrius.forces.gravity.tides.TerrestrialTides

All Implemented Interfaces:

ForceModel, GradientModel, PotentialTimeVariations, IJacobiansParameterizable, IParameterizable, Serializable

public class TerrestrialTides
extends AbstractTides

This class implements the perturbating force due to terrestrial tides (deformation due to third body attraction on an aneslatic crust, ellipticity correction, frequency correction). It is possible to activate/deactivate one of these corrections. At least the model take into account the deformation due to the moon and the sun attraction up to degree 2.

The implementation of this class enables the computation of partial derivatives by finite differences with respect to the central attraction coefficient.

Since:

1.1

Version:

$Id: TerrestrialTides.java 17582 2017-05-10 12:58:16Z bignon $

Author:

Julie Anton, Gerald Mercadier

See Also:

Serialized Form

Concurrency :

not thread-safe

Concurrency comment :

not thread safe because of the method updateCoefficientsCandS().

Field Summary

Fields inherited from class fr.cnes.sirius.patrius.forces.gravity.tides.AbstractTides

bodyFrame, coefficientsC, coefficientsCPD, coefficientsS, coefficientsSPD, MU, paramAe, paramMu, RADIUS

Constructor Summary

Constructors

Constructor and Description
TerrestrialTides(Frame centralBodyFrame, double equatorialRadius, double mu) Creates a new instance.
TerrestrialTides(Frame centralBodyFrame, double equatorialRadius, double mu, boolean computePD) Creates a new instance.
TerrestrialTides(Frame centralBodyFrame, double equatorialRadius, double mu, List<CelestialBody> bodies, boolean thirdBodyAttDegree3, boolean frequencyCorr, boolean ellipticityCorr, ITerrestrialTidesDataProvider terrestrialData) Creates a new instance.
TerrestrialTides(Frame centralBodyFrame, double equatorialRadius, double mu, List<CelestialBody> bodies, boolean thirdBodyAttDegree3, boolean frequencyCorr, boolean ellipticityCorr, ITerrestrialTidesDataProvider terrestrialData, boolean computePD) Creates a new instance.
TerrestrialTides(Frame centralBodyFrame, Parameter equatorialRadius, Parameter mu) Creates a new instance.
TerrestrialTides(Frame centralBodyFrame, Parameter equatorialRadius, Parameter mu, boolean computePD) Creates a new instance.
TerrestrialTides(Frame centralBodyFrame, Parameter equatorialRadius, Parameter mu, List<CelestialBody> bodies, boolean thirdBodyAttDegree3, boolean frequencyCorr, boolean ellipticityCorr, ITerrestrialTidesDataProvider terrestrialData) Creates a new instance using Parameter.
TerrestrialTides(Frame centralBodyFrame, Parameter equatorialRadius, Parameter mu, List<CelestialBody> bodies, boolean thirdBodyAttDegree3, boolean frequencyCorr, boolean ellipticityCorr, ITerrestrialTidesDataProvider terrestrialData, boolean computePD) Creates a new instance using Parameter.

Method Summary

Methods

Modifier and Type	Method and Description
boolean	computeGradientPosition() This method returns true if the acceleration partial derivatives with respect to position have to be computed.
void	updateCoefficientsCandS(AbsoluteDate date) Update the C and the S coefficients for acceleration computation.
void	updateCoefficientsCandSPD(AbsoluteDate date) Update the C and the S coefficients for partial derivatives computation.

Methods inherited from class fr.cnes.sirius.patrius.forces.gravity.tides.AbstractTides

addContribution, addDAccDParam, addDAccDState, computeAcceleration, computeAcceleration, computeGradientVelocity, getEventsDetectors

Methods inherited from class fr.cnes.sirius.patrius.math.parameter.JacobiansParameterizable

addJacobiansParameter, addJacobiansParameter, addJacobiansParameter, supportsJacobianParameter

Methods inherited from class fr.cnes.sirius.patrius.math.parameter.Parameterizable

addParameter, getParameters, supportsParameter

Methods inherited from class java.lang.Object

clone, equals, finalize, getClass, hashCode, notify, notifyAll, toString, wait, wait, wait

Methods inherited from interface fr.cnes.sirius.patrius.math.parameter.IParameterizable

getParameters, supportsParameter

Constructor Detail

TerrestrialTides

public TerrestrialTides(Frame centralBodyFrame,
                double equatorialRadius,
                double mu,
                List<CelestialBody> bodies,
                boolean thirdBodyAttDegree3,
                boolean frequencyCorr,
                boolean ellipticityCorr,
                ITerrestrialTidesDataProvider terrestrialData)
                 throws PatriusException

Creates a new instance. It is possible to consider several perturbing bodies. The correction due to the tidal potential is taken into account up to degree 2 and 3 if it is specified by the user. It is also possible to activate the frequency correction and the ellipticity correction.

Parameters:

centralBodyFrame - rotating body frame

equatorialRadius - reference equatorial radius of the potential

mu - central body attraction coefficient (m³/s²)

bodies - perturbing bodies

thirdBodyAttDegree3 - if true the perturbation of tidal potential are taken into account up to degree 3

frequencyCorr - if true the frequency correction is applied

ellipticityCorr - if true the ellipticity correction is applied

terrestrialData - terrestrial tide data

Throws:

IllegalArgumentException - if coefficients array do not match

PatriusException - if a perturbing celestial body cannot be built

TerrestrialTides

public TerrestrialTides(Frame centralBodyFrame,
                double equatorialRadius,
                double mu,
                List<CelestialBody> bodies,
                boolean thirdBodyAttDegree3,
                boolean frequencyCorr,
                boolean ellipticityCorr,
                ITerrestrialTidesDataProvider terrestrialData,
                boolean computePD)
                 throws PatriusException

Creates a new instance. It is possible to consider several perturbing bodies. The correction due to the tidal potential is taken into account up to degree 2 and 3 if it is specified by the user. It is also possible to activate the frequency correction and the ellipticity correction.

Parameters:

centralBodyFrame - rotating body frame

equatorialRadius - reference equatorial radius of the potential

mu - central body attraction coefficient (m³/s²)

bodies - perturbing bodies

thirdBodyAttDegree3 - if true the perturbation of tidal potential are taken into account up to degree 3

frequencyCorr - if true the frequency correction is applied

ellipticityCorr - if true the ellipticity correction is applied

terrestrialData - terrestrial tide data

computePD - if partial derivatives wrt position have to be computed

Throws:

IllegalArgumentException - if coefficients array do not match

PatriusException - if a perturbing celestial body cannot be built

TerrestrialTides

public TerrestrialTides(Frame centralBodyFrame,
                Parameter equatorialRadius,
                Parameter mu,
                List<CelestialBody> bodies,
                boolean thirdBodyAttDegree3,
                boolean frequencyCorr,
                boolean ellipticityCorr,
                ITerrestrialTidesDataProvider terrestrialData)
                 throws PatriusException

Creates a new instance using Parameter. It is possible to consider several perturbing bodies. The correction due to the tidal potential is taken into account up to degree 2 and 3 if it is specified by the user. It is also possible to activate the frequency correction and the ellipticity correction.

Parameters:

centralBodyFrame - rotating body frame

equatorialRadius - reference equatorial radius of the potential parameter

mu - central body attraction coefficient (m³/s²) parameter

bodies - perturbing bodies

thirdBodyAttDegree3 - if true the perturbation of tidal potential are taken into account up to degree 3

frequencyCorr - if true the frequency correction is applied

ellipticityCorr - if true the ellipticity correction is applied

terrestrialData - terrestrial tide data

Throws:

IllegalArgumentException - if coefficients array do not match

PatriusException - if a perturbing celestial body cannot be built

TerrestrialTides

public TerrestrialTides(Frame centralBodyFrame,
                Parameter equatorialRadius,
                Parameter mu,
                List<CelestialBody> bodies,
                boolean thirdBodyAttDegree3,
                boolean frequencyCorr,
                boolean ellipticityCorr,
                ITerrestrialTidesDataProvider terrestrialData,
                boolean computePD)
                 throws PatriusException

Creates a new instance using Parameter. It is possible to consider several perturbing bodies. The correction due to the tidal potential is taken into account up to degree 2 and 3 if it is specified by the user. It is also possible to activate the frequency correction and the ellipticity correction.

Parameters:

centralBodyFrame - rotating body frame

equatorialRadius - reference equatorial radius of the potential as a parameter

mu - central body attraction coefficient (m³/s²) as a parameter

bodies - perturbing bodies

thirdBodyAttDegree3 - if true the perturbation of tidal potential are taken into account up to degree 3

frequencyCorr - if true the frequency correction is applied

ellipticityCorr - if true the ellipticity correction is applied

terrestrialData - terrestrial tide data

computePD - true if partial derivatives wrt position have to be computed

Throws:

IllegalArgumentException - if coefficients array do not match

PatriusException - if a perturbing celestial body cannot be built

TerrestrialTides

public TerrestrialTides(Frame centralBodyFrame,
                double equatorialRadius,
                double mu)
                 throws PatriusException

Creates a new instance. The perturbating bodies are the moon and the sun. This constructor takes into account all of the corrections.

Parameters:

centralBodyFrame - rotating body frame

equatorialRadius - reference equatorial radius of the potential

mu - central body attraction coefficient (m³/s²)

Throws:

IllegalArgumentException - if coefficients array do not match

PatriusException - if a perturbing celestial body cannot be built

TerrestrialTides

public TerrestrialTides(Frame centralBodyFrame,
                double equatorialRadius,
                double mu,
                boolean computePD)
                 throws PatriusException

Creates a new instance. The perturbating bodies are the moon and the sun. This constructor takes into account all of the corrections.

Parameters:

centralBodyFrame - rotating body frame

equatorialRadius - reference equatorial radius of the potential

mu - central body attraction coefficient (m³/s²)

computePD - true if partial derivatives wrt position have to be computed

Throws:

IllegalArgumentException - if coefficients array do not match

PatriusException - if a perturbing celestial body cannot be built

TerrestrialTides

public TerrestrialTides(Frame centralBodyFrame,
                Parameter equatorialRadius,
                Parameter mu)
                 throws PatriusException

Creates a new instance. The perturbating bodies are the moon and the sun. This constructor takes into account all of the corrections.

Parameters:

centralBodyFrame - rotating body frame

equatorialRadius - reference equatorial radius of the potential parameter

mu - central body attraction coefficient (m³/s²) parameter

Throws:

IllegalArgumentException - if coefficients array do not match

PatriusException - if a perturbing celestial body cannot be built

TerrestrialTides

public TerrestrialTides(Frame centralBodyFrame,
                Parameter equatorialRadius,
                Parameter mu,
                boolean computePD)
                 throws PatriusException

Creates a new instance. The perturbating bodies are the moon and the sun. This constructor takes into account all of the corrections.

Parameters:

centralBodyFrame - rotating body frame

equatorialRadius - reference equatorial radius of the potential parameter

mu - central body attraction coefficient (m³/s²) parameter

computePD - true if partial derivatives have to be computed

Throws:

IllegalArgumentException - if coefficients array do not match

PatriusException - if a perturbing celestial body cannot be built

Method Detail

updateCoefficientsCandS

public void updateCoefficientsCandS(AbsoluteDate date)
                             throws PatriusException

Update the C and the S coefficients for acceleration computation.

Specified by:

updateCoefficientsCandS in interface PotentialTimeVariations

Specified by:

updateCoefficientsCandS in class AbstractTides

Parameters:

date - : date

Throws:

PatriusException - if position cannot be computed in given frame

updateCoefficientsCandSPD

public void updateCoefficientsCandSPD(AbsoluteDate date)
                               throws PatriusException

Update the C and the S coefficients for partial derivatives computation.

Specified by:

updateCoefficientsCandSPD in interface PotentialTimeVariations

Specified by:

updateCoefficientsCandSPD in class AbstractTides

Parameters:

date - : date

Throws:

PatriusException - if position cannot be computed in given frame

computeGradientPosition

public boolean computeGradientPosition()

This method returns true if the acceleration partial derivatives with respect to position have to be computed.

Returns:

true if the derivatives have to be computed, false otherwise