ThirdBodyAttractionEpoch.java
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package org.orekit.forces.gravity;
import org.hipparchus.analysis.differentiation.Gradient;
import org.hipparchus.geometry.euclidean.threed.FieldVector3D;
import org.hipparchus.geometry.euclidean.threed.Vector3D;
import org.orekit.bodies.CelestialBody;
import org.orekit.propagation.SpacecraftState;
/** Third body attraction force model.
* This class is a copy of {@link ThirdBodyAttraction} class.
* The computation of derivatives of the acceleration
* w.r.t. the Epoch has been added.
*
* @author Fabien Maussion
* @author Véronique Pommier-Maurussane
* @since 10.2
*/
public class ThirdBodyAttractionEpoch extends ThirdBodyAttraction {
/** The body to consider. */
private final CelestialBody body;
/** Simple constructor.
* @param body the third body to consider
* (ex: {@link org.orekit.bodies.CelestialBodyFactory#getSun()} or
* {@link org.orekit.bodies.CelestialBodyFactory#getMoon()})
*/
public ThirdBodyAttractionEpoch(final CelestialBody body) {
super(body);
this.body = body;
}
/** Compute acceleration.
* @param s current state information: date, kinematics, attitude
* @param parameters values of the force model parameters
* @return acceleration in same frame as state
*/
private FieldVector3D<Gradient> accelerationToEpoch(final SpacecraftState s, final double[] parameters) {
final double gm = parameters[0];
// compute bodies separation vectors and squared norm
final Vector3D centralToBody = body.getPVCoordinates(s.getDate(), s.getFrame()).getPosition();
// Spacecraft Position
final double rx = centralToBody.getX();
final double ry = centralToBody.getY();
final double rz = centralToBody.getZ();
final int freeParameters = 3;
final Gradient fpx = Gradient.variable(freeParameters, 0, rx);
final Gradient fpy = Gradient.variable(freeParameters, 1, ry);
final Gradient fpz = Gradient.variable(freeParameters, 2, rz);
final FieldVector3D<Gradient> centralToBodyFV = new FieldVector3D<>(new Gradient[] {fpx, fpy, fpz});
final Gradient r2Central = centralToBodyFV.getNormSq();
final FieldVector3D<Gradient> satToBody = centralToBodyFV.subtract(s.getPVCoordinates().getPosition());
final Gradient r2Sat = satToBody.getNormSq();
return new FieldVector3D<>(gm, satToBody.scalarMultiply(r2Sat.multiply(r2Sat.sqrt()).reciprocal()),
-gm, centralToBodyFV.scalarMultiply(r2Central.multiply(r2Central.sqrt()).reciprocal()));
}
/** Compute derivatives of the state w.r.t epoch.
* @param s current state information: date, kinematics, attitude
* @param parameters values of the force model parameters
* @return derivatives
*/
public double[] getDerivativesToEpoch(final SpacecraftState s, final double[] parameters) {
final FieldVector3D<Gradient> acc = accelerationToEpoch(s, parameters);
final Vector3D centralToBodyVelocity = body.getPVCoordinates(s.getDate(), s.getFrame()).getVelocity();
final double[] dAccxdR1i = acc.getX().getGradient();
final double[] dAccydR1i = acc.getY().getGradient();
final double[] dAcczdR1i = acc.getZ().getGradient();
final double[] v = centralToBodyVelocity.toArray();
return new double[] {dAccxdR1i[0] * v[0] + dAccxdR1i[0] * v[1] + dAccxdR1i[0] * v[2],
dAccydR1i[0] * v[0] + dAccydR1i[0] * v[1] + dAccydR1i[0] * v[2],
dAcczdR1i[0] * v[0] + dAcczdR1i[0] * v[1] + dAcczdR1i[0] * v[2]};
}
}