FieldApsideDetector.java
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package org.orekit.propagation.events;
import org.hipparchus.CalculusFieldElement;
import org.hipparchus.geometry.euclidean.threed.FieldVector3D;
import org.hipparchus.ode.events.Action;
import org.orekit.orbits.FieldOrbit;
import org.orekit.propagation.FieldSpacecraftState;
import org.orekit.propagation.events.handlers.FieldEventHandler;
import org.orekit.propagation.events.handlers.FieldStopOnIncreasing;
import org.orekit.utils.FieldPVCoordinates;
/** Finder for apside crossing events.
* <p>This class finds apside crossing events (i.e. apogee or perigee crossing).</p>
* <p>The default implementation behavior is to {@link Action#CONTINUE continue}
* propagation at apogee crossing and to {@link Action#STOP stop} propagation
* at perigee crossing. This can be changed by calling
* {@link #withHandler(FieldEventHandler)} after construction.</p>
* <p>Beware that apside detection will fail for almost circular orbits. If
* for example an apside detector is used to trigger an {@link
* org.orekit.forces.maneuvers.ImpulseManeuver ImpulseManeuver} and the maneuver
* change the orbit shape to circular, then the detector may completely fail just
* after the maneuver has been performed!</p>
* @see org.orekit.propagation.FieldPropagator#addEventDetector(FieldEventDetector)
* @author Luc Maisonobe
* @param <T> type of the field elements
*/
public class FieldApsideDetector<T extends CalculusFieldElement<T>> extends FieldAbstractDetector<FieldApsideDetector<T>, T> {
/** Build a new instance.
* <p>The Keplerian period is used only to set an upper bound for the
* max check interval to period/3 and to set the convergence threshold.</p>
* @param keplerianPeriod estimate of the Keplerian period
* @since 12.1
*/
public FieldApsideDetector(final T keplerianPeriod) {
super(new FieldEventDetectionSettings<>(keplerianPeriod.divide(3).getReal(), keplerianPeriod.multiply(1e-13),
DEFAULT_MAX_ITER), new FieldStopOnIncreasing<>());
}
/** Build a new instance.
* <p>The orbit is used only to set an upper bound for the
* max check interval to period/3 and to set the convergence
* threshold according to orbit size</p>
* @param orbit initial orbit
*/
public FieldApsideDetector(final FieldOrbit<T> orbit) {
this(orbit.getKeplerianPeriod());
}
/** Build a new instance.
* <p>The orbit is used only to set an upper bound for the
* max check interval to period/3</p>
* @param threshold convergence threshold (s)
* @param orbit initial orbit
*/
public FieldApsideDetector(final T threshold, final FieldOrbit<T> orbit) {
super(new FieldEventDetectionSettings<>(orbit.getKeplerianPeriod().divide(3).getReal(), threshold,
DEFAULT_MAX_ITER), new FieldStopOnIncreasing<>());
}
/** Constructor with full parameters.
* <p>
* This constructor is public because otherwise all accessible ones would require an orbit.
* </p>
* @param detectionSettings event detection settings
* @param handler event handler to call at event occurrences
* @since 13.0
*/
public FieldApsideDetector(final FieldEventDetectionSettings<T> detectionSettings,
final FieldEventHandler<T> handler) {
super(detectionSettings, handler);
}
/** {@inheritDoc} */
@Override
protected FieldApsideDetector<T> create(final FieldEventDetectionSettings<T> detectionSettings,
final FieldEventHandler<T> newHandler) {
return new FieldApsideDetector<>(detectionSettings, newHandler);
}
/** Compute the value of the switching function.
* This function computes the dot product of the 2 vectors : position.velocity.
* @param s the current state information: date, kinematics, attitude
* @return value of the switching function
*/
public T g(final FieldSpacecraftState<T> s) {
final FieldPVCoordinates<T> pv = s.getPVCoordinates();
return FieldVector3D.dotProduct(pv.getPosition(), pv.getVelocity());
}
}