CylindricalShadowEclipseDetector.java
/* Copyright 2022-2024 Romain Serra
* Licensed to CS GROUP (CS) under one or more
* contributor license agreements. See the NOTICE file distributed with
* this work for additional information regarding copyright ownership.
* CS licenses this file to You under the Apache License, Version 2.0
* (the "License"); you may not use this file except in compliance with
* the License. You may obtain a copy of the License at
*
* http://www.apache.org/licenses/LICENSE-2.0
*
* Unless required by applicable law or agreed to in writing, software
* distributed under the License is distributed on an "AS IS" BASIS,
* WITHOUT WARRANTIES OR CONDITIONS OF ANY KIND, either express or implied.
* See the License for the specific language governing permissions and
* limitations under the License.
*/
package org.orekit.propagation.events;
import org.hipparchus.geometry.euclidean.threed.Vector3D;
import org.hipparchus.util.FastMath;
import org.orekit.propagation.SpacecraftState;
import org.orekit.propagation.events.handlers.EventHandler;
import org.orekit.utils.PVCoordinatesProvider;
/**
* Event detector for eclipses from a single, infinitely-distant light source, occulted by a spherical central body.
* The shadow region is cylindrical, a model less accurate than a conical one but more computationally-performant.
* <p>
* The so-called g function is negative in eclipse, positive otherwise.
* </p>
* @author Romain Serra
* @see EclipseDetector
* @since 12.1
*/
public class CylindricalShadowEclipseDetector extends AbstractDetector<CylindricalShadowEclipseDetector> {
/** Direction provider for the occulted light source i.e. the Sun (whose shadow is approximated as if the body was infinitely distant). */
private final PVCoordinatesProvider sun;
/** Radius of central, occulting body (approximated as spherical).
* Its center is assumed to be at the origin of the frame linked to the state. */
private final double occultingBodyRadius;
/**
* Constructor.
* @param sun light source provider (infinitely distant)
* @param occultingBodyRadius occulting body radius
* @param maxCheck maximum check for event detection
* @param threshold threshold for event detection
* @param maxIter maximum iteration for event detection
* @param handler event handler
*/
public CylindricalShadowEclipseDetector(final PVCoordinatesProvider sun,
final double occultingBodyRadius,
final AdaptableInterval maxCheck, final double threshold,
final int maxIter, final EventHandler handler) {
super(maxCheck, threshold, maxIter, handler);
this.sun = sun;
this.occultingBodyRadius = FastMath.abs(occultingBodyRadius);
}
/**
* Constructor with default detection settings.
* @param sun light source provider
* @param occultingBodyRadius occulting body radius
* @param handler event handler
*/
public CylindricalShadowEclipseDetector(final PVCoordinatesProvider sun,
final double occultingBodyRadius, final EventHandler handler) {
this(sun, occultingBodyRadius, AdaptableInterval.of(DEFAULT_MAXCHECK), DEFAULT_THRESHOLD, DEFAULT_MAX_ITER, handler);
}
/**
* Getter for occulting body radius.
* @return radius
*/
public double getOccultingBodyRadius() {
return occultingBodyRadius;
}
/** {@inheritDoc} */
@Override
public double g(final SpacecraftState s) {
final Vector3D sunDirection = sun.getPosition(s.getDate(), s.getFrame()).normalize();
final Vector3D position = s.getPosition();
final double dotProduct = position.dotProduct(sunDirection);
if (dotProduct >= 0.) {
return position.getNorm() / occultingBodyRadius;
} else {
final double distanceToCylinderAxis = (position.subtract(sunDirection.scalarMultiply(dotProduct))).getNorm();
return distanceToCylinderAxis / occultingBodyRadius - 1.;
}
}
/** {@inheritDoc} */
@Override
protected CylindricalShadowEclipseDetector create(final AdaptableInterval newMaxCheck, final double newThreshold,
final int newMaxIter, final EventHandler newHandler) {
return new CylindricalShadowEclipseDetector(sun, occultingBodyRadius, newMaxCheck, newThreshold, newMaxIter, newHandler);
}
}