EclipticProvider.java
/* Contributed in the public domain.
* Licensed to CS Systèmes d'Information (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.frames;
import java.io.Serializable;
import org.apache.commons.math3.geometry.euclidean.threed.Rotation;
import org.apache.commons.math3.geometry.euclidean.threed.RotationConvention;
import org.apache.commons.math3.geometry.euclidean.threed.Vector3D;
import org.orekit.errors.OrekitException;
import org.orekit.errors.OrekitInternalError;
import org.orekit.time.AbsoluteDate;
import org.orekit.time.TimeFunction;
import org.orekit.utils.IERSConventions;
/**
* An inertial frame aligned with the ecliptic.
* <p>
* The IAU defines the ecliptic as "the plane perpendicular to the mean heliocentric
* orbital angular momentum vector of the Earth-Moon barycentre in the BCRS (IAU 2006
* Resolution B1)." The +z axis is aligned with the angular momentum vector, and the +x
* axis is aligned with +x axis of {@link FramesFactory#getMOD(IERSConventions) MOD}.
* </p>
*
* <p>
* This implementation agrees with the JPL 406 ephemerides to within 0.5 arc seconds.
* </p>
*
* @since 7.0
*/
public class EclipticProvider implements TransformProvider {
/** Serializable UID. */
private static final long serialVersionUID = 20140516L;
/** IERS conventions. */
private final IERSConventions conventions;
/** the obliquity of the ecliptic, in radians as a function of time. */
private final transient TimeFunction<Double> obliquity;
/**
* Create a transform provider from MOD to an ecliptically aligned frame.
* @param conventions IERS conventions
* @throws OrekitException if the mean obliquity of the ecliptic function can not be
* loaded.
*/
public EclipticProvider(final IERSConventions conventions) throws OrekitException {
this.conventions = conventions;
this.obliquity = conventions.getMeanObliquityFunction();
}
@Override
public Transform getTransform(final AbsoluteDate date) throws OrekitException {
//mean obliquity of date
final double epsA = obliquity.value(date);
return new Transform(date, new Rotation(Vector3D.MINUS_I, epsA, RotationConvention.VECTOR_OPERATOR));
}
/** Replace the instance with a data transfer object for serialization.
* <p>
* This intermediate class serializes only the frame key.
* </p>
* @return data transfer object that will be serialized
*/
private Object writeReplace() {
return new DataTransferObject(conventions);
}
/** Internal class used only for serialization. */
private static class DataTransferObject implements Serializable {
/** Serializable UID. */
private static final long serialVersionUID = 20140516L;
/** IERS conventions. */
private final IERSConventions conventions;
/** Simple constructor.
* @param conventions IERS conventions
*/
DataTransferObject(final IERSConventions conventions) {
this.conventions = conventions;
}
/** Replace the deserialized data transfer object with a {@link EclipticProvider}.
* @return replacement {@link EclipticProvider}
*/
private Object readResolve() {
try {
// retrieve a transform
return new EclipticProvider(conventions);
} catch (OrekitException oe) {
throw new OrekitInternalError(oe);
}
}
}
}