EcksteinHechlerPropagator.java
/* Copyright 2002-2023 CS GROUP
* 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
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* Unless required by applicable law or agreed to in writing, software
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package org.orekit.propagation.analytical;
import java.io.Serializable;
import org.hipparchus.analysis.differentiation.UnivariateDerivative2;
import org.hipparchus.geometry.euclidean.threed.FieldVector3D;
import org.hipparchus.geometry.euclidean.threed.Vector3D;
import org.hipparchus.linear.RealMatrix;
import org.hipparchus.util.FastMath;
import org.hipparchus.util.MathUtils;
import org.hipparchus.util.SinCos;
import org.orekit.attitudes.AttitudeProvider;
import org.orekit.attitudes.FrameAlignedProvider;
import org.orekit.errors.OrekitException;
import org.orekit.errors.OrekitMessages;
import org.orekit.forces.gravity.potential.UnnormalizedSphericalHarmonicsProvider;
import org.orekit.forces.gravity.potential.UnnormalizedSphericalHarmonicsProvider.UnnormalizedSphericalHarmonics;
import org.orekit.orbits.CartesianOrbit;
import org.orekit.orbits.CircularOrbit;
import org.orekit.orbits.Orbit;
import org.orekit.orbits.OrbitType;
import org.orekit.orbits.PositionAngleType;
import org.orekit.propagation.AbstractMatricesHarvester;
import org.orekit.propagation.PropagationType;
import org.orekit.propagation.SpacecraftState;
import org.orekit.time.AbsoluteDate;
import org.orekit.utils.DoubleArrayDictionary;
import org.orekit.utils.TimeSpanMap;
import org.orekit.utils.TimeStampedPVCoordinates;
/** This class propagates a {@link org.orekit.propagation.SpacecraftState}
* using the analytical Eckstein-Hechler model.
* <p>The Eckstein-Hechler model is suited for near circular orbits
* (e < 0.1, with poor accuracy between 0.005 and 0.1) and inclination
* neither equatorial (direct or retrograde) nor critical (direct or
* retrograde).</p>
* <p>
* Note that before version 7.0, there was a large inconsistency in the generated
* orbits, and it was fixed as of version 7.0 of Orekit, with a visible side effect.
* The problems is that if the circular parameters produced by the Eckstein-Hechler
* model are used to build an orbit considered to be osculating, the velocity deduced
* from this orbit was <em>inconsistent with the position evolution</em>! The reason is
* that the model includes non-Keplerian effects but it does not include a corresponding
* circular/Cartesian conversion. As a consequence, all subsequent computation involving
* velocity were wrong. This includes attitude modes like yaw compensation and Doppler
* effect. As this effect was considered serious enough and as accurate velocities were
* considered important, the propagator now generates {@link CartesianOrbit Cartesian
* orbits} which are built in a special way to ensure consistency throughout propagation.
* A side effect is that if circular parameters are rebuilt by user from these propagated
* Cartesian orbit, the circular parameters will generally <em>not</em> match the initial
* orbit (differences in semi-major axis can exceed 120 m). The position however <em>will</em>
* match to sub-micrometer level, and this position will be identical to the positions
* that were generated by previous versions (in other words, the internals of the models
* have not been changed, only the output parameters have been changed). The correctness
* of the initialization has been assessed and is good, as it allows the subsequent orbit
* to remain close to a numerical reference orbit.
* </p>
* <p>
* If users need a more definitive initialization of an Eckstein-Hechler propagator, they
* should consider using a {@link org.orekit.propagation.conversion.PropagatorConverter
* propagator converter} to initialize their Eckstein-Hechler propagator using a complete
* sample instead of just a single initial orbit.
* </p>
* @see Orbit
* @author Guylaine Prat
*/
public class EcksteinHechlerPropagator extends AbstractAnalyticalPropagator {
/** Default convergence threshold for mean parameters conversion. */
private static final double EPSILON_DEFAULT = 1.0e-11;
/** Default value for maxIterations. */
private static final int MAX_ITERATIONS_DEFAULT = 100;
/** Initial Eckstein-Hechler model. */
private EHModel initialModel;
/** All models. */
private transient TimeSpanMap<EHModel> models;
/** Reference radius of the central body attraction model (m). */
private double referenceRadius;
/** Central attraction coefficient (m³/s²). */
private double mu;
/** Un-normalized zonal coefficients. */
private double[] ck0;
/** Build a propagator from orbit and potential provider.
* <p>Mass and attitude provider are set to unspecified non-null arbitrary values.</p>
*
* <p>Using this constructor, an initial osculating orbit is considered.</p>
*
* @param initialOrbit initial orbit
* @param provider for un-normalized zonal coefficients
* @see #EcksteinHechlerPropagator(Orbit, AttitudeProvider,
* UnnormalizedSphericalHarmonicsProvider)
* @see #EcksteinHechlerPropagator(Orbit, UnnormalizedSphericalHarmonicsProvider,
* PropagationType)
*/
public EcksteinHechlerPropagator(final Orbit initialOrbit,
final UnnormalizedSphericalHarmonicsProvider provider) {
this(initialOrbit, FrameAlignedProvider.of(initialOrbit.getFrame()),
DEFAULT_MASS, provider, provider.onDate(initialOrbit.getDate()));
}
/**
* Private helper constructor.
* <p>Using this constructor, an initial osculating orbit is considered.</p>
* @param initialOrbit initial orbit
* @param attitude attitude provider
* @param mass spacecraft mass
* @param provider for un-normalized zonal coefficients
* @param harmonics {@code provider.onDate(initialOrbit.getDate())}
* @see #EcksteinHechlerPropagator(Orbit, AttitudeProvider, double,
* UnnormalizedSphericalHarmonicsProvider,
* UnnormalizedSphericalHarmonicsProvider.UnnormalizedSphericalHarmonics,
* PropagationType)
*/
public EcksteinHechlerPropagator(final Orbit initialOrbit,
final AttitudeProvider attitude,
final double mass,
final UnnormalizedSphericalHarmonicsProvider provider,
final UnnormalizedSphericalHarmonics harmonics) {
this(initialOrbit, attitude, mass, provider.getAe(), provider.getMu(),
harmonics.getUnnormalizedCnm(2, 0),
harmonics.getUnnormalizedCnm(3, 0),
harmonics.getUnnormalizedCnm(4, 0),
harmonics.getUnnormalizedCnm(5, 0),
harmonics.getUnnormalizedCnm(6, 0));
}
/** Build a propagator from orbit and potential.
* <p>Mass and attitude provider are set to unspecified non-null arbitrary values.</p>
* <p>The C<sub>n,0</sub> coefficients are the denormalized zonal coefficients, they
* are related to both the normalized coefficients
* <span style="text-decoration: overline">C</span><sub>n,0</sub>
* and the J<sub>n</sub> one as follows:</p>
*
* <p> C<sub>n,0</sub> = [(2-δ<sub>0,m</sub>)(2n+1)(n-m)!/(n+m)!]<sup>½</sup>
* <span style="text-decoration: overline">C</span><sub>n,0</sub>
*
* <p> C<sub>n,0</sub> = -J<sub>n</sub>
*
* <p>Using this constructor, an initial osculating orbit is considered.</p>
*
* @param initialOrbit initial orbit
* @param referenceRadius reference radius of the Earth for the potential model (m)
* @param mu central attraction coefficient (m³/s²)
* @param c20 un-normalized zonal coefficient (about -1.08e-3 for Earth)
* @param c30 un-normalized zonal coefficient (about +2.53e-6 for Earth)
* @param c40 un-normalized zonal coefficient (about +1.62e-6 for Earth)
* @param c50 un-normalized zonal coefficient (about +2.28e-7 for Earth)
* @param c60 un-normalized zonal coefficient (about -5.41e-7 for Earth)
* @see org.orekit.utils.Constants
* @see #EcksteinHechlerPropagator(Orbit, AttitudeProvider, double, double, double,
* double, double, double, double, double)
*/
public EcksteinHechlerPropagator(final Orbit initialOrbit,
final double referenceRadius, final double mu,
final double c20, final double c30, final double c40,
final double c50, final double c60) {
this(initialOrbit, FrameAlignedProvider.of(initialOrbit.getFrame()),
DEFAULT_MASS, referenceRadius, mu, c20, c30, c40, c50, c60);
}
/** Build a propagator from orbit, mass and potential provider.
* <p>Attitude law is set to an unspecified non-null arbitrary value.</p>
*
* <p>Using this constructor, an initial osculating orbit is considered.</p>
*
* @param initialOrbit initial orbit
* @param mass spacecraft mass
* @param provider for un-normalized zonal coefficients
* @see #EcksteinHechlerPropagator(Orbit, AttitudeProvider, double,
* UnnormalizedSphericalHarmonicsProvider)
*/
public EcksteinHechlerPropagator(final Orbit initialOrbit, final double mass,
final UnnormalizedSphericalHarmonicsProvider provider) {
this(initialOrbit, FrameAlignedProvider.of(initialOrbit.getFrame()),
mass, provider, provider.onDate(initialOrbit.getDate()));
}
/** Build a propagator from orbit, mass and potential.
* <p>Attitude law is set to an unspecified non-null arbitrary value.</p>
* <p>The C<sub>n,0</sub> coefficients are the denormalized zonal coefficients, they
* are related to both the normalized coefficients
* <span style="text-decoration: overline">C</span><sub>n,0</sub>
* and the J<sub>n</sub> one as follows:</p>
*
* <p> C<sub>n,0</sub> = [(2-δ<sub>0,m</sub>)(2n+1)(n-m)!/(n+m)!]<sup>½</sup>
* <span style="text-decoration: overline">C</span><sub>n,0</sub>
*
* <p> C<sub>n,0</sub> = -J<sub>n</sub>
*
* <p>Using this constructor, an initial osculating orbit is considered.</p>
*
* @param initialOrbit initial orbit
* @param mass spacecraft mass
* @param referenceRadius reference radius of the Earth for the potential model (m)
* @param mu central attraction coefficient (m³/s²)
* @param c20 un-normalized zonal coefficient (about -1.08e-3 for Earth)
* @param c30 un-normalized zonal coefficient (about +2.53e-6 for Earth)
* @param c40 un-normalized zonal coefficient (about +1.62e-6 for Earth)
* @param c50 un-normalized zonal coefficient (about +2.28e-7 for Earth)
* @param c60 un-normalized zonal coefficient (about -5.41e-7 for Earth)
* @see #EcksteinHechlerPropagator(Orbit, AttitudeProvider, double, double, double,
* double, double, double, double, double)
*/
public EcksteinHechlerPropagator(final Orbit initialOrbit, final double mass,
final double referenceRadius, final double mu,
final double c20, final double c30, final double c40,
final double c50, final double c60) {
this(initialOrbit, FrameAlignedProvider.of(initialOrbit.getFrame()),
mass, referenceRadius, mu, c20, c30, c40, c50, c60);
}
/** Build a propagator from orbit, attitude provider and potential provider.
* <p>Mass is set to an unspecified non-null arbitrary value.</p>
* <p>Using this constructor, an initial osculating orbit is considered.</p>
* @param initialOrbit initial orbit
* @param attitudeProv attitude provider
* @param provider for un-normalized zonal coefficients
*/
public EcksteinHechlerPropagator(final Orbit initialOrbit,
final AttitudeProvider attitudeProv,
final UnnormalizedSphericalHarmonicsProvider provider) {
this(initialOrbit, attitudeProv, DEFAULT_MASS, provider, provider.onDate(initialOrbit.getDate()));
}
/** Build a propagator from orbit, attitude provider and potential.
* <p>Mass is set to an unspecified non-null arbitrary value.</p>
* <p>The C<sub>n,0</sub> coefficients are the denormalized zonal coefficients, they
* are related to both the normalized coefficients
* <span style="text-decoration: overline">C</span><sub>n,0</sub>
* and the J<sub>n</sub> one as follows:</p>
*
* <p> C<sub>n,0</sub> = [(2-δ<sub>0,m</sub>)(2n+1)(n-m)!/(n+m)!]<sup>½</sup>
* <span style="text-decoration: overline">C</span><sub>n,0</sub>
*
* <p> C<sub>n,0</sub> = -J<sub>n</sub>
*
* <p>Using this constructor, an initial osculating orbit is considered.</p>
*
* @param initialOrbit initial orbit
* @param attitudeProv attitude provider
* @param referenceRadius reference radius of the Earth for the potential model (m)
* @param mu central attraction coefficient (m³/s²)
* @param c20 un-normalized zonal coefficient (about -1.08e-3 for Earth)
* @param c30 un-normalized zonal coefficient (about +2.53e-6 for Earth)
* @param c40 un-normalized zonal coefficient (about +1.62e-6 for Earth)
* @param c50 un-normalized zonal coefficient (about +2.28e-7 for Earth)
* @param c60 un-normalized zonal coefficient (about -5.41e-7 for Earth)
*/
public EcksteinHechlerPropagator(final Orbit initialOrbit,
final AttitudeProvider attitudeProv,
final double referenceRadius, final double mu,
final double c20, final double c30, final double c40,
final double c50, final double c60) {
this(initialOrbit, attitudeProv, DEFAULT_MASS, referenceRadius, mu, c20, c30, c40, c50, c60);
}
/** Build a propagator from orbit, attitude provider, mass and potential provider.
* <p>Using this constructor, an initial osculating orbit is considered.</p>
* @param initialOrbit initial orbit
* @param attitudeProv attitude provider
* @param mass spacecraft mass
* @param provider for un-normalized zonal coefficients
* @see #EcksteinHechlerPropagator(Orbit, AttitudeProvider, double,
* UnnormalizedSphericalHarmonicsProvider, PropagationType)
*/
public EcksteinHechlerPropagator(final Orbit initialOrbit,
final AttitudeProvider attitudeProv,
final double mass,
final UnnormalizedSphericalHarmonicsProvider provider) {
this(initialOrbit, attitudeProv, mass, provider, provider.onDate(initialOrbit.getDate()));
}
/** Build a propagator from orbit, attitude provider, mass and potential.
* <p>The C<sub>n,0</sub> coefficients are the denormalized zonal coefficients, they
* are related to both the normalized coefficients
* <span style="text-decoration: overline">C</span><sub>n,0</sub>
* and the J<sub>n</sub> one as follows:</p>
*
* <p> C<sub>n,0</sub> = [(2-δ<sub>0,m</sub>)(2n+1)(n-m)!/(n+m)!]<sup>½</sup>
* <span style="text-decoration: overline">C</span><sub>n,0</sub>
*
* <p> C<sub>n,0</sub> = -J<sub>n</sub>
*
* <p>Using this constructor, an initial osculating orbit is considered.</p>
*
* @param initialOrbit initial orbit
* @param attitudeProv attitude provider
* @param mass spacecraft mass
* @param referenceRadius reference radius of the Earth for the potential model (m)
* @param mu central attraction coefficient (m³/s²)
* @param c20 un-normalized zonal coefficient (about -1.08e-3 for Earth)
* @param c30 un-normalized zonal coefficient (about +2.53e-6 for Earth)
* @param c40 un-normalized zonal coefficient (about +1.62e-6 for Earth)
* @param c50 un-normalized zonal coefficient (about +2.28e-7 for Earth)
* @param c60 un-normalized zonal coefficient (about -5.41e-7 for Earth)
* @see #EcksteinHechlerPropagator(Orbit, AttitudeProvider, double, double, double,
* double, double, double, double, double, PropagationType)
*/
public EcksteinHechlerPropagator(final Orbit initialOrbit,
final AttitudeProvider attitudeProv,
final double mass,
final double referenceRadius, final double mu,
final double c20, final double c30, final double c40,
final double c50, final double c60) {
this(initialOrbit, attitudeProv, mass, referenceRadius, mu, c20, c30, c40, c50, c60,
PropagationType.OSCULATING);
}
/** Build a propagator from orbit and potential provider.
* <p>Mass and attitude provider are set to unspecified non-null arbitrary values.</p>
*
* <p>Using this constructor, it is possible to define the initial orbit as
* a mean Eckstein-Hechler orbit or an osculating one.</p>
*
* @param initialOrbit initial orbit
* @param provider for un-normalized zonal coefficients
* @param initialType initial orbit type (mean Eckstein-Hechler orbit or osculating orbit)
* @since 10.2
*/
public EcksteinHechlerPropagator(final Orbit initialOrbit,
final UnnormalizedSphericalHarmonicsProvider provider,
final PropagationType initialType) {
this(initialOrbit, FrameAlignedProvider.of(initialOrbit.getFrame()),
DEFAULT_MASS, provider, provider.onDate(initialOrbit.getDate()), initialType);
}
/** Build a propagator from orbit, attitude provider, mass and potential provider.
* <p>Using this constructor, it is possible to define the initial orbit as
* a mean Eckstein-Hechler orbit or an osculating one.</p>
* @param initialOrbit initial orbit
* @param attitudeProv attitude provider
* @param mass spacecraft mass
* @param provider for un-normalized zonal coefficients
* @param initialType initial orbit type (mean Eckstein-Hechler orbit or osculating orbit)
* @since 10.2
*/
public EcksteinHechlerPropagator(final Orbit initialOrbit,
final AttitudeProvider attitudeProv,
final double mass,
final UnnormalizedSphericalHarmonicsProvider provider,
final PropagationType initialType) {
this(initialOrbit, attitudeProv, mass, provider, provider.onDate(initialOrbit.getDate()), initialType);
}
/**
* Private helper constructor.
* <p>Using this constructor, it is possible to define the initial orbit as
* a mean Eckstein-Hechler orbit or an osculating one.</p>
* @param initialOrbit initial orbit
* @param attitude attitude provider
* @param mass spacecraft mass
* @param provider for un-normalized zonal coefficients
* @param harmonics {@code provider.onDate(initialOrbit.getDate())}
* @param initialType initial orbit type (mean Eckstein-Hechler orbit or osculating orbit)
* @since 10.2
*/
public EcksteinHechlerPropagator(final Orbit initialOrbit,
final AttitudeProvider attitude,
final double mass,
final UnnormalizedSphericalHarmonicsProvider provider,
final UnnormalizedSphericalHarmonics harmonics,
final PropagationType initialType) {
this(initialOrbit, attitude, mass, provider.getAe(), provider.getMu(),
harmonics.getUnnormalizedCnm(2, 0),
harmonics.getUnnormalizedCnm(3, 0),
harmonics.getUnnormalizedCnm(4, 0),
harmonics.getUnnormalizedCnm(5, 0),
harmonics.getUnnormalizedCnm(6, 0),
initialType);
}
/** Build a propagator from orbit, attitude provider, mass and potential.
* <p>The C<sub>n,0</sub> coefficients are the denormalized zonal coefficients, they
* are related to both the normalized coefficients
* <span style="text-decoration: overline">C</span><sub>n,0</sub>
* and the J<sub>n</sub> one as follows:</p>
*
* <p> C<sub>n,0</sub> = [(2-δ<sub>0,m</sub>)(2n+1)(n-m)!/(n+m)!]<sup>½</sup>
* <span style="text-decoration: overline">C</span><sub>n,0</sub>
*
* <p> C<sub>n,0</sub> = -J<sub>n</sub>
*
* <p>Using this constructor, it is possible to define the initial orbit as
* a mean Eckstein-Hechler orbit or an osculating one.</p>
*
* @param initialOrbit initial orbit
* @param attitudeProv attitude provider
* @param mass spacecraft mass
* @param referenceRadius reference radius of the Earth for the potential model (m)
* @param mu central attraction coefficient (m³/s²)
* @param c20 un-normalized zonal coefficient (about -1.08e-3 for Earth)
* @param c30 un-normalized zonal coefficient (about +2.53e-6 for Earth)
* @param c40 un-normalized zonal coefficient (about +1.62e-6 for Earth)
* @param c50 un-normalized zonal coefficient (about +2.28e-7 for Earth)
* @param c60 un-normalized zonal coefficient (about -5.41e-7 for Earth)
* @param initialType initial orbit type (mean Eckstein-Hechler orbit or osculating orbit)
* @since 10.2
*/
public EcksteinHechlerPropagator(final Orbit initialOrbit,
final AttitudeProvider attitudeProv,
final double mass,
final double referenceRadius, final double mu,
final double c20, final double c30, final double c40,
final double c50, final double c60,
final PropagationType initialType) {
this(initialOrbit, attitudeProv, mass, referenceRadius, mu,
c20, c30, c40, c50, c60, initialType, EPSILON_DEFAULT, MAX_ITERATIONS_DEFAULT);
}
/** Build a propagator from orbit, attitude provider, mass and potential.
* <p>The C<sub>n,0</sub> coefficients are the denormalized zonal coefficients, they
* are related to both the normalized coefficients
* <span style="text-decoration: overline">C</span><sub>n,0</sub>
* and the J<sub>n</sub> one as follows:</p>
*
* <p> C<sub>n,0</sub> = [(2-δ<sub>0,m</sub>)(2n+1)(n-m)!/(n+m)!]<sup>½</sup>
* <span style="text-decoration: overline">C</span><sub>n,0</sub>
*
* <p> C<sub>n,0</sub> = -J<sub>n</sub>
*
* <p>Using this constructor, it is possible to define the initial orbit as
* a mean Eckstein-Hechler orbit or an osculating one.</p>
*
* @param initialOrbit initial orbit
* @param attitudeProv attitude provider
* @param mass spacecraft mass
* @param referenceRadius reference radius of the Earth for the potential model (m)
* @param mu central attraction coefficient (m³/s²)
* @param c20 un-normalized zonal coefficient (about -1.08e-3 for Earth)
* @param c30 un-normalized zonal coefficient (about +2.53e-6 for Earth)
* @param c40 un-normalized zonal coefficient (about +1.62e-6 for Earth)
* @param c50 un-normalized zonal coefficient (about +2.28e-7 for Earth)
* @param c60 un-normalized zonal coefficient (about -5.41e-7 for Earth)
* @param epsilon convergence threshold for mean parameters conversion
* @param maxIterations maximum iterations for mean parameters conversion
* @param initialType initial orbit type (mean Eckstein-Hechler orbit or osculating orbit)
* @since 11.2
*/
public EcksteinHechlerPropagator(final Orbit initialOrbit,
final AttitudeProvider attitudeProv,
final double mass,
final double referenceRadius, final double mu,
final double c20, final double c30, final double c40,
final double c50, final double c60,
final PropagationType initialType,
final double epsilon, final int maxIterations) {
super(attitudeProv);
// store model coefficients
this.referenceRadius = referenceRadius;
this.mu = mu;
this.ck0 = new double[] {
0.0, 0.0, c20, c30, c40, c50, c60
};
// compute mean parameters if needed
// transform into circular adapted parameters used by the Eckstein-Hechler model
resetInitialState(new SpacecraftState(initialOrbit,
attitudeProv.getAttitude(initialOrbit,
initialOrbit.getDate(),
initialOrbit.getFrame()),
mass),
initialType, epsilon, maxIterations);
}
/** Conversion from osculating to mean orbit.
* <p>
* Compute mean orbit <b>in a Eckstein-Hechler sense</b>, corresponding to the
* osculating SpacecraftState in input.
* </p>
* <p>
* Since the osculating orbit is obtained with the computation of
* short-periodic variation, the resulting output will depend on
* the gravity field parameterized in input.
* </p>
* <p>
* The computation is done through a fixed-point iteration process.
* </p>
* @param osculating osculating orbit to convert
* @param provider for un-normalized zonal coefficients
* @param harmonics {@code provider.onDate(osculating.getDate())}
* @return mean orbit in a Eckstein-Hechler sense
* @since 11.2
*/
public static CircularOrbit computeMeanOrbit(final Orbit osculating,
final UnnormalizedSphericalHarmonicsProvider provider,
final UnnormalizedSphericalHarmonics harmonics) {
return computeMeanOrbit(osculating, provider, harmonics, EPSILON_DEFAULT, MAX_ITERATIONS_DEFAULT);
}
/** Conversion from osculating to mean orbit.
* <p>
* Compute mean orbit <b>in a Eckstein-Hechler sense</b>, corresponding to the
* osculating SpacecraftState in input.
* </p>
* <p>
* Since the osculating orbit is obtained with the computation of
* short-periodic variation, the resulting output will depend on
* the gravity field parameterized in input.
* </p>
* <p>
* The computation is done through a fixed-point iteration process.
* </p>
* @param osculating osculating orbit to convert
* @param provider for un-normalized zonal coefficients
* @param harmonics {@code provider.onDate(osculating.getDate())}
* @param epsilon convergence threshold for mean parameters conversion
* @param maxIterations maximum iterations for mean parameters conversion
* @return mean orbit in a Eckstein-Hechler sense
* @since 11.2
*/
public static CircularOrbit computeMeanOrbit(final Orbit osculating,
final UnnormalizedSphericalHarmonicsProvider provider,
final UnnormalizedSphericalHarmonics harmonics,
final double epsilon, final int maxIterations) {
return computeMeanOrbit(osculating,
provider.getAe(), provider.getMu(),
harmonics.getUnnormalizedCnm(2, 0),
harmonics.getUnnormalizedCnm(3, 0),
harmonics.getUnnormalizedCnm(4, 0),
harmonics.getUnnormalizedCnm(5, 0),
harmonics.getUnnormalizedCnm(6, 0),
epsilon, maxIterations);
}
/** Conversion from osculating to mean orbit.
* <p>
* Compute mean orbit <b>in a Eckstein-Hechler sense</b>, corresponding to the
* osculating SpacecraftState in input.
* </p>
* <p>
* Since the osculating orbit is obtained with the computation of
* short-periodic variation, the resulting output will depend on
* the gravity field parameterized in input.
* </p>
* <p>
* The computation is done through a fixed-point iteration process.
* </p>
* @param osculating osculating orbit to convert
* @param referenceRadius reference radius of the Earth for the potential model (m)
* @param mu central attraction coefficient (m³/s²)
* @param c20 un-normalized zonal coefficient (about -1.08e-3 for Earth)
* @param c30 un-normalized zonal coefficient (about +2.53e-6 for Earth)
* @param c40 un-normalized zonal coefficient (about +1.62e-6 for Earth)
* @param c50 un-normalized zonal coefficient (about +2.28e-7 for Earth)
* @param c60 un-normalized zonal coefficient (about -5.41e-7 for Earth)
* @param epsilon convergence threshold for mean parameters conversion
* @param maxIterations maximum iterations for mean parameters conversion
* @return mean orbit in a Eckstein-Hechler sense
* @since 11.2
*/
public static CircularOrbit computeMeanOrbit(final Orbit osculating,
final double referenceRadius, final double mu,
final double c20, final double c30, final double c40,
final double c50, final double c60,
final double epsilon, final int maxIterations) {
final EcksteinHechlerPropagator propagator =
new EcksteinHechlerPropagator(osculating,
FrameAlignedProvider.of(osculating.getFrame()),
DEFAULT_MASS,
referenceRadius, mu, c20, c30, c40, c50, c60,
PropagationType.OSCULATING, epsilon, maxIterations);
return propagator.initialModel.mean;
}
/** {@inheritDoc}
* <p>The new initial state to consider
* must be defined with an osculating orbit.</p>
* @see #resetInitialState(SpacecraftState, PropagationType)
*/
public void resetInitialState(final SpacecraftState state) {
resetInitialState(state, PropagationType.OSCULATING);
}
/** Reset the propagator initial state.
* @param state new initial state to consider
* @param stateType mean Eckstein-Hechler orbit or osculating orbit
* @since 10.2
*/
public void resetInitialState(final SpacecraftState state, final PropagationType stateType) {
resetInitialState(state, stateType, EPSILON_DEFAULT, MAX_ITERATIONS_DEFAULT);
}
/** Reset the propagator initial state.
* @param state new initial state to consider
* @param stateType mean Eckstein-Hechler orbit or osculating orbit
* @param epsilon convergence threshold for mean parameters conversion
* @param maxIterations maximum iterations for mean parameters conversion
* @since 11.2
*/
public void resetInitialState(final SpacecraftState state, final PropagationType stateType,
final double epsilon, final int maxIterations) {
super.resetInitialState(state);
final CircularOrbit circular = (CircularOrbit) OrbitType.CIRCULAR.convertType(state.getOrbit());
this.initialModel = (stateType == PropagationType.MEAN) ?
new EHModel(circular, state.getMass(), referenceRadius, mu, ck0) :
computeMeanParameters(circular, state.getMass(), epsilon, maxIterations);
this.models = new TimeSpanMap<EHModel>(initialModel);
}
/** {@inheritDoc} */
protected void resetIntermediateState(final SpacecraftState state, final boolean forward) {
resetIntermediateState(state, forward, EPSILON_DEFAULT, MAX_ITERATIONS_DEFAULT);
}
/** Reset an intermediate state.
* @param state new intermediate state to consider
* @param forward if true, the intermediate state is valid for
* propagations after itself
* @param epsilon convergence threshold for mean parameters conversion
* @param maxIterations maximum iterations for mean parameters conversion
* @since 11.2
*/
protected void resetIntermediateState(final SpacecraftState state, final boolean forward,
final double epsilon, final int maxIterations) {
final EHModel newModel = computeMeanParameters((CircularOrbit) OrbitType.CIRCULAR.convertType(state.getOrbit()),
state.getMass(), epsilon, maxIterations);
if (forward) {
models.addValidAfter(newModel, state.getDate(), false);
} else {
models.addValidBefore(newModel, state.getDate(), false);
}
stateChanged(state);
}
/** Compute mean parameters according to the Eckstein-Hechler analytical model.
* @param osculating osculating orbit
* @param mass constant mass
* @param epsilon convergence threshold for mean parameters conversion
* @param maxIterations maximum iterations for mean parameters conversion
* @return Eckstein-Hechler mean model
*/
private EHModel computeMeanParameters(final CircularOrbit osculating, final double mass,
final double epsilon, final int maxIterations) {
// sanity check
if (osculating.getA() < referenceRadius) {
throw new OrekitException(OrekitMessages.TRAJECTORY_INSIDE_BRILLOUIN_SPHERE,
osculating.getA());
}
// rough initialization of the mean parameters
EHModel current = new EHModel(osculating, mass, referenceRadius, mu, ck0);
// threshold for each parameter
final double thresholdA = epsilon * (1 + FastMath.abs(current.mean.getA()));
final double thresholdE = epsilon * (1 + current.mean.getE());
final double thresholdAngles = epsilon * MathUtils.TWO_PI;
int i = 0;
while (i++ < maxIterations) {
// recompute the osculating parameters from the current mean parameters
final UnivariateDerivative2[] parameters = current.propagateParameters(current.mean.getDate());
// adapted parameters residuals
final double deltaA = osculating.getA() - parameters[0].getValue();
final double deltaEx = osculating.getCircularEx() - parameters[1].getValue();
final double deltaEy = osculating.getCircularEy() - parameters[2].getValue();
final double deltaI = osculating.getI() - parameters[3].getValue();
final double deltaRAAN = MathUtils.normalizeAngle(osculating.getRightAscensionOfAscendingNode() -
parameters[4].getValue(),
0.0);
final double deltaAlphaM = MathUtils.normalizeAngle(osculating.getAlphaM() - parameters[5].getValue(), 0.0);
// update mean parameters
current = new EHModel(new CircularOrbit(current.mean.getA() + deltaA,
current.mean.getCircularEx() + deltaEx,
current.mean.getCircularEy() + deltaEy,
current.mean.getI() + deltaI,
current.mean.getRightAscensionOfAscendingNode() + deltaRAAN,
current.mean.getAlphaM() + deltaAlphaM,
PositionAngleType.MEAN,
current.mean.getFrame(),
current.mean.getDate(), mu),
mass, referenceRadius, mu, ck0);
// check convergence
if (FastMath.abs(deltaA) < thresholdA &&
FastMath.abs(deltaEx) < thresholdE &&
FastMath.abs(deltaEy) < thresholdE &&
FastMath.abs(deltaI) < thresholdAngles &&
FastMath.abs(deltaRAAN) < thresholdAngles &&
FastMath.abs(deltaAlphaM) < thresholdAngles) {
return current;
}
}
throw new OrekitException(OrekitMessages.UNABLE_TO_COMPUTE_ECKSTEIN_HECHLER_MEAN_PARAMETERS, i);
}
/** {@inheritDoc} */
public CartesianOrbit propagateOrbit(final AbsoluteDate date) {
// compute Cartesian parameters, taking derivatives into account
// to make sure velocity and acceleration are consistent
final EHModel current = models.get(date);
return new CartesianOrbit(toCartesian(date, current.propagateParameters(date)),
current.mean.getFrame(), mu);
}
/**
* Get the central attraction coefficient μ.
* @return mu central attraction coefficient (m³/s²)
* @since 11.1
*/
public double getMu() {
return mu;
}
/**
* Get the un-normalized zonal coefficients.
* @return the un-normalized zonal coefficients
* @since 11.1
*/
public double[] getCk0() {
return ck0.clone();
}
/**
* Get the reference radius of the central body attraction model.
* @return the reference radius in meters
* @since 11.1
*/
public double getReferenceRadius() {
return referenceRadius;
}
/** {@inheritDoc} */
@Override
protected AbstractMatricesHarvester createHarvester(final String stmName, final RealMatrix initialStm,
final DoubleArrayDictionary initialJacobianColumns) {
// Create the harvester
final EcksteinHechlerHarvester harvester = new EcksteinHechlerHarvester(this, stmName, initialStm, initialJacobianColumns);
// Update the list of additional state provider
addAdditionalStateProvider(harvester);
// Return the configured harvester
return harvester;
}
/** Local class for Eckstein-Hechler model, with fixed mean parameters. */
private static class EHModel implements Serializable {
/** Serializable UID. */
private static final long serialVersionUID = 20160115L;
/** Mean orbit. */
private final CircularOrbit mean;
/** Constant mass. */
private final double mass;
// CHECKSTYLE: stop JavadocVariable check
// preprocessed values
private final double xnotDot;
private final double rdpom;
private final double rdpomp;
private final double eps1;
private final double eps2;
private final double xim;
private final double ommD;
private final double rdl;
private final double aMD;
private final double kh;
private final double kl;
private final double ax1;
private final double ay1;
private final double as1;
private final double ac2;
private final double axy3;
private final double as3;
private final double ac4;
private final double as5;
private final double ac6;
private final double ex1;
private final double exx2;
private final double exy2;
private final double ex3;
private final double ex4;
private final double ey1;
private final double eyx2;
private final double eyy2;
private final double ey3;
private final double ey4;
private final double rx1;
private final double ry1;
private final double r2;
private final double r3;
private final double rl;
private final double iy1;
private final double ix1;
private final double i2;
private final double i3;
private final double ih;
private final double lx1;
private final double ly1;
private final double l2;
private final double l3;
private final double ll;
// CHECKSTYLE: resume JavadocVariable check
/** Create a model for specified mean orbit.
* @param mean mean orbit
* @param mass constant mass
* @param referenceRadius reference radius of the central body attraction model (m)
* @param mu central attraction coefficient (m³/s²)
* @param ck0 un-normalized zonal coefficients
*/
EHModel(final CircularOrbit mean, final double mass,
final double referenceRadius, final double mu, final double[] ck0) {
this.mean = mean;
this.mass = mass;
// preliminary processing
double q = referenceRadius / mean.getA();
double ql = q * q;
final double g2 = ck0[2] * ql;
ql *= q;
final double g3 = ck0[3] * ql;
ql *= q;
final double g4 = ck0[4] * ql;
ql *= q;
final double g5 = ck0[5] * ql;
ql *= q;
final double g6 = ck0[6] * ql;
final SinCos sc = FastMath.sinCos(mean.getI());
final double cosI1 = sc.cos();
final double sinI1 = sc.sin();
final double sinI2 = sinI1 * sinI1;
final double sinI4 = sinI2 * sinI2;
final double sinI6 = sinI2 * sinI4;
if (sinI2 < 1.0e-10) {
throw new OrekitException(OrekitMessages.ALMOST_EQUATORIAL_ORBIT,
FastMath.toDegrees(mean.getI()));
}
if (FastMath.abs(sinI2 - 4.0 / 5.0) < 1.0e-3) {
throw new OrekitException(OrekitMessages.ALMOST_CRITICALLY_INCLINED_ORBIT,
FastMath.toDegrees(mean.getI()));
}
if (mean.getE() > 0.1) {
// if 0.005 < e < 0.1 no error is triggered, but accuracy is poor
throw new OrekitException(OrekitMessages.TOO_LARGE_ECCENTRICITY_FOR_PROPAGATION_MODEL,
mean.getE());
}
xnotDot = FastMath.sqrt(mu / mean.getA()) / mean.getA();
rdpom = -0.75 * g2 * (4.0 - 5.0 * sinI2);
rdpomp = 7.5 * g4 * (1.0 - 31.0 / 8.0 * sinI2 + 49.0 / 16.0 * sinI4) -
13.125 * g6 * (1.0 - 8.0 * sinI2 + 129.0 / 8.0 * sinI4 - 297.0 / 32.0 * sinI6);
q = 3.0 / (32.0 * rdpom);
eps1 = q * g4 * sinI2 * (30.0 - 35.0 * sinI2) -
175.0 * q * g6 * sinI2 * (1.0 - 3.0 * sinI2 + 2.0625 * sinI4);
q = 3.0 * sinI1 / (8.0 * rdpom);
eps2 = q * g3 * (4.0 - 5.0 * sinI2) - q * g5 * (10.0 - 35.0 * sinI2 + 26.25 * sinI4);
xim = mean.getI();
ommD = cosI1 * (1.50 * g2 - 2.25 * g2 * g2 * (2.5 - 19.0 / 6.0 * sinI2) +
0.9375 * g4 * (7.0 * sinI2 - 4.0) +
3.28125 * g6 * (2.0 - 9.0 * sinI2 + 8.25 * sinI4));
rdl = 1.0 - 1.50 * g2 * (3.0 - 4.0 * sinI2);
aMD = rdl +
2.25 * g2 * g2 * (9.0 - 263.0 / 12.0 * sinI2 + 341.0 / 24.0 * sinI4) +
15.0 / 16.0 * g4 * (8.0 - 31.0 * sinI2 + 24.5 * sinI4) +
105.0 / 32.0 * g6 * (-10.0 / 3.0 + 25.0 * sinI2 - 48.75 * sinI4 + 27.5 * sinI6);
final double qq = -1.5 * g2 / rdl;
final double qA = 0.75 * g2 * g2 * sinI2;
final double qB = 0.25 * g4 * sinI2;
final double qC = 105.0 / 16.0 * g6 * sinI2;
final double qD = -0.75 * g3 * sinI1;
final double qE = 3.75 * g5 * sinI1;
kh = 0.375 / rdpom;
kl = kh / sinI1;
ax1 = qq * (2.0 - 3.5 * sinI2);
ay1 = qq * (2.0 - 2.5 * sinI2);
as1 = qD * (4.0 - 5.0 * sinI2) +
qE * (2.625 * sinI4 - 3.5 * sinI2 + 1.0);
ac2 = qq * sinI2 +
qA * 7.0 * (2.0 - 3.0 * sinI2) +
qB * (15.0 - 17.5 * sinI2) +
qC * (3.0 * sinI2 - 1.0 - 33.0 / 16.0 * sinI4);
axy3 = qq * 3.5 * sinI2;
as3 = qD * 5.0 / 3.0 * sinI2 +
qE * 7.0 / 6.0 * sinI2 * (1.0 - 1.125 * sinI2);
ac4 = qA * sinI2 +
qB * 4.375 * sinI2 +
qC * 0.75 * (1.1 * sinI4 - sinI2);
as5 = qE * 21.0 / 80.0 * sinI4;
ac6 = qC * -11.0 / 80.0 * sinI4;
ex1 = qq * (1.0 - 1.25 * sinI2);
exx2 = qq * 0.5 * (3.0 - 5.0 * sinI2);
exy2 = qq * (2.0 - 1.5 * sinI2);
ex3 = qq * 7.0 / 12.0 * sinI2;
ex4 = qq * 17.0 / 8.0 * sinI2;
ey1 = qq * (1.0 - 1.75 * sinI2);
eyx2 = qq * (1.0 - 3.0 * sinI2);
eyy2 = qq * (2.0 * sinI2 - 1.5);
ey3 = qq * 7.0 / 12.0 * sinI2;
ey4 = qq * 17.0 / 8.0 * sinI2;
q = -qq * cosI1;
rx1 = 3.5 * q;
ry1 = -2.5 * q;
r2 = -0.5 * q;
r3 = 7.0 / 6.0 * q;
rl = g3 * cosI1 * (4.0 - 15.0 * sinI2) -
2.5 * g5 * cosI1 * (4.0 - 42.0 * sinI2 + 52.5 * sinI4);
q = 0.5 * qq * sinI1 * cosI1;
iy1 = q;
ix1 = -q;
i2 = q;
i3 = q * 7.0 / 3.0;
ih = -g3 * cosI1 * (4.0 - 5.0 * sinI2) +
2.5 * g5 * cosI1 * (4.0 - 14.0 * sinI2 + 10.5 * sinI4);
lx1 = qq * (7.0 - 77.0 / 8.0 * sinI2);
ly1 = qq * (55.0 / 8.0 * sinI2 - 7.50);
l2 = qq * (1.25 * sinI2 - 0.5);
l3 = qq * (77.0 / 24.0 * sinI2 - 7.0 / 6.0);
ll = g3 * (53.0 * sinI2 - 4.0 - 57.5 * sinI4) +
2.5 * g5 * (4.0 - 96.0 * sinI2 + 269.5 * sinI4 - 183.75 * sinI6);
}
/** Extrapolate an orbit up to a specific target date.
* @param date target date for the orbit
* @return propagated parameters
*/
public UnivariateDerivative2[] propagateParameters(final AbsoluteDate date) {
// Keplerian evolution
final UnivariateDerivative2 dt = new UnivariateDerivative2(date.durationFrom(mean.getDate()), 1.0, 0.0);
final UnivariateDerivative2 xnot = dt.multiply(xnotDot);
// secular effects
// eccentricity
final UnivariateDerivative2 x = xnot.multiply(rdpom + rdpomp);
final UnivariateDerivative2 cx = x.cos();
final UnivariateDerivative2 sx = x.sin();
final UnivariateDerivative2 exm = cx.multiply(mean.getCircularEx()).
add(sx.multiply(eps2 - (1.0 - eps1) * mean.getCircularEy()));
final UnivariateDerivative2 eym = sx.multiply((1.0 + eps1) * mean.getCircularEx()).
add(cx.multiply(mean.getCircularEy() - eps2)).
add(eps2);
// no secular effect on inclination
// right ascension of ascending node
final UnivariateDerivative2 omm = new UnivariateDerivative2(MathUtils.normalizeAngle(mean.getRightAscensionOfAscendingNode() + ommD * xnot.getValue(),
FastMath.PI),
ommD * xnotDot,
0.0);
// latitude argument
final UnivariateDerivative2 xlm = new UnivariateDerivative2(MathUtils.normalizeAngle(mean.getAlphaM() + aMD * xnot.getValue(),
FastMath.PI),
aMD * xnotDot,
0.0);
// periodical terms
final UnivariateDerivative2 cl1 = xlm.cos();
final UnivariateDerivative2 sl1 = xlm.sin();
final UnivariateDerivative2 cl2 = cl1.multiply(cl1).subtract(sl1.multiply(sl1));
final UnivariateDerivative2 sl2 = cl1.multiply(sl1).add(sl1.multiply(cl1));
final UnivariateDerivative2 cl3 = cl2.multiply(cl1).subtract(sl2.multiply(sl1));
final UnivariateDerivative2 sl3 = cl2.multiply(sl1).add(sl2.multiply(cl1));
final UnivariateDerivative2 cl4 = cl3.multiply(cl1).subtract(sl3.multiply(sl1));
final UnivariateDerivative2 sl4 = cl3.multiply(sl1).add(sl3.multiply(cl1));
final UnivariateDerivative2 cl5 = cl4.multiply(cl1).subtract(sl4.multiply(sl1));
final UnivariateDerivative2 sl5 = cl4.multiply(sl1).add(sl4.multiply(cl1));
final UnivariateDerivative2 cl6 = cl5.multiply(cl1).subtract(sl5.multiply(sl1));
final UnivariateDerivative2 qh = eym.subtract(eps2).multiply(kh);
final UnivariateDerivative2 ql = exm.multiply(kl);
final UnivariateDerivative2 exmCl1 = exm.multiply(cl1);
final UnivariateDerivative2 exmSl1 = exm.multiply(sl1);
final UnivariateDerivative2 eymCl1 = eym.multiply(cl1);
final UnivariateDerivative2 eymSl1 = eym.multiply(sl1);
final UnivariateDerivative2 exmCl2 = exm.multiply(cl2);
final UnivariateDerivative2 exmSl2 = exm.multiply(sl2);
final UnivariateDerivative2 eymCl2 = eym.multiply(cl2);
final UnivariateDerivative2 eymSl2 = eym.multiply(sl2);
final UnivariateDerivative2 exmCl3 = exm.multiply(cl3);
final UnivariateDerivative2 exmSl3 = exm.multiply(sl3);
final UnivariateDerivative2 eymCl3 = eym.multiply(cl3);
final UnivariateDerivative2 eymSl3 = eym.multiply(sl3);
final UnivariateDerivative2 exmCl4 = exm.multiply(cl4);
final UnivariateDerivative2 exmSl4 = exm.multiply(sl4);
final UnivariateDerivative2 eymCl4 = eym.multiply(cl4);
final UnivariateDerivative2 eymSl4 = eym.multiply(sl4);
// semi major axis
final UnivariateDerivative2 rda = exmCl1.multiply(ax1).
add(eymSl1.multiply(ay1)).
add(sl1.multiply(as1)).
add(cl2.multiply(ac2)).
add(exmCl3.add(eymSl3).multiply(axy3)).
add(sl3.multiply(as3)).
add(cl4.multiply(ac4)).
add(sl5.multiply(as5)).
add(cl6.multiply(ac6));
// eccentricity
final UnivariateDerivative2 rdex = cl1.multiply(ex1).
add(exmCl2.multiply(exx2)).
add(eymSl2.multiply(exy2)).
add(cl3.multiply(ex3)).
add(exmCl4.add(eymSl4).multiply(ex4));
final UnivariateDerivative2 rdey = sl1.multiply(ey1).
add(exmSl2.multiply(eyx2)).
add(eymCl2.multiply(eyy2)).
add(sl3.multiply(ey3)).
add(exmSl4.subtract(eymCl4).multiply(ey4));
// ascending node
final UnivariateDerivative2 rdom = exmSl1.multiply(rx1).
add(eymCl1.multiply(ry1)).
add(sl2.multiply(r2)).
add(eymCl3.subtract(exmSl3).multiply(r3)).
add(ql.multiply(rl));
// inclination
final UnivariateDerivative2 rdxi = eymSl1.multiply(iy1).
add(exmCl1.multiply(ix1)).
add(cl2.multiply(i2)).
add(exmCl3.add(eymSl3).multiply(i3)).
add(qh.multiply(ih));
// latitude argument
final UnivariateDerivative2 rdxl = exmSl1.multiply(lx1).
add(eymCl1.multiply(ly1)).
add(sl2.multiply(l2)).
add(exmSl3.subtract(eymCl3).multiply(l3)).
add(ql.multiply(ll));
// osculating parameters
return new UnivariateDerivative2[] {
rda.add(1.0).multiply(mean.getA()),
rdex.add(exm),
rdey.add(eym),
rdxi.add(xim),
rdom.add(omm),
rdxl.add(xlm)
};
}
}
/** Convert circular parameters <em>with derivatives</em> to Cartesian coordinates.
* @param date date of the orbital parameters
* @param parameters circular parameters (a, ex, ey, i, raan, alphaM)
* @return Cartesian coordinates consistent with values and derivatives
*/
private TimeStampedPVCoordinates toCartesian(final AbsoluteDate date, final UnivariateDerivative2[] parameters) {
// evaluate coordinates in the orbit canonical reference frame
final UnivariateDerivative2 cosOmega = parameters[4].cos();
final UnivariateDerivative2 sinOmega = parameters[4].sin();
final UnivariateDerivative2 cosI = parameters[3].cos();
final UnivariateDerivative2 sinI = parameters[3].sin();
final UnivariateDerivative2 alphaE = meanToEccentric(parameters[5], parameters[1], parameters[2]);
final UnivariateDerivative2 cosAE = alphaE.cos();
final UnivariateDerivative2 sinAE = alphaE.sin();
final UnivariateDerivative2 ex2 = parameters[1].multiply(parameters[1]);
final UnivariateDerivative2 ey2 = parameters[2].multiply(parameters[2]);
final UnivariateDerivative2 exy = parameters[1].multiply(parameters[2]);
final UnivariateDerivative2 q = ex2.add(ey2).subtract(1).negate().sqrt();
final UnivariateDerivative2 beta = q.add(1).reciprocal();
final UnivariateDerivative2 bx2 = beta.multiply(ex2);
final UnivariateDerivative2 by2 = beta.multiply(ey2);
final UnivariateDerivative2 bxy = beta.multiply(exy);
final UnivariateDerivative2 u = bxy.multiply(sinAE).subtract(parameters[1].add(by2.subtract(1).multiply(cosAE)));
final UnivariateDerivative2 v = bxy.multiply(cosAE).subtract(parameters[2].add(bx2.subtract(1).multiply(sinAE)));
final UnivariateDerivative2 x = parameters[0].multiply(u);
final UnivariateDerivative2 y = parameters[0].multiply(v);
// canonical orbit reference frame
final FieldVector3D<UnivariateDerivative2> p =
new FieldVector3D<>(x.multiply(cosOmega).subtract(y.multiply(cosI.multiply(sinOmega))),
x.multiply(sinOmega).add(y.multiply(cosI.multiply(cosOmega))),
y.multiply(sinI));
// dispatch derivatives
final Vector3D p0 = new Vector3D(p.getX().getValue(),
p.getY().getValue(),
p.getZ().getValue());
final Vector3D p1 = new Vector3D(p.getX().getFirstDerivative(),
p.getY().getFirstDerivative(),
p.getZ().getFirstDerivative());
final Vector3D p2 = new Vector3D(p.getX().getSecondDerivative(),
p.getY().getSecondDerivative(),
p.getZ().getSecondDerivative());
return new TimeStampedPVCoordinates(date, p0, p1, p2);
}
/** Computes the eccentric latitude argument from the mean latitude argument.
* @param alphaM = M + Ω mean latitude argument (rad)
* @param ex e cos(Ω), first component of circular eccentricity vector
* @param ey e sin(Ω), second component of circular eccentricity vector
* @return the eccentric latitude argument.
*/
private UnivariateDerivative2 meanToEccentric(final UnivariateDerivative2 alphaM,
final UnivariateDerivative2 ex,
final UnivariateDerivative2 ey) {
// Generalization of Kepler equation to circular parameters
// with alphaE = PA + E and
// alphaM = PA + M = alphaE - ex.sin(alphaE) + ey.cos(alphaE)
UnivariateDerivative2 alphaE = alphaM;
UnivariateDerivative2 shift = alphaM.getField().getZero();
UnivariateDerivative2 alphaEMalphaM = alphaM.getField().getZero();
UnivariateDerivative2 cosAlphaE = alphaE.cos();
UnivariateDerivative2 sinAlphaE = alphaE.sin();
int iter = 0;
do {
final UnivariateDerivative2 f2 = ex.multiply(sinAlphaE).subtract(ey.multiply(cosAlphaE));
final UnivariateDerivative2 f1 = alphaM.getField().getOne().subtract(ex.multiply(cosAlphaE)).subtract(ey.multiply(sinAlphaE));
final UnivariateDerivative2 f0 = alphaEMalphaM.subtract(f2);
final UnivariateDerivative2 f12 = f1.multiply(2);
shift = f0.multiply(f12).divide(f1.multiply(f12).subtract(f0.multiply(f2)));
alphaEMalphaM = alphaEMalphaM.subtract(shift);
alphaE = alphaM.add(alphaEMalphaM);
cosAlphaE = alphaE.cos();
sinAlphaE = alphaE.sin();
} while (++iter < 50 && FastMath.abs(shift.getValue()) > 1.0e-12);
return alphaE;
}
/** {@inheritDoc} */
protected double getMass(final AbsoluteDate date) {
return models.get(date).mass;
}
}