1 /* Copyright 2002-2026 CS GROUP
2 * Licensed to CS GROUP (CS) under one or more
3 * contributor license agreements. See the NOTICE file distributed with
4 * this work for additional information regarding copyright ownership.
5 * CS licenses this file to You under the Apache License, Version 2.0
6 * (the "License"); you may not use this file except in compliance with
7 * the License. You may obtain a copy of the License at
8 *
9 * http://www.apache.org/licenses/LICENSE-2.0
10 *
11 * Unless required by applicable law or agreed to in writing, software
12 * distributed under the License is distributed on an "AS IS" BASIS,
13 * WITHOUT WARRANTIES OR CONDITIONS OF ANY KIND, either express or implied.
14 * See the License for the specific language governing permissions and
15 * limitations under the License.
16 */
17 package org.orekit.propagation.events;
18
19 import org.hipparchus.ode.events.Action;
20 import org.hipparchus.util.FastMath;
21 import org.hipparchus.util.MathUtils;
22 import org.orekit.frames.Frame;
23 import org.orekit.orbits.KeplerianOrbit;
24 import org.orekit.orbits.Orbit;
25 import org.orekit.orbits.OrbitType;
26 import org.orekit.orbits.PositionAngleType;
27 import org.orekit.propagation.SpacecraftState;
28 import org.orekit.propagation.events.functions.NodeEventFunction;
29 import org.orekit.propagation.events.handlers.EventHandler;
30 import org.orekit.propagation.events.handlers.StopOnIncreasing;
31 import org.orekit.propagation.events.intervals.AdaptableInterval;
32
33 /** Finder for node crossing events.
34 * <p>This class finds equator crossing events (i.e. ascending
35 * or descending node crossing).</p>
36 * <p>The default implementation behavior is to {@link Action#CONTINUE continue}
37 * propagation at descending node crossing and to {@link Action#STOP stop} propagation
38 * at ascending node crossing. This can be changed by calling
39 * {@link #withHandler(EventHandler)} after construction.</p>
40 * <p>Beware that node detection will fail for almost equatorial orbits. If
41 * for example a node detector is used to trigger an {@link
42 * org.orekit.forces.maneuvers.ImpulseManeuver ImpulseManeuver} and the maneuver
43 * turn the orbit plane to equator, then the detector may completely fail just
44 * after the maneuver has been performed! This is a real case that has been
45 * encountered during validation ...</p>
46 * @see org.orekit.propagation.Propagator#addEventDetector(EventDetector)
47 * @author Luc Maisonobe
48 */
49 public class NodeDetector extends AbstractDetector<NodeDetector> {
50
51 /** Default max check interval. */
52 private static final double DEFAULT_MAX_CHECK = 1800.0;
53
54 /** Default convergence threshold. */
55 private static final double DEFAULT_THRESHOLD = 1.0e-3;
56
57 /** Frame in which the equator is defined. */
58 private final Frame frame;
59
60 /** Build a new instance.
61 * <p>The default {@link #getMaxCheckInterval() max check interval}
62 * is set to 1800s, it can be changed using {@link #withMaxCheck(double)}
63 * in the fluent API. The default {@link #getThreshold() convergence threshold}
64 * is set to 1.0e-3s, it can be changed using {@link #withThreshold(double)}
65 * in the fluent API.</p>
66 * @param frame frame in which the equator is defined (typical
67 * values are {@link org.orekit.frames.FramesFactory#getEME2000() EME<sub>2000</sub>} or
68 * {@link org.orekit.frames.FramesFactory#getITRF(org.orekit.utils.IERSConventions, boolean) ITRF})
69 * @since 10.3
70 */
71 public NodeDetector(final Frame frame) {
72 this(new EventDetectionSettings(DEFAULT_MAX_CHECK, DEFAULT_THRESHOLD, EventDetectionSettings.DEFAULT_MAX_ITER),
73 new StopOnIncreasing(), frame);
74 }
75
76 /** Build a new instance.
77 * <p>The orbit is used only to set an upper bound for the max check interval
78 * to a value related to nodes separation (as computed by a Keplerian model)
79 * and to set the convergence threshold according to orbit size.</p>
80 * @param orbit initial orbit
81 * @param frame frame in which the equator is defined (typical
82 * values are {@link org.orekit.frames.FramesFactory#getEME2000() EME<sub>2000</sub>} or
83 * {@link org.orekit.frames.FramesFactory#getITRF(org.orekit.utils.IERSConventions, boolean) ITRF})
84 */
85 public NodeDetector(final Orbit orbit, final Frame frame) {
86 this(1.0e-13 * orbit.getKeplerianPeriod(), orbit, frame);
87 }
88
89 /** Build a new instance.
90 * <p>The orbit is used only to set an upper bound for the max check interval
91 * to a value related to nodes separation (as computed by a Keplerian model).</p>
92 * @param threshold convergence threshold (s)
93 * @param orbit initial orbit
94 * @param frame frame in which the equator is defined (typical
95 * values are {@link org.orekit.frames.FramesFactory#getEME2000() EME<sub>2000</sub>} or
96 * {@link org.orekit.frames.FramesFactory#getITRF(org.orekit.utils.IERSConventions, boolean) ITRF})
97 */
98 public NodeDetector(final double threshold, final Orbit orbit, final Frame frame) {
99 this(new EventDetectionSettings(AdaptableInterval.of(2 * estimateNodesTimeSeparation(orbit) / 3), threshold,
100 DEFAULT_MAX_ITER), new StopOnIncreasing(),
101 frame);
102 }
103
104 /** Constructor with detection settings and handler.
105 * @param detectionSettings detection settings
106 * @param handler event handler to call at event occurrences
107 * @param frame frame in which the equator is defined (typical values are {@link org.orekit.frames.FramesFactory#getEME2000() EME<sub>2000</sub>} or
108 * {@link org.orekit.frames.FramesFactory#getITRF(org.orekit.utils.IERSConventions, boolean) ITRF})
109 */
110 public NodeDetector(final EventDetectionSettings detectionSettings, final EventHandler handler, final Frame frame) {
111 this(new NodeEventFunction(frame), detectionSettings, handler);
112 }
113
114 /** Protected constructor with full parameters.
115 * <p>
116 * This constructor is not public as users are expected to use the builder
117 * API with the various {@code withXxx()} methods to set up the instance
118 * in a readable manner without using a huge amount of parameters.
119 * </p>
120 * @param nodeEventFunction event function
121 * @param detectionSettings detection settings
122 * @param handler event handler to call at event occurrences
123 * values are {@link org.orekit.frames.FramesFactory#getEME2000() EME<sub>2000</sub>} or
124 * {@link org.orekit.frames.FramesFactory#getITRF(org.orekit.utils.IERSConventions, boolean) ITRF})
125 * @since 14.0
126 */
127 protected NodeDetector(final NodeEventFunction nodeEventFunction,
128 final EventDetectionSettings detectionSettings, final EventHandler handler) {
129 super(nodeEventFunction, detectionSettings, handler);
130 this.frame = nodeEventFunction.getFrame();
131 }
132
133 /** {@inheritDoc} */
134 @Override
135 protected NodeDetector create(final EventDetectionSettings detectionSettings, final EventHandler newHandler) {
136 return new NodeDetector((NodeEventFunction) getEventFunction(), detectionSettings, newHandler);
137 }
138
139 /** Find time separation between nodes.
140 * <p>
141 * The estimation of time separation is based on Keplerian motion, it is only
142 * used as a rough guess for a safe setting of default max check interval for
143 * event detection.
144 * </p>
145 * @param orbit initial orbit
146 * @return minimum time separation between nodes
147 */
148 private static double estimateNodesTimeSeparation(final Orbit orbit) {
149
150 final KeplerianOrbit keplerian = (KeplerianOrbit) OrbitType.KEPLERIAN.convertType(orbit);
151
152 // mean anomaly of ascending node
153 final double ascendingM = new KeplerianOrbit(keplerian.getA(), keplerian.getE(),
154 keplerian.getI(),
155 keplerian.getPerigeeArgument(),
156 keplerian.getRightAscensionOfAscendingNode(),
157 -keplerian.getPerigeeArgument(), PositionAngleType.TRUE,
158 keplerian.getFrame(), keplerian.getDate(),
159 keplerian.getMu()).getMeanAnomaly();
160
161 // mean anomaly of descending node
162 final double descendingM = new KeplerianOrbit(keplerian.getA(), keplerian.getE(),
163 keplerian.getI(),
164 keplerian.getPerigeeArgument(),
165 keplerian.getRightAscensionOfAscendingNode(),
166 FastMath.PI - keplerian.getPerigeeArgument(), PositionAngleType.TRUE,
167 keplerian.getFrame(), keplerian.getDate(),
168 keplerian.getMu()).getMeanAnomaly();
169
170 // differences between mean anomalies
171 final double delta1 = MathUtils.normalizeAngle(ascendingM, descendingM + FastMath.PI) - descendingM;
172 final double delta2 = 2 * FastMath.PI - delta1;
173
174 // minimum time separation between the two nodes
175 return FastMath.min(delta1, delta2) / keplerian.getKeplerianMeanMotion();
176
177 }
178
179 /** Get the frame in which the equator is defined.
180 * @return the frame in which the equator is defined
181 */
182 public Frame getFrame() {
183 return frame;
184 }
185
186 /** Compute the value of the switching function.
187 * This function computes the Z position in the defined frame.
188 * @param s the current state information: date, kinematics, attitude
189 * @return value of the switching function
190 */
191 public double g(final SpacecraftState s) {
192 return getEventFunction().value(s);
193 }
194
195 }