/* Copyright 2002-2017 CS Systèmes d'Information * 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.propagation.analytical.tle; import org.hipparchus.util.FastMath; import org.hipparchus.util.MathUtils; import org.orekit.attitudes.AttitudeProvider; import org.orekit.errors.OrekitException; import org.orekit.time.AbsoluteDate; import org.orekit.time.TimeScalesFactory; import org.orekit.utils.Constants; /** This class contains methods to compute propagated coordinates with the SDP4 model. * <p> * The user should not bother in this class since it is handled internally by the * {@link TLEPropagator}. * </p> * <p>This implementation is largely inspired from the paper and source code <a * href="http://www.celestrak.com/publications/AIAA/2006-6753/">Revisiting Spacetrack * Report #3</a> and is fully compliant with its results and tests cases.</p> * @author Felix R. Hoots, Ronald L. Roehrich, December 1980 (original fortran) * @author David A. Vallado, Paul Crawford, Richard Hujsak, T.S. Kelso (C++ translation and improvements) * @author Fabien Maussion (java translation) */ abstract class SDP4 extends TLEPropagator { // CHECKSTYLE: stop VisibilityModifierCheck /** New perigee argument. */ protected double omgadf; /** New mean motion. */ protected double xn; /** Parameter for xl computation. */ protected double xll; /** New eccentricity. */ protected double em; /** New inclination. */ protected double xinc; // CHECKSTYLE: resume VisibilityModifierCheck /** Constructor for a unique initial TLE. * @param initialTLE the TLE to propagate. * @param attitudeProvider provider for attitude computation * @param mass spacecraft mass (kg) * @exception OrekitException if some specific error occurs */ protected SDP4(final TLE initialTLE, final AttitudeProvider attitudeProvider, final double mass) throws OrekitException { super(initialTLE, attitudeProvider, mass); } /** Initialization proper to each propagator (SGP or SDP). * @exception OrekitException when UTC time steps can't be read */ protected void sxpInitialize() throws OrekitException { luniSolarTermsComputation(); } // End of initialization /** Propagation proper to each propagator (SGP or SDP). * @param tSince the offset from initial epoch (minutes) */ protected void sxpPropagate(final double tSince) { // Update for secular gravity and atmospheric drag omgadf = tle.getPerigeeArgument() + omgdot * tSince; final double xnoddf = tle.getRaan() + xnodot * tSince; final double tSinceSq = tSince * tSince; xnode = xnoddf + xnodcf * tSinceSq; xn = xn0dp; // Update for deep-space secular effects xll = tle.getMeanAnomaly() + xmdot * tSince; deepSecularEffects(tSince); final double tempa = 1 - c1 * tSince; a = FastMath.pow(TLEConstants.XKE / xn, TLEConstants.TWO_THIRD) * tempa * tempa; em -= tle.getBStar() * c4 * tSince; // Update for deep-space periodic effects xll += xn0dp * t2cof * tSinceSq; deepPeriodicEffects(tSince); xl = xll + omgadf + xnode; // Dundee change: Reset cosio, sinio for new xinc: cosi0 = FastMath.cos(xinc); sini0 = FastMath.sin(xinc); e = em; i = xinc; omega = omgadf; // end of calculus, go for PV computation } /** Computes SPACETRACK#3 compliant earth rotation angle. * @param date the current date * @return the ERA (rad) * @exception OrekitException when UTC time steps can't be read */ protected static double thetaG(final AbsoluteDate date) throws OrekitException { // Reference: The 1992 Astronomical Almanac, page B6. final double omega_E = 1.00273790934; final double jd = (date.durationFrom(AbsoluteDate.JULIAN_EPOCH) + date.timeScalesOffset(TimeScalesFactory.getUTC(), TimeScalesFactory.getTT()) ) / Constants.JULIAN_DAY; // Earth rotations per sidereal day (non-constant) final double UT = (jd + 0.5) % 1; final double seconds_per_day = Constants.JULIAN_DAY; final double jd_2000 = 2451545.0; /* 1.5 Jan 2000 = JD 2451545. */ final double t_cen = (jd - UT - jd_2000) / 36525.; double GMST = 24110.54841 + t_cen * (8640184.812866 + t_cen * (0.093104 - t_cen * 6.2E-6)); GMST = (GMST + seconds_per_day * omega_E * UT) % seconds_per_day; if (GMST < 0.) { GMST += seconds_per_day; } return MathUtils.TWO_PI * GMST / seconds_per_day; } /** Computes luni - solar terms from initial coordinates and epoch. * @exception OrekitException when UTC time steps can't be read */ protected abstract void luniSolarTermsComputation() throws OrekitException; /** Computes secular terms from current coordinates and epoch. * @param t offset from initial epoch (min) */ protected abstract void deepSecularEffects(double t); /** Computes periodic terms from current coordinates and epoch. * @param t offset from initial epoch (min) */ protected abstract void deepPeriodicEffects(double t); }