FieldDSSTZonalContext.java
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package org.orekit.propagation.semianalytical.dsst.forces;
import org.hipparchus.CalculusFieldElement;
import org.hipparchus.util.FastMath;
import org.orekit.forces.gravity.potential.UnnormalizedSphericalHarmonicsProvider;
import org.orekit.propagation.semianalytical.dsst.utilities.FieldAuxiliaryElements;
import org.orekit.time.AbsoluteDate;
/**
* This class is a container for the common "field" parameters used in {@link DSSTZonal}.
* <p>
* It performs parameters initialization at each integration step for the Zonal contribution
* to the central body gravitational perturbation.
* </p>
* @author Bryan Cazabonne
* @since 10.0
* @param <T> type of the field elements
*/
public class FieldDSSTZonalContext<T extends CalculusFieldElement<T>> extends FieldForceModelContext<T> {
// Common factors for potential computation
/** A = sqrt(μ * a). */
private final T A;
/** Χ = 1 / sqrt(1 - e²) = 1 / B. */
private T X;
/** Χ². */
private T XX;
/** Χ³. */
private T XXX;
/** 1 / (A * B) . */
private T ooAB;
/** B / A . */
private T BoA;
/** B / A(1 + B) . */
private T BoABpo;
/** -C / (2 * A * B) . */
private T mCo2AB;
/** -2 * a / A . */
private T m2aoA;
/** μ / a . */
private T muoa;
/** R / a . */
private T roa;
/** Keplerian mean motion. */
private final T n;
// Short period terms
/** h * k. */
private T hk;
/** k² - h². */
private T k2mh2;
/** (k² - h²) / 2. */
private T k2mh2o2;
/** 1 / (n² * a²). */
private T oon2a2;
/** 1 / (n² * a) . */
private T oon2a;
/** χ³ / (n² * a). */
private T x3on2a;
/** χ / (n² * a²). */
private T xon2a2;
/** (C * χ) / ( 2 * n² * a² ). */
private T cxo2n2a2;
/** (χ²) / (n² * a² * (χ + 1 ) ). */
private T x2on2a2xp1;
/** B * B. */
private T BB;
/**
* Simple constructor.
*
* @param auxiliaryElements auxiliary elements related to the current orbit
* @param provider provider for spherical harmonics
* @param parameters values of the force model parameters (only 1 values
* for each parameters corresponding to state date) obtained by calling the extract
* parameter method {@link #extractParameters(double[], AbsoluteDate)}
* to selected the right value for state date or by getting the parameters for a specific date
*/
FieldDSSTZonalContext(final FieldAuxiliaryElements<T> auxiliaryElements,
final UnnormalizedSphericalHarmonicsProvider provider,
final T[] parameters) {
super(auxiliaryElements);
final T mu = parameters[0];
// Keplerian mean motion
final T absA = FastMath.abs(auxiliaryElements.getSma());
n = FastMath.sqrt(mu.divide(absA)).divide(absA);
A = FastMath.sqrt(mu.multiply(auxiliaryElements.getSma()));
// Χ = 1 / B
X = auxiliaryElements.getB().reciprocal();
XX = X.square();
XXX = X.multiply(XX);
// 1 / AB
ooAB = (A.multiply(auxiliaryElements.getB())).reciprocal();
// B / A
BoA = auxiliaryElements.getB().divide(A);
// -C / 2AB
mCo2AB = auxiliaryElements.getC().multiply(ooAB).divide(2.).negate();
// B / A(1 + B)
BoABpo = BoA.divide(auxiliaryElements.getB().add(1.));
// -2 * a / A
m2aoA = auxiliaryElements.getSma().divide(A).multiply(2.).negate();
// μ / a
muoa = mu.divide(auxiliaryElements.getSma());
// R / a
roa = auxiliaryElements.getSma().divide(provider.getAe()).reciprocal();
// Short period terms
// h * k.
hk = auxiliaryElements.getH().multiply(auxiliaryElements.getK());
// k² - h².
k2mh2 = auxiliaryElements.getK().multiply(auxiliaryElements.getK()).subtract(auxiliaryElements.getH().multiply(auxiliaryElements.getH()));
// (k² - h²) / 2.
k2mh2o2 = k2mh2.divide(2.);
// 1 / (n² * a²) = 1 / (n * A)
oon2a2 = (A.multiply(n)).reciprocal();
// 1 / (n² * a) = a / (n * A)
oon2a = auxiliaryElements.getSma().multiply(oon2a2);
// χ³ / (n² * a)
x3on2a = XXX.multiply(oon2a);
// χ / (n² * a²)
xon2a2 = X.multiply(oon2a2);
// (C * χ) / ( 2 * n² * a² )
cxo2n2a2 = xon2a2.multiply(auxiliaryElements.getC()).divide(2.);
// (χ²) / (n² * a² * (χ + 1 ) )
x2on2a2xp1 = xon2a2.multiply(X).divide(X.add(1.));
// B * B
BB = auxiliaryElements.getB().multiply(auxiliaryElements.getB());
}
/** Get Χ = 1 / sqrt(1 - e²) = 1 / B.
* @return Χ
*/
public T getX() {
return X;
}
/** Get Χ².
* @return Χ².
*/
public T getXX() {
return XX;
}
/** Get Χ³.
* @return Χ³
*/
public T getXXX() {
return XXX;
}
/** Get m2aoA = -2 * a / A.
* @return m2aoA
*/
public T getM2aoA() {
return m2aoA;
}
/** Get B / A.
* @return BoA
*/
public T getBoA() {
return BoA;
}
/** Get ooAB = 1 / (A * B).
* @return ooAB
*/
public T getOoAB() {
return ooAB;
}
/** Get mCo2AB = -C / 2AB.
* @return mCo2AB
*/
public T getMCo2AB() {
return mCo2AB;
}
/** Get BoABpo = B / A(1 + B).
* @return BoABpo
*/
public T getBoABpo() {
return BoABpo;
}
/** Get μ / a .
* @return muoa
*/
public T getMuoa() {
return muoa;
}
/** Get roa = R / a.
* @return roa
*/
public T getRoa() {
return roa;
}
/** Get the Keplerian mean motion.
* <p>The Keplerian mean motion is computed directly from semi major axis
* and central acceleration constant.</p>
* @return Keplerian mean motion in radians per second
*/
public T getMeanMotion() {
return n;
}
/** Get h * k.
* @return hk
*/
public T getHK() {
return hk;
}
/** Get k² - h².
* @return k2mh2
*/
public T getK2MH2() {
return k2mh2;
}
/** Get (k² - h²) / 2.
* @return k2mh2o2
*/
public T getK2MH2O2() {
return k2mh2o2;
}
/** Get 1 / (n² * a²).
* @return oon2a2
*/
public T getOON2A2() {
return oon2a2;
}
/** Get χ³ / (n² * a).
* @return x3on2a
*/
public T getX3ON2A() {
return x3on2a;
}
/** Get χ / (n² * a²).
* @return xon2a2
*/
public T getXON2A2() {
return xon2a2;
}
/** Get (C * χ) / ( 2 * n² * a² ).
* @return cxo2n2a2
*/
public T getCXO2N2A2() {
return cxo2n2a2;
}
/** Get (χ²) / (n² * a² * (χ + 1 ) ).
* @return x2on2a2xp1
*/
public T getX2ON2A2XP1() {
return x2on2a2xp1;
}
/** Get B * B.
* @return BB
*/
public T getBB() {
return BB;
}
}