public class CartesianOrbit extends Orbit
The parameters used internally are the Cartesian coordinates:
PVCoordinates.
Note that the implementation of this class delegates all non-Cartesian related
computations (getA(), getEquinoctialEx(), ...) to an underlying
instance of the EquinoctialOrbit class. This implies that using this class
only for analytical computations which are always based on non-Cartesian
parameters is perfectly possible but somewhat sub-optimal.
The instance CartesianOrbit is guaranteed to be immutable.
Orbit,
KeplerianOrbit,
CircularOrbit,
EquinoctialOrbit,
Serialized Form| Constructor and Description |
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CartesianOrbit(Orbit op)
Constructor from any kind of orbital parameters.
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CartesianOrbit(PVCoordinates pvaCoordinates,
Frame frame,
AbsoluteDate date,
double mu)
Constructor from Cartesian parameters.
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CartesianOrbit(TimeStampedPVCoordinates pvaCoordinates,
Frame frame,
double mu)
Constructor from Cartesian parameters.
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| Modifier and Type | Method and Description |
|---|---|
void |
addKeplerContribution(PositionAngleType type,
double gm,
double[] pDot)
Add the contribution of the Keplerian motion to parameters derivatives
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protected double[][] |
computeJacobianEccentricWrtCartesian()
Compute the Jacobian of the orbital parameters with eccentric angle with respect to the Cartesian parameters.
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protected double[][] |
computeJacobianMeanWrtCartesian()
Compute the Jacobian of the orbital parameters with mean angle with respect to the Cartesian parameters.
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protected double[][] |
computeJacobianTrueWrtCartesian()
Compute the Jacobian of the orbital parameters with true angle with respect to the Cartesian parameters.
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double |
getA()
Get the semi-major axis.
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double |
getADot()
Get the semi-major axis derivative.
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double |
getE()
Get the eccentricity.
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double |
getEDot()
Get the eccentricity derivative.
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double |
getEquinoctialEx()
Get the first component of the equinoctial eccentricity vector derivative.
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double |
getEquinoctialExDot()
Get the first component of the equinoctial eccentricity vector.
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double |
getEquinoctialEy()
Get the second component of the equinoctial eccentricity vector derivative.
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double |
getEquinoctialEyDot()
Get the second component of the equinoctial eccentricity vector.
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double |
getHx()
Get the first component of the inclination vector.
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double |
getHxDot()
Get the first component of the inclination vector derivative.
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double |
getHy()
Get the second component of the inclination vector.
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double |
getHyDot()
Get the second component of the inclination vector derivative.
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double |
getI()
Get the inclination.
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double |
getIDot()
Get the inclination derivative.
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double |
getLE()
Get the eccentric longitude argument.
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double |
getLEDot()
Get the eccentric longitude argument derivative.
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double |
getLM()
Get the mean longitude argument.
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double |
getLMDot()
Get the mean longitude argument derivative.
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double |
getLv()
Get the true longitude argument.
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double |
getLvDot()
Get the true longitude argument derivative.
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OrbitType |
getType()
Get the orbit type.
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boolean |
hasDerivatives()
Check if orbit includes derivatives.
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protected org.hipparchus.geometry.euclidean.threed.Vector3D |
initPosition()
Compute the position coordinates from the canonical parameters.
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protected TimeStampedPVCoordinates |
initPVCoordinates()
Compute the position/velocity coordinates from the canonical parameters.
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CartesianOrbit |
shiftedBy(double dt)
Get a time-shifted orbit.
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String |
toString()
Returns a string representation of this Orbit object.
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fillHalfRow, fillHalfRow, fillHalfRow, fillHalfRow, fillHalfRow, fillHalfRow, getDate, getFrame, getJacobianWrtCartesian, getJacobianWrtParameters, getKeplerianMeanMotion, getKeplerianPeriod, getMeanAnomalyDotWrtA, getMu, getPosition, getPosition, getPVCoordinates, getPVCoordinates, getPVCoordinates, hasNonKeplerianAcceleration, isEllipticalclone, equals, finalize, getClass, hashCode, notify, notifyAll, wait, wait, waitdurationFromgetPositionpublic CartesianOrbit(TimeStampedPVCoordinates pvaCoordinates, Frame frame, double mu) throws IllegalArgumentException
The acceleration provided in pvCoordinates is accessible using
Orbit.getPVCoordinates() and Orbit.getPVCoordinates(Frame). All other methods
use mu and the position to compute the acceleration, including
shiftedBy(double) and Orbit.getPVCoordinates(AbsoluteDate, Frame).
pvaCoordinates - the position, velocity and acceleration of the satellite.frame - the frame in which the PVCoordinates are defined
(must be a pseudo-inertial frame)mu - central attraction coefficient (m³/s²)IllegalArgumentException - if frame is not a pseudo-inertial framepublic CartesianOrbit(PVCoordinates pvaCoordinates, Frame frame, AbsoluteDate date, double mu) throws IllegalArgumentException
The acceleration provided in pvCoordinates is accessible using
Orbit.getPVCoordinates() and Orbit.getPVCoordinates(Frame). All other methods
use mu and the position to compute the acceleration, including
shiftedBy(double) and Orbit.getPVCoordinates(AbsoluteDate, Frame).
pvaCoordinates - the position and velocity of the satellite.frame - the frame in which the PVCoordinates are defined
(must be a pseudo-inertial frame)date - date of the orbital parametersmu - central attraction coefficient (m³/s²)IllegalArgumentException - if frame is not a pseudo-inertial framepublic CartesianOrbit(Orbit op)
op - orbital parameters to copypublic OrbitType getType()
public double getA()
Note that the semi-major axis is considered negative for hyperbolic orbits.
public double getADot()
Note that the semi-major axis is considered negative for hyperbolic orbits.
If the orbit was created without derivatives, the value returned is Double.NaN.
getADot in class OrbitOrbit.hasDerivatives()public double getE()
public double getEDot()
If the orbit was created without derivatives, the value returned is Double.NaN.
getEDot in class OrbitOrbit.hasDerivatives()public double getI()
public double getIDot()
If the orbit was created without derivatives, the value returned is Double.NaN.
getIDot in class OrbitOrbit.hasDerivatives()public double getEquinoctialEx()
getEquinoctialEx in class Orbitpublic double getEquinoctialExDot()
If the orbit was created without derivatives, the value returned is Double.NaN.
getEquinoctialExDot in class OrbitOrbit.hasDerivatives()public double getEquinoctialEy()
getEquinoctialEy in class Orbitpublic double getEquinoctialEyDot()
If the orbit was created without derivatives, the value returned is Double.NaN.
getEquinoctialEyDot in class OrbitOrbit.hasDerivatives()public double getHx()
public double getHxDot()
If the orbit was created without derivatives, the value returned is Double.NaN.
getHxDot in class OrbitOrbit.hasDerivatives()public double getHy()
public double getHyDot()
If the orbit was created without derivatives, the value returned is Double.NaN.
getHyDot in class OrbitOrbit.hasDerivatives()public double getLv()
public double getLvDot()
If the orbit was created without derivatives, the value returned is Double.NaN.
getLvDot in class OrbitOrbit.hasDerivatives()public double getLE()
public double getLEDot()
If the orbit was created without derivatives, the value returned is Double.NaN.
getLEDot in class OrbitOrbit.hasDerivatives()public double getLM()
public double getLMDot()
If the orbit was created without derivatives, the value returned is Double.NaN.
getLMDot in class OrbitOrbit.hasDerivatives()public boolean hasDerivatives()
hasDerivatives in class OrbitOrbit.getADot(),
Orbit.getEquinoctialExDot(),
Orbit.getEquinoctialEyDot(),
Orbit.getHxDot(),
Orbit.getHyDot(),
Orbit.getLEDot(),
Orbit.getLvDot(),
Orbit.getLMDot(),
Orbit.getEDot(),
Orbit.getIDot()protected org.hipparchus.geometry.euclidean.threed.Vector3D initPosition()
initPosition in class Orbitprotected TimeStampedPVCoordinates initPVCoordinates()
initPVCoordinates in class Orbitpublic CartesianOrbit shiftedBy(double dt)
The orbit can be slightly shifted to close dates. The shifting model is a Keplerian one if no derivatives are available in the orbit, or Keplerian plus quadratic effect of the non-Keplerian acceleration if derivatives are available. Shifting is not intended as a replacement for proper orbit propagation but should be sufficient for small time shifts or coarse accuracy.
shiftedBy in interface TimeShiftable<Orbit>shiftedBy in class Orbitdt - time shift in secondsprotected double[][] computeJacobianMeanWrtCartesian()
Orbit
Element jacobian[i][j] is the derivative of parameter i of the orbit with
respect to Cartesian coordinate j. This means each row correspond to one orbital parameter
whereas columns 0 to 5 correspond to the Cartesian coordinates x, y, z, xDot, yDot and zDot.
The array returned by this method will not be modified.
computeJacobianMeanWrtCartesian in class OrbitOrbit.computeJacobianEccentricWrtCartesian(),
Orbit.computeJacobianTrueWrtCartesian()protected double[][] computeJacobianEccentricWrtCartesian()
Orbit
Element jacobian[i][j] is the derivative of parameter i of the orbit with
respect to Cartesian coordinate j. This means each row correspond to one orbital parameter
whereas columns 0 to 5 correspond to the Cartesian coordinates x, y, z, xDot, yDot and zDot.
The array returned by this method will not be modified.
computeJacobianEccentricWrtCartesian in class OrbitOrbit.computeJacobianMeanWrtCartesian(),
Orbit.computeJacobianTrueWrtCartesian()protected double[][] computeJacobianTrueWrtCartesian()
Orbit
Element jacobian[i][j] is the derivative of parameter i of the orbit with
respect to Cartesian coordinate j. This means each row correspond to one orbital parameter
whereas columns 0 to 5 correspond to the Cartesian coordinates x, y, z, xDot, yDot and zDot.
The array returned by this method will not be modified.
computeJacobianTrueWrtCartesian in class OrbitOrbit.computeJacobianMeanWrtCartesian(),
Orbit.computeJacobianEccentricWrtCartesian()public void addKeplerContribution(PositionAngleType type, double gm, double[] pDot)
This method is used by integration-based propagators to evaluate the part of Keplerian motion to evolution of the orbital state.
addKeplerContribution in class Orbittype - type of the position angle in the stategm - attraction coefficient to usepDot - array containing orbital state derivatives to update (the Keplerian
part must be added to the array components, as the array may already
contain some non-zero elements corresponding to non-Keplerian parts)Copyright © 2002-2023 CS GROUP. All rights reserved.