public final class CircularOrbit extends Orbit
The parameters used internally are the circular elements (see CircularParameters
for more information.
The instance CircularOrbit
is guaranteed to be immutable.
Orbit
,
KeplerianOrbit
,
CartesianOrbit
,
EquinoctialOrbit
,
Serialized FormConstructor and Description |
---|
CircularOrbit(double a,
double ex,
double ey,
double i,
double raan,
double alpha,
PositionAngle type,
Frame frame,
AbsoluteDate date,
double mu)
Creates a new instance.
|
CircularOrbit(IOrbitalParameters parametersIn,
Frame frame,
AbsoluteDate date)
Creates a new instance.
|
CircularOrbit(Orbit op)
Constructor from any kind of orbital parameters.
|
CircularOrbit(PVCoordinates pvCoordinates,
Frame frame,
AbsoluteDate date,
double mu)
Constructor from cartesian parameters.
|
Modifier and Type | Method and Description |
---|---|
protected double[][] |
computeJacobianEccentricWrtCartesian()
Compute the Jacobian of the orbital parameters with eccentric angle with respect to the Cartesian parameters.
|
protected double[][] |
computeJacobianMeanWrtCartesian()
Compute the Jacobian of the orbital parameters with mean angle with respect to the Cartesian parameters.
|
protected double[][] |
computeJacobianTrueWrtCartesian()
Compute the Jacobian of the orbital parameters with true angle with respect to the Cartesian parameters.
|
double |
getA()
Get the semi-major axis.
|
double |
getAlpha(PositionAngle type)
Get the latitude argument.
|
double |
getAlphaE()
Get the eccentric latitude argument.
|
double |
getAlphaM()
Get the mean latitude argument.
|
double |
getAlphaV()
Get the true latitude argument.
|
double |
getCircularEx()
Get the first component of the circular eccentricity vector.
|
double |
getCircularEy()
Get the second component of the circular eccentricity vector.
|
CircularParameters |
getCircularParameters()
Getter for underlying circular parameters.
|
double |
getE()
Get the eccentricity.
|
double |
getEquinoctialEx()
Get the first component of the equinoctial eccentricity vector.
|
double |
getEquinoctialEy()
Get the second component of the equinoctial eccentricity vector.
|
double |
getHx()
Get hx = ix / (2 * cos(i/2)), where ix is the first component of the inclination vector.
|
double |
getHy()
Get hy = iy / (2 * cos(i/2)), where iy is the second component of the inclination vector.
|
double |
getI()
Get the inclination.
|
double |
getLE()
Get the eccentric longitude argument.
|
double |
getLM()
Get the mean longitude argument.
|
double |
getLv()
Get the true longitude argument.
|
IOrbitalParameters |
getParameters()
Get underlying orbital parameters.
|
double |
getRightAscensionOfAscendingNode()
Get the right ascension of the ascending node.
|
OrbitType |
getType()
Get the orbit type.
|
protected PVCoordinates |
initPVCoordinates()
Compute the position/velocity coordinates from the canonical parameters.
|
CircularOrbit |
interpolate(AbsoluteDate date,
Collection<Orbit> sample)
Get an interpolated instance.
|
protected void |
orbitAddKeplerContribution(PositionAngle type,
double gm,
double[] pDot)
Add the contribution of the Keplerian motion to parameters derivatives
|
protected CircularOrbit |
orbitShiftedBy(double dt)
Get a time-shifted orbit.
|
String |
toString() |
addKeplerContribution, createInverseJacobian, fillHalfRow, fillHalfRow, fillHalfRow, fillHalfRow, fillHalfRow, fillHalfRow, getDate, getFrame, getJacobian, getJacobianWrtCartesian, getJacobianWrtParameters, getJacobianWrtParametersEccentric, getJacobianWrtParametersMean, getJacobianWrtParametersTrue, getKeplerianMeanMotion, getKeplerianPeriod, getKeplerianTransitionMatrix, getMu, getPVCoordinates, getPVCoordinates, getPVCoordinates, isPositiveDefinite, setJacobianWrtParametersEccentric, setJacobianWrtParametersMean, setJacobianWrtParametersTrue, shiftedBy
public CircularOrbit(IOrbitalParameters parametersIn, Frame frame, AbsoluteDate date)
parametersIn
- orbital parametersframe
- the frame in which the parameters are defined
(must be a pseudo-inertial frame
)date
- date of the orbital parameterspublic CircularOrbit(double a, double ex, double ey, double i, double raan, double alpha, PositionAngle type, Frame frame, AbsoluteDate date, double mu)
a
- semi-major axis (m)ex
- e cos(ω), first component of circular eccentricity vectorey
- e sin(ω), second component of circular eccentricity vectori
- inclination (rad)raan
- right ascension of ascending node (Ω, rad)alpha
- an + ω, mean, eccentric or true latitude argument (rad)type
- type of latitude argumentframe
- the frame in which are defined the parametersdate
- date of the orbital parametersmu
- central attraction coefficient (m3/s2)IllegalArgumentException
- if eccentricity is equal to 1 or largerpublic CircularOrbit(PVCoordinates pvCoordinates, Frame frame, AbsoluteDate date, double mu)
pvCoordinates
- the PVCoordinates
in inertial frameframe
- the frame in which are defined the PVCoordinates
date
- date of the orbital parametersmu
- central attraction coefficient (m3/s2)public CircularOrbit(Orbit op)
op
- orbital parameters to copypublic IOrbitalParameters getParameters()
getParameters
in class Orbit
public CircularParameters getCircularParameters()
public OrbitType getType()
public double getA()
Note that the semi-major axis is considered negative for hyperbolic orbits.
public double getEquinoctialEx()
getEquinoctialEx
in class Orbit
public double getEquinoctialEy()
getEquinoctialEy
in class Orbit
public double getCircularEx()
public double getCircularEy()
public double getHx()
public double getHy()
public double getAlphaV()
public double getAlpha(PositionAngle type)
type
- type of the anglepublic double getAlphaE()
public double getAlphaM()
public double getE()
public double getI()
public double getRightAscensionOfAscendingNode()
public double getLv()
public double getLE()
public double getLM()
protected PVCoordinates initPVCoordinates()
initPVCoordinates
in class Orbit
protected CircularOrbit orbitShiftedBy(double dt)
The orbit can be slightly shifted to close dates. This shift is based on a simple keplerian model. It is not intended as a replacement for proper orbit and attitude propagation but should be sufficient for small time shifts or coarse accuracy.
orbitShiftedBy
in class Orbit
dt
- time shift in secondspublic CircularOrbit interpolate(AbsoluteDate date, Collection<Orbit> sample)
Note that the state of the current instance may not be used in the interpolation process, only its type and non interpolable fields are used (for example central attraction coefficient or frame when interpolating orbits). The interpolable fields taken into account are taken only from the states of the sample points. So if the state of the instance must be used, the instance should be included in the sample points.
The interpolated instance is created by polynomial Hermite interpolation on circular elements, without derivatives (which means the interpolation falls back to Lagrange interpolation only).
date
- interpolation datesample
- sample points on which interpolation should be doneprotected double[][] computeJacobianMeanWrtCartesian()
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.
computeJacobianMeanWrtCartesian
in class Orbit
Orbit.computeJacobianEccentricWrtCartesian()
,
Orbit.computeJacobianTrueWrtCartesian()
protected double[][] computeJacobianEccentricWrtCartesian()
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.
computeJacobianEccentricWrtCartesian
in class Orbit
Orbit.computeJacobianMeanWrtCartesian()
,
Orbit.computeJacobianTrueWrtCartesian()
protected double[][] computeJacobianTrueWrtCartesian()
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.
computeJacobianTrueWrtCartesian
in class Orbit
Orbit.computeJacobianMeanWrtCartesian()
,
Orbit.computeJacobianEccentricWrtCartesian()
protected void orbitAddKeplerContribution(PositionAngle type, double gm, double[] pDot)
This method is used by numerical propagators to evaluate the part of Keplerrian motion to evolution of the orbital state.
orbitAddKeplerContribution
in class Orbit
type
- 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 © 2018 CNES. All Rights Reserved.