FieldTimeInterpolable<FieldSpacecraftState<T>,T>
, FieldTimeShiftable<FieldSpacecraftState<T>,T>
, FieldTimeStamped<T>
public class FieldSpacecraftState<T extends org.hipparchus.RealFieldElement<T>> extends Object implements FieldTimeStamped<T>, FieldTimeShiftable<FieldSpacecraftState<T>,T>, FieldTimeInterpolable<FieldSpacecraftState<T>,T>
It contains an orbital state
at a current
FieldAbsoluteDate
both handled by an FieldOrbit
, plus the current
mass and attitude. FieldOrbitand state are guaranteed to be consistent in terms
of date and reference frame. The spacecraft state may also contain additional
states, which are simply named double arrays which can hold any user-defined
data.
The state can be slightly shifted to close dates. This shift is based on a simple Keplerian model for orbit, a linear extrapolation for attitude taking the spin rate into account and no mass change. It is not intended as a replacement for proper orbit and attitude propagation but should be sufficient for either small time shifts or coarse accuracy.
The instance FieldSpacecraftState
is guaranteed to be immutable.
NumericalPropagator
Constructor | Description |
---|---|
FieldSpacecraftState(org.hipparchus.Field<T> field,
SpacecraftState state) |
Convert a
SpacecraftState . |
FieldSpacecraftState(FieldOrbit<T> orbit) |
Build a spacecraft state from orbit only.
|
FieldSpacecraftState(FieldOrbit<T> orbit,
Map<String,T[]> additional) |
Build a spacecraft state from orbit only.
|
FieldSpacecraftState(FieldOrbit<T> orbit,
FieldAttitude<T> attitude) |
Build a spacecraft state from orbit and attitude provider.
|
FieldSpacecraftState(FieldOrbit<T> orbit,
FieldAttitude<T> attitude,
Map<String,T[]> additional) |
Build a spacecraft state from orbit and attitude provider.
|
FieldSpacecraftState(FieldOrbit<T> orbit,
FieldAttitude<T> attitude,
T mass) |
Build a spacecraft state from orbit, attitude provider and mass.
|
FieldSpacecraftState(FieldOrbit<T> orbit,
FieldAttitude<T> attitude,
T mass,
Map<String,T[]> additional) |
Build a spacecraft state from orbit, attitude provider and mass.
|
FieldSpacecraftState(FieldOrbit<T> orbit,
T mass) |
Create a new instance from orbit and mass.
|
FieldSpacecraftState(FieldOrbit<T> orbit,
T mass,
Map<String,T[]> additional) |
Create a new instance from orbit and mass.
|
Modifier and Type | Method | Description |
---|---|---|
FieldSpacecraftState<T> |
addAdditionalState(String name,
T... value) |
Add an additional state.
|
void |
ensureCompatibleAdditionalStates(FieldSpacecraftState<T> state) |
Check if two instances have the same set of additional states available.
|
T |
getA() |
Get the semi-major axis.
|
T[] |
getAdditionalState(String name) |
Get an additional state.
|
Map<String,T[]> |
getAdditionalStates() |
Get an unmodifiable map of additional states.
|
FieldAttitude<T> |
getAttitude() |
Get the attitude.
|
FieldAbsoluteDate<T> |
getDate() |
Get the date.
|
T |
getE() |
Get the eccentricity.
|
T |
getEquinoctialEx() |
Get the first component of the eccentricity vector (as per equinoctial parameters).
|
T |
getEquinoctialEy() |
Get the second component of the eccentricity vector (as per equinoctial parameters).
|
Frame |
getFrame() |
Get the inertial frame.
|
T |
getHx() |
Get the first component of the inclination vector (as per equinoctial parameters).
|
T |
getHy() |
Get the second component of the inclination vector (as per equinoctial parameters).
|
T |
getI() |
Get the inclination.
|
T |
getKeplerianMeanMotion() |
Get the Keplerian mean motion.
|
T |
getKeplerianPeriod() |
Get the Keplerian period.
|
T |
getLE() |
Get the eccentric latitude argument (as per equinoctial parameters).
|
T |
getLM() |
Get the mean latitude argument (as per equinoctial parameters).
|
T |
getLv() |
Get the true latitude argument (as per equinoctial parameters).
|
T |
getMass() |
Gets the current mass.
|
double |
getMu() |
Get the central attraction coefficient.
|
FieldOrbit<T> |
getOrbit() |
Gets the current orbit.
|
TimeStampedFieldPVCoordinates<T> |
getPVCoordinates() |
Get the
TimeStampedFieldPVCoordinates in orbit definition frame. |
TimeStampedFieldPVCoordinates<T> |
getPVCoordinates(Frame outputFrame) |
Get the
TimeStampedFieldPVCoordinates in given output frame. |
boolean |
hasAdditionalState(String name) |
Check if an additional state is available.
|
FieldSpacecraftState<T> |
interpolate(FieldAbsoluteDate<T> date,
Stream<FieldSpacecraftState<T>> sample) |
Get an interpolated instance.
|
FieldSpacecraftState<T> |
shiftedBy(double dt) |
Get a time-shifted state.
|
FieldSpacecraftState<T> |
shiftedBy(T dt) |
Get a time-shifted state.
|
SpacecraftState |
toSpacecraftState() |
To convert a FieldSpacecraftState instance into a SpacecraftState instance.
|
FieldTransform<T> |
toTransform() |
Compute the transform from orbite/attitude reference frame to spacecraft frame.
|
interpolate
public FieldSpacecraftState(FieldOrbit<T> orbit)
FieldAttitude
orbit
- the orbitpublic FieldSpacecraftState(FieldOrbit<T> orbit, FieldAttitude<T> attitude) throws IllegalArgumentException
Mass is set to an unspecified non-null arbitrary value.
orbit
- the orbitattitude
- attitudeIllegalArgumentException
- if orbit and attitude dates
or frames are not equalpublic FieldSpacecraftState(FieldOrbit<T> orbit, T mass)
FieldAttitude
orbit
- the orbitmass
- the mass (kg)public FieldSpacecraftState(FieldOrbit<T> orbit, FieldAttitude<T> attitude, T mass) throws IllegalArgumentException
orbit
- the orbitattitude
- attitudemass
- the mass (kg)IllegalArgumentException
- if orbit and attitude dates
or frames are not equalpublic FieldSpacecraftState(FieldOrbit<T> orbit, Map<String,T[]> additional)
FieldAttitude
orbit
- the orbitadditional
- additional statespublic FieldSpacecraftState(FieldOrbit<T> orbit, FieldAttitude<T> attitude, Map<String,T[]> additional) throws IllegalArgumentException
Mass is set to an unspecified non-null arbitrary value.
orbit
- the orbitattitude
- attitudeadditional
- additional statesIllegalArgumentException
- if orbit and attitude dates
or frames are not equalpublic FieldSpacecraftState(FieldOrbit<T> orbit, T mass, Map<String,T[]> additional)
FieldAttitude
orbit
- the orbitmass
- the mass (kg)additional
- additional statespublic FieldSpacecraftState(FieldOrbit<T> orbit, FieldAttitude<T> attitude, T mass, Map<String,T[]> additional) throws IllegalArgumentException
orbit
- the orbitattitude
- attitudemass
- the mass (kg)additional
- additional states (may be null if no additional states are available)IllegalArgumentException
- if orbit and attitude dates
or frames are not equalpublic FieldSpacecraftState(org.hipparchus.Field<T> field, SpacecraftState state)
SpacecraftState
.field
- field to which the elements belongstate
- state to convert@SafeVarargs public final FieldSpacecraftState<T> addAdditionalState(String name, T... value)
SpacecraftState
instances are immutable,
so this method does not change the instance, but rather
creates a new instance, which has the same orbit, attitude, mass
and additional states as the original instance, except it also
has the specified state. If the original instance already had an
additional state with the same name, it will be overridden. If it
did not have any additional state with that name, the new instance
will have one more additional state than the original instance.
name
- name of the additional statevalue
- value of the additional statehasAdditionalState(String)
,
getAdditionalState(String)
,
getAdditionalStates()
public FieldSpacecraftState<T> shiftedBy(double dt)
The state can be slightly shifted to close dates. This shift is based on a simple Keplerian model for orbit, a linear extrapolation for attitude taking the spin rate into account and neither mass nor additional states changes. It is not intended as a replacement for proper orbit and attitude propagation but should be sufficient for small time shifts or coarse accuracy.
As a rough order of magnitude, the following table shows the extrapolation
errors obtained between this simple shift method and an numerical
propagator
for a low Earth Sun Synchronous Orbit, with a 20x20 gravity field,
Sun and Moon third bodies attractions, drag and solar radiation pressure.
Beware that these results will be different for other orbits.
interpolation time (s) | position error without derivatives (m) | position error with derivatives (m) |
---|---|---|
60 | 18 | 1.1 |
120 | 72 | 9.1 |
300 | 447 | 140 |
600 | 1601 | 1067 |
900 | 3141 | 3307 |
shiftedBy
in interface FieldTimeShiftable<FieldSpacecraftState<T extends org.hipparchus.RealFieldElement<T>>,T extends org.hipparchus.RealFieldElement<T>>
dt
- time shift in secondspublic FieldSpacecraftState<T> shiftedBy(T dt)
The state can be slightly shifted to close dates. This shift is based on a simple Keplerian model for orbit, a linear extrapolation for attitude taking the spin rate into account and neither mass nor additional states changes. It is not intended as a replacement for proper orbit and attitude propagation but should be sufficient for small time shifts or coarse accuracy.
As a rough order of magnitude, the following table shows the extrapolation
errors obtained between this simple shift method and an numerical
propagator
for a low Earth Sun Synchronous Orbit, with a 20x20 gravity field,
Sun and Moon third bodies attractions, drag and solar radiation pressure.
Beware that these results will be different for other orbits.
interpolation time (s) | position error without derivatives (m) | position error with derivatives (m) |
---|---|---|
60 | 18 | 1.1 |
120 | 72 | 9.1 |
300 | 447 | 140 |
600 | 1601 | 1067 |
900 | 3141 | 3307 |
shiftedBy
in interface FieldTimeShiftable<FieldSpacecraftState<T extends org.hipparchus.RealFieldElement<T>>,T extends org.hipparchus.RealFieldElement<T>>
dt
- time shift in secondspublic FieldSpacecraftState<T> interpolate(FieldAbsoluteDate<T> date, Stream<FieldSpacecraftState<T>> sample)
The additional states that are interpolated are the ones already present in the instance. The sample instances must therefore have at least the same additional states has the instance. They may have more additional states, but the extra ones will be ignored.
As this implementation of interpolation is polynomial, it should be used only with small samples (about 10-20 points) in order to avoid Runge's phenomenon and numerical problems (including NaN appearing).
interpolate
in interface FieldTimeInterpolable<FieldSpacecraftState<T extends org.hipparchus.RealFieldElement<T>>,T extends org.hipparchus.RealFieldElement<T>>
date
- interpolation datesample
- sample points on which interpolation should be donepublic FieldOrbit<T> getOrbit()
public FieldAbsoluteDate<T> getDate()
getDate
in interface FieldTimeStamped<T extends org.hipparchus.RealFieldElement<T>>
public Frame getFrame()
public boolean hasAdditionalState(String name)
name
- name of the additional stateaddAdditionalState(String, RealFieldElement...)
,
getAdditionalState(String)
,
getAdditionalStates()
public void ensureCompatibleAdditionalStates(FieldSpacecraftState<T> state) throws org.hipparchus.exception.MathIllegalArgumentException
Only the names and dimensions of the additional states are compared, not their values.
state
- state to compare to instanceorg.hipparchus.exception.MathIllegalArgumentException
- if an additional state does not have
the same dimension in both statespublic T[] getAdditionalState(String name)
name
- name of the additional stateaddAdditionalState(String, RealFieldElement...)
,
hasAdditionalState(String)
,
getAdditionalStates()
public Map<String,T[]> getAdditionalStates()
addAdditionalState(String, RealFieldElement...)
,
hasAdditionalState(String)
,
getAdditionalState(String)
public FieldTransform<T> toTransform()
The spacecraft frame origin is at the point defined by the orbit, and its orientation is defined by the attitude.
public double getMu()
public T getKeplerianPeriod()
The Keplerian period is computed directly from semi major axis and central acceleration constant.
public T getKeplerianMeanMotion()
The Keplerian mean motion is computed directly from semi major axis and central acceleration constant.
public T getA()
public T getEquinoctialEx()
getE()
public T getEquinoctialEy()
getE()
public T getHx()
getI()
public T getHy()
getI()
public T getLv()
public T getLE()
public T getLM()
public T getE()
getEquinoctialEx()
,
getEquinoctialEy()
public TimeStampedFieldPVCoordinates<T> getPVCoordinates()
TimeStampedFieldPVCoordinates
in orbit definition frame.
Compute the position and velocity of the satellite. This method caches its
results, and recompute them only when the method is called with a new value
for mu. The result is provided as a reference to the internally cached
TimeStampedFieldPVCoordinates
, so the caller is responsible to copy it in a separate
TimeStampedFieldPVCoordinates
if it needs to keep the value for a while.public TimeStampedFieldPVCoordinates<T> getPVCoordinates(Frame outputFrame)
TimeStampedFieldPVCoordinates
in given output frame.
Compute the position and velocity of the satellite. This method caches its
results, and recompute them only when the method is called with a new value
for mu. The result is provided as a reference to the internally cached
TimeStampedFieldPVCoordinates
, so the caller is responsible to copy it in a separate
TimeStampedFieldPVCoordinates
if it needs to keep the value for a while.outputFrame
- frame in which coordinates should be definedpublic FieldAttitude<T> getAttitude()
public T getMass()
public SpacecraftState toSpacecraftState()
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