Interface | Description |
---|---|
AdditionalStateProvider |
This interface represents providers for additional state data beyond
SpacecraftState . |
BoundedPropagator |
This interface is intended for ephemerides valid only during a time range.
|
FieldAdditionalStateProvider<T extends org.hipparchus.RealFieldElement<T>> |
This interface represents providers for additional state data beyond
SpacecraftState . |
FieldBoundedPropagator<T extends org.hipparchus.RealFieldElement<T>> |
This interface is intended for ephemerides valid only during a time range.
|
FieldPropagator<T extends org.hipparchus.RealFieldElement<T>> |
This interface provides a way to propagate an orbit at any time.
|
Propagator |
This interface provides a way to propagate an orbit at any time.
|
Class | Description |
---|---|
AbstractPropagator |
Common handling of
Propagator methods for analytical propagators. |
FieldAbstractPropagator<T extends org.hipparchus.RealFieldElement<T>> |
Common handling of
Propagator methods for analytical propagators. |
FieldSpacecraftState<T extends org.hipparchus.RealFieldElement<T>> |
This class is the representation of a complete state holding orbit, attitude
and mass information at a given date.
|
PropagatorsParallelizer |
This class provides a way to propagate simultaneously several orbits.
|
SpacecraftState |
This class is the representation of a complete state holding orbit, attitude
and mass information at a given date.
|
Propagation is the prediction of the evolution of an initial state.
The initial state and the propagated states are represented in OREKIT by a
SpacecraftState
, which is a simple container
for all needed information at a specific date : mass,
kinematics
,
attitude
,
date
,
frame
. The state provides basic interpolation
features allowing to shift it slightly to close dates. For more accurate and
farthest dates, several full-featured propagators are available to propagate
the state.
The KeplerianPropagator
implements the Propagator
interface, which ensures that we can obtain a propagated SpacecraftState
at any time once the instance is initialized with an initial state.
This extrapolation is not a problem with a simple
EquinoctialOrbit
representation: only the mean anomaly value changes.
This analytical model is suited for near circular orbits and inclination
neither equatorial nor critical. It considers J2 to J6 potential
coefficients correctors, and uses mean parameters to compute the new
position. As the Keplerian propagator, it implements the
Propagator
interface.
It is the most important part of the OREKIT project. Based on Hipparchus
integrators, the NumericalPropagator
class realizes the interface between space mechanics and mathematical
resolutions. If its utilization seems difficult on first sight, it is in
fact quite clear and intuitive.
The mathematical problem to integrate is a seven dimension time derivative
equations system. The six first equations are given by the Gauss equations
(expressed in EquinoctialOrbit
) and the seventh
is simply the flow rate and mass equation. This first order system is computed
by the TimeDerivativesEquations
class. It will be instanced by the propagator and then be modified at each
step (a fixed t value) by all the needed force models
which will add their contribution,
the perturbing acceleration.
The integrators
provided by Hipparchus need the state vector at t0, the state vector first
time derivate at t0, and then calculates the next step state vector, and ask
for the next first time derivative, etc. until it reaches the final asked date.
Copyright © 2002-2017 CS Systèmes d'information. All rights reserved.