public class DSSTSolarRadiationPressure extends AbstractGaussianContribution
DSSTPropagator.
The solar radiation pressure acceleration is computed through the
acceleration model of
SolarRadiationPressure.
| Constructor and Description |
|---|
DSSTSolarRadiationPressure(double dRef,
double pRef,
double cr,
double area,
PVCoordinatesProvider sun,
double equatorialRadius)
Constructor with customizable reference values but spherical spacecraft.
|
DSSTSolarRadiationPressure(double cr,
double area,
PVCoordinatesProvider sun,
double equatorialRadius)
Simple constructor with default reference values and spherical spacecraft.
|
DSSTSolarRadiationPressure(double dRef,
double pRef,
PVCoordinatesProvider sun,
double equatorialRadius,
RadiationSensitive spacecraft)
Complete constructor.
|
DSSTSolarRadiationPressure(PVCoordinatesProvider sun,
double equatorialRadius,
RadiationSensitive spacecraft)
Simple constructor with default reference values, but custom spacecraft.
|
| Modifier and Type | Method and Description |
|---|---|
double |
getEquatorialRadius()
Get the central body equatorial radius.
|
EventDetector[] |
getEventsDetectors()
Get the discrete events related to the model.
|
protected double[] |
getLLimits(SpacecraftState state)
Compute the limits in L, the true longitude, for integration.
|
RadiationSensitive |
getSpacecraft()
Get spacecraft shape.
|
getAcceleration, getMeanElementRate, initialize, initializeStep, registerAttitudeProvider, updateShortPeriodTermspublic DSSTSolarRadiationPressure(double cr,
double area,
PVCoordinatesProvider sun,
double equatorialRadius)
When this constructor is used, the reference values are:
The spacecraft has a spherical shape.
cr - satellite radiation pressure coefficient (assuming total specular reflection)area - cross sectionnal area of satellitesun - Sun modelequatorialRadius - central body equatorial radius (for shadow computation)public DSSTSolarRadiationPressure(PVCoordinatesProvider sun, double equatorialRadius, RadiationSensitive spacecraft)
When this constructor is used, the reference values are:
sun - Sun modelequatorialRadius - central body equatorial radius (for shadow computation)spacecraft - spacecraft modelpublic DSSTSolarRadiationPressure(double dRef,
double pRef,
double cr,
double area,
PVCoordinatesProvider sun,
double equatorialRadius)
Note that reference solar radiation pressure pRef in N/m² is linked
to solar flux SF in W/m² using formula pRef = SF/c where c is the speed of light
(299792458 m/s). So at 1UA a 1367 W/m² solar flux is a 4.56 10-6
N/m² solar radiation pressure.
dRef - reference distance for the solar radiation pressure (m)pRef - reference solar radiation pressure at dRef (N/m²)cr - satellite radiation pressure coefficient (assuming total specular reflection)area - cross sectionnal area of satellitesun - Sun modelequatorialRadius - central body equatrial radius (for shadow computation)public DSSTSolarRadiationPressure(double dRef,
double pRef,
PVCoordinatesProvider sun,
double equatorialRadius,
RadiationSensitive spacecraft)
Note that reference solar radiation pressure pRef in N/m² is linked
to solar flux SF in W/m² using formula pRef = SF/c where c is the speed of light
(299792458 m/s). So at 1UA a 1367 W/m² solar flux is a 4.56 10-6
N/m² solar radiation pressure.
dRef - reference distance for the solar radiation pressure (m)pRef - reference solar radiation pressure at dRef (N/m²)sun - Sun modelequatorialRadius - central body equatrial radius (for shadow computation)spacecraft - spacecraft modelpublic RadiationSensitive getSpacecraft()
public EventDetector[] getEventsDetectors()
protected double[] getLLimits(SpacecraftState state) throws OrekitException
getLLimits in class AbstractGaussianContributionstate - current state information: date, kinematics, attitudeOrekitException - if some specific error occurspublic double getEquatorialRadius()
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