Uses of Class
edu.nrao.sss.astronomy.VelocityFrame

Packages that use VelocityFrame

edu.nrao.sss.astronomy	General astronomical concepts.
edu.nrao.sss.geom	Geometric concepts.

Uses of VelocityFrame in edu.nrao.sss.astronomy

Methods in edu.nrao.sss.astronomy that return VelocityFrame

static VelocityFrame	VelocityFrame.fromString(String text) Returns the velocity frame represented by text.
static VelocityFrame	VelocityFrame.getDefault() Returns a default velocity frame.
VelocityFrame	DopplerTracker.getVelocityFrame() Returns the rest frame against which velocity values will be calculated.
static VelocityFrame	VelocityFrame.valueOf(String name) Returns the enum constant of this type with the specified name.
static VelocityFrame[]	VelocityFrame.values() Returns an array containing the constants of this enum type, in the order they are declared.

Methods in edu.nrao.sss.astronomy with parameters of type VelocityFrame

void	DopplerTracker.setSource(SkyPosition newPosition, LinearVelocity newVelocity, VelocityFrame newFrame, VelocityConvention newConvention) A convenience method for setting the position and velocity of a celestial source.
void	DopplerTracker.setSourceVelocity(LinearVelocity newVelocity, VelocityFrame newFrame, VelocityConvention newConvention) A convenience method for setting the source velocity and frame.
void	DopplerTracker.setVelocityFrame(VelocityFrame newFrame) Sets the rest frame against which velocity values will be calculated.

Constructors in edu.nrao.sss.astronomy with parameters of type VelocityFrame

DopplerTracker(EarthPosition observer, SkyPosition skyPosition, LinearVelocity sourceVelocity, VelocityFrame sourceFrame, VelocityConvention velocityConvention)
Creates a new Doppler tracker with the given parameters.

Uses of VelocityFrame in edu.nrao.sss.geom

Methods in edu.nrao.sss.geom with parameters of type VelocityFrame

LinearVelocity

EarthPosition.calcVelocityRelativeTo(SkyPosition skyPosition, Date calcTime, VelocityFrame referenceFrame) Returns the velocity of this position to the given sky position at a particular point in time and with respect to the given frame of reference.