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IersTechnicalNote36RelativisticCorrectionForceScaledAngularVelocityAngularMomentumPerUnitMass Method

A static helper method that computes a CentralBodyAngularMomentumPerUnitMass vector for the input centralBody. This method computes the rotational velocity between the central body's fixed and inertial frames. This vector is then normalized and the magnitude is set to the input scale factor. An appropriate scale factor for the Earth, for example, would be 9.8e8 m^2/s as was cited in "IERS Conventions (2010)".

Namespace:  AGI.Foundation.Celestial
Assembly:  AGI.Foundation.OrbitPropagation (in AGI.Foundation.OrbitPropagation.dll) Version: 24.1.418.0 (24.1.418.0)
public static Vector ScaledAngularVelocityAngularMomentumPerUnitMass(
	CentralBody centralBody,
	double scale


Type: AGI.Foundation.CelestialCentralBody
The central body for which to create this vector.
Type: SystemDouble
A double that represents the value of the magnitude of the output vector.

Return Value

Type: Vector
A vector suitable for use with the CentralBodyAngularMomentumPerUnitMass property.
See Also