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: 24.3.420.0 (24.3.420.0)

Syntax

C++

Copy

public static Vector ScaledAngularVelocityAngularMomentumPerUnitMass(
	CentralBody centralBody,
	double scale
)

Public Shared Function ScaledAngularVelocityAngularMomentumPerUnitMass ( 
	centralBody As CentralBody,
	scale As Double
) As Vector

public:
static Vector^ ScaledAngularVelocityAngularMomentumPerUnitMass(
	CentralBody^ centralBody, 
	double scale
)

static member ScaledAngularVelocityAngularMomentumPerUnitMass : 
        centralBody : CentralBody * 
        scale : float -> Vector

Parameters

centralBody: Type: AGI.Foundation.CelestialCentralBody
The central body for which to create this vector.
scale: 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.

Reference

IersTechnicalNote36RelativisticCorrectionForce Class

AGI.Foundation.Celestial Namespace

IersTechnicalNote36RelativisticCorrectionForceAddLanguageSpecificTextSet("LST312FC115_0?cpp=::|nu=.");ScaledAngularVelocityAngularMomentumPerUnitMass Method

Parameters

Return Value

Reference

IersTechnicalNote36RelativisticCorrectionForceScaledAngularVelocityAngularMomentumPerUnitMass Method