SofaBpn2xy Method
Extract the CIP X,Y coordinates from a bias-precession-nutation matrix.
Namespace: ASCOM.ToolsAssembly: ASCOM.AstrometryTools (in ASCOM.AstrometryTools.dll) Version: 3.0.0-rc.1+86c25ce733aebb4d8b1b8a62e84770ea5e972bea
public static void Bpn2xy(
double[] rbpn,
ref double x,
ref double y
)
Public Shared Sub Bpn2xy (
rbpn As Double(),
ByRef x As Double,
ByRef y As Double
)
Parameters
- rbpn Double
- Celestial-to-true rotation matrix (row-major, length 9).
- x Double
- Returned X coordinate of the Celestial Intermediate Pole (GCRS).
- y Double
- Returned Y coordinate of the Celestial Intermediate Pole (GCRS).
The input matrix transforms vectors from GCRS to the true equator (and CIO/equinox) of date; the CIP unit vector is the
bottom row of the matrix.
Supported in: 2.0