[x, y] = ERFA.fw2xy(gamb, phib, psi, eps)
CIP X,Y given Fukushima-Williams bias-precession-nutation angles.
gamb double F-W angle gamma_bar (radians)
phib double F-W angle phi_bar (radians)
psi double F-W angle psi (radians)
eps double F-W angle epsilon (radians)
x,y double CIP unit vector X,Y
e = J2000.0 ecliptic pole,
p = GCRS pole
E = ecliptic pole of date,
and P = CIP,
the four Fukushima-Williams angles are as follows:
gamb = gamma = epE
phib = phi = pE
psi = psi = pEP
eps = epsilon = EP
- The matrix representing the combined effects of frame bias, precession and nutation is:
NxPxB = R_1(-epsA).R_3(-psi).R_1(phib).R_3(gamb)
The returned values x,y are elements [2][0] and [2][1] of the matrix. Near J2000.0, they are essentially angles in radians.
eraFw2m F-W angles to r-matrix
eraBpn2xy extract CIP X,Y coordinates from NPB matrix
Hilton, J. et al., 2006, Celest.Mech.Dyn.Astron. 94, 351
This revision: 2021 May 11
Copyright (C) 2013-2021, NumFOCUS Foundation. Derived, with permission, from the SOFA library.