XYS00B Subroutine

  1. astro_module.f90
  2. astro_module
  3. XYS00B

public subroutine XYS00B(date1, date2, x, y, s)

For a given TT date, compute the X,Y coordinates of the Celestial Intermediate Pole and the CIO locator s, using the IAU 2000B precession-nutation model.

Status: support routine.

Notes

  1. The TT date DATE1+DATE2 is a Julian Date, apportioned in any convenient way between the two arguments. For example, JD(TT)=2450123.7 could be expressed in any of these ways, among others:

        DATE1          DATE2

 2450123.7D0        0D0        (JD method)
  2451545D0      -1421.3D0     (J2000 method)
 2400000.5D0     50123.2D0     (MJD method)
 2450123.5D0       0.2D0       (date & time method)

    The JD method is the most natural and convenient to use in cases where the loss of several decimal digits of resolution is acceptable. The J2000 method is best matched to the way the argument is handled internally and will deliver the optimum resolution. The MJD method and the date & time methods are both good compromises between resolution and convenience.

  2. The Celestial Intermediate Pole coordinates are the x,y components of the unit vector in the Geocentric Celestial Reference System.

  3. The CIO locator s (in radians) positions the Celestial Intermediate Origin on the equator of the CIP.

  4. The present routine is faster, but slightly less accurate (about 1 mas in X,Y), than the XYS00A routine.

Reference

  • McCarthy, D. D., Petit, G. (eds.), IERS Conventions (2003), IERS Technical Note No. 32, BKG (2004)

History

  • IAU SOFA revision: 2006 November 13

Arguments

TypeIntentOptionalAttributesName
real(kind=wp), intent(in) :: date1

TT as a 2-part Julian Date (Note 1)
real(kind=wp), intent(in) :: date2

TT as a 2-part Julian Date (Note 1)
real(kind=wp), intent(out) :: x

Celestial Intermediate Pole (Note 2)
real(kind=wp), intent(out) :: y

Celestial Intermediate Pole (Note 2)
real(kind=wp), intent(out) :: s

the CIO locator s (Note 2)

Calls

proc~~xys00b~~CallsGraph proc~xys00b XYS00B proc~pnm00b PNM00B proc~xys00b->proc~pnm00b proc~s00 S00 proc~xys00b->proc~s00 proc~bpn2xy BPN2XY proc~xys00b->proc~bpn2xy proc~pn00b PN00B proc~pnm00b->proc~pn00b proc~faom03 FAOM03 proc~s00->proc~faom03 proc~falp03 FALP03 proc~s00->proc~falp03 proc~fae03 FAE03 proc~s00->proc~fae03 proc~fal03 FAL03 proc~s00->proc~fal03 proc~faf03 FAF03 proc~s00->proc~faf03 proc~fad03 FAD03 proc~s00->proc~fad03 proc~fave03 FAVE03 proc~s00->proc~fave03 proc~fapa03 FAPA03 proc~s00->proc~fapa03 proc~nut00b NUT00B proc~pn00b->proc~nut00b proc~pn00 PN00 proc~pn00b->proc~pn00 proc~obl80 OBL80 proc~pn00->proc~obl80 proc~numat NUMAT proc~pn00->proc~numat proc~bp00 BP00 proc~pn00->proc~bp00 proc~rxr RXR proc~pn00->proc~rxr proc~pr00 PR00 proc~pn00->proc~pr00 proc~rx RX proc~numat->proc~rx proc~ir IR proc~numat->proc~ir proc~rz RZ proc~numat->proc~rz proc~bp00->proc~rxr proc~bp00->proc~pr00 proc~bp00->proc~rx proc~ry RY proc~bp00->proc~ry proc~bp00->proc~ir proc~bp00->proc~rz proc~bi00 BI00 proc~bp00->proc~bi00

Contents

Source Code

XYS00B

Source Code

    subroutine XYS00B ( date1, date2, x, y, s )

    implicit none

    real(wp),intent(in) :: date1 !! TT as a 2-part Julian Date (Note 1)
    real(wp),intent(in) :: date2 !! TT as a 2-part Julian Date (Note 1)
    real(wp),intent(out) :: x !! Celestial Intermediate Pole (Note 2)
    real(wp),intent(out) :: y !! Celestial Intermediate Pole (Note 2)
    real(wp),intent(out) :: s !! the CIO locator s (Note 2)

    real(wp) :: rbpn(3,3)

    !  Form the bias-precession-nutation matrix, IAU 2000A.
    call PNM00B ( date1, date2, rbpn )

    !  Extract X,Y.
    call BPN2XY ( rbpn, x, y )

    !  Obtain s.
    s = S00 ( date1, date2, x, y )

    end subroutine XYS00B