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-#include "erfa.h"
-
-void eraPvtob(double elong, double phi, double hm,
- double xp, double yp, double sp, double theta,
- double pv[2][3])
-/*
-** - - - - - - - - -
-** e r a P v t o b
-** - - - - - - - - -
-**
-** Position and velocity of a terrestrial observing station.
-**
-** Given:
-** elong double longitude (radians, east +ve, Note 1)
-** phi double latitude (geodetic, radians, Note 1)
-** hm double height above ref. ellipsoid (geodetic, m)
-** xp,yp double coordinates of the pole (radians, Note 2)
-** sp double the TIO locator s' (radians, Note 2)
-** theta double Earth rotation angle (radians, Note 3)
-**
-** Returned:
-** pv double[2][3] position/velocity vector (m, m/s, CIRS)
-**
-** Notes:
-**
-** 1) The terrestrial coordinates are with respect to the ERFA_WGS84
-** reference ellipsoid.
-**
-** 2) xp and yp are the coordinates (in radians) of the Celestial
-** Intermediate Pole with respect to the International Terrestrial
-** Reference System (see IERS Conventions), measured along the
-** meridians 0 and 90 deg west respectively. sp is the TIO locator
-** s', in radians, which positions the Terrestrial Intermediate
-** Origin on the equator. For many applications, xp, yp and
-** (especially) sp can be set to zero.
-**
-** 3) If theta is Greenwich apparent sidereal time instead of Earth
-** rotation angle, the result is with respect to the true equator
-** and equinox of date, i.e. with the x-axis at the equinox rather
-** than the celestial intermediate origin.
-**
-** 4) The velocity units are meters per UT1 second, not per SI second.
-** This is unlikely to have any practical consequences in the modern
-** era.
-**
-** 5) No validation is performed on the arguments. Error cases that
-** could lead to arithmetic exceptions are trapped by the eraGd2gc
-** function, and the result set to zeros.
-**
-** References:
-**
-** McCarthy, D. D., Petit, G. (eds.), IERS Conventions (2003),
-** IERS Technical Note No. 32, BKG (2004)
-**
-** Urban, S. & Seidelmann, P. K. (eds), Explanatory Supplement to
-** the Astronomical Almanac, 3rd ed., University Science Books
-** (2013), Section 7.4.3.3.
-**
-** Called:
-** eraGd2gc geodetic to geocentric transformation
-** eraPom00 polar motion matrix
-** eraTrxp product of transpose of r-matrix and p-vector
-**
-** Copyright (C) 2013-2016, NumFOCUS Foundation.
-** Derived, with permission, from the SOFA library. See notes at end of file.
-*/
-{
-/* Earth rotation rate in radians per UT1 second */
- const double OM = 1.00273781191135448 * ERFA_D2PI / ERFA_DAYSEC;
-
- double xyzm[3], rpm[3][3], xyz[3], x, y, z, s, c;
-
-
-/* Geodetic to geocentric transformation (ERFA_WGS84). */
- (void) eraGd2gc(1, elong, phi, hm, xyzm);
-
-/* Polar motion and TIO position. */
- eraPom00(xp, yp, sp, rpm);
- eraTrxp(rpm, xyzm, xyz);
- x = xyz[0];
- y = xyz[1];
- z = xyz[2];
-
-/* Functions of ERA. */
- s = sin(theta);
- c = cos(theta);
-
-/* Position. */
- pv[0][0] = c*x - s*y;
- pv[0][1] = s*x + c*y;
- pv[0][2] = z;
-
-/* Velocity. */
- pv[1][0] = OM * ( -s*x - c*y );
- pv[1][1] = OM * ( c*x - s*y );
- pv[1][2] = 0.0;
-
-/* Finished. */
-
-}
-/*----------------------------------------------------------------------
-**
-**
-** Copyright (C) 2013-2016, NumFOCUS Foundation.
-** All rights reserved.
-**
-** This library is derived, with permission, from the International
-** Astronomical Union's "Standards of Fundamental Astronomy" library,
-** available from http://www.iausofa.org.
-**
-** The ERFA version is intended to retain identical functionality to
-** the SOFA library, but made distinct through different function and
-** file names, as set out in the SOFA license conditions. The SOFA
-** original has a role as a reference standard for the IAU and IERS,
-** and consequently redistribution is permitted only in its unaltered
-** state. The ERFA version is not subject to this restriction and
-** therefore can be included in distributions which do not support the
-** concept of "read only" software.
-**
-** Although the intent is to replicate the SOFA API (other than
-** replacement of prefix names) and results (with the exception of
-** bugs; any that are discovered will be fixed), SOFA is not
-** responsible for any errors found in this version of the library.
-**
-** If you wish to acknowledge the SOFA heritage, please acknowledge
-** that you are using a library derived from SOFA, rather than SOFA
-** itself.
-**
-**
-** TERMS AND CONDITIONS
-**
-** Redistribution and use in source and binary forms, with or without
-** modification, are permitted provided that the following conditions
-** are met:
-**
-** 1 Redistributions of source code must retain the above copyright
-** notice, this list of conditions and the following disclaimer.
-**
-** 2 Redistributions in binary form must reproduce the above copyright
-** notice, this list of conditions and the following disclaimer in
-** the documentation and/or other materials provided with the
-** distribution.
-**
-** 3 Neither the name of the Standards Of Fundamental Astronomy Board,
-** the International Astronomical Union nor the names of its
-** contributors may be used to endorse or promote products derived
-** from this software without specific prior written permission.
-**
-** THIS SOFTWARE IS PROVIDED BY THE COPYRIGHT HOLDERS AND CONTRIBUTORS
-** "AS IS" AND ANY EXPRESS OR IMPLIED WARRANTIES, INCLUDING, BUT NOT
-** LIMITED TO, THE IMPLIED WARRANTIES OF MERCHANTABILITY AND FITNESS
-** FOR A PARTICULAR PURPOSE ARE DISCLAIMED. IN NO EVENT SHALL THE
-** COPYRIGHT HOLDER OR CONTRIBUTORS BE LIABLE FOR ANY DIRECT, INDIRECT,
-** INCIDENTAL, SPECIAL, EXEMPLARY, OR CONSEQUENTIAL DAMAGES (INCLUDING,
-** BUT NOT LIMITED TO, PROCUREMENT OF SUBSTITUTE GOODS OR SERVICES;
-** LOSS OF USE, DATA, OR PROFITS; OR BUSINESS INTERRUPTION) HOWEVER
-** CAUSED AND ON ANY THEORY OF LIABILITY, WHETHER IN CONTRACT, STRICT
-** LIABILITY, OR TORT (INCLUDING NEGLIGENCE OR OTHERWISE) ARISING IN
-** ANY WAY OUT OF THE USE OF THIS SOFTWARE, EVEN IF ADVISED OF THE
-** POSSIBILITY OF SUCH DAMAGE.
-**
-*/