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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) 2013-2014, 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) 2013-2014, 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.
+**
+*/