#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) 2013-2017, 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) 2013-2017, 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. ** */