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author | William Joye <wjoye@cfa.harvard.edu> | 2017-12-08 18:57:06 (GMT) |
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committer | William Joye <wjoye@cfa.harvard.edu> | 2017-12-08 18:57:06 (GMT) |
commit | 90a861b642f765d5657ab827aedabe3920ff9333 (patch) | |
tree | 88b93d468ca1feed91ef2958f46f3f74f1418aac /ast/erfa/pvtob.c | |
parent | fba23129f50db253ed3fbbaa23d6e342bf86068e (diff) | |
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upgrade AST
Diffstat (limited to 'ast/erfa/pvtob.c')
-rw-r--r-- | ast/erfa/pvtob.c | 162 |
1 files changed, 0 insertions, 162 deletions
diff --git a/ast/erfa/pvtob.c b/ast/erfa/pvtob.c deleted file mode 100644 index 943a63c..0000000 --- a/ast/erfa/pvtob.c +++ /dev/null @@ -1,162 +0,0 @@ -#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. -** -*/ |