summaryrefslogtreecommitdiffstats
path: root/ast/erfa/ld.c
diff options
context:
space:
mode:
Diffstat (limited to 'ast/erfa/ld.c')
-rw-r--r--ast/erfa/ld.c161
1 files changed, 0 insertions, 161 deletions
diff --git a/ast/erfa/ld.c b/ast/erfa/ld.c
deleted file mode 100644
index c1569fd..0000000
--- a/ast/erfa/ld.c
+++ /dev/null
@@ -1,161 +0,0 @@
-#include "erfa.h"
-
-void eraLd(double bm, double p[3], double q[3], double e[3],
- double em, double dlim, double p1[3])
-/*
-** - - - - - -
-** e r a L d
-** - - - - - -
-**
-** Apply light deflection by a solar-system body, as part of
-** transforming coordinate direction into natural direction.
-**
-** Given:
-** bm double mass of the gravitating body (solar masses)
-** p double[3] direction from observer to source (unit vector)
-** q double[3] direction from body to source (unit vector)
-** e double[3] direction from body to observer (unit vector)
-** em double distance from body to observer (au)
-** dlim double deflection limiter (Note 4)
-**
-** Returned:
-** p1 double[3] observer to deflected source (unit vector)
-**
-** Notes:
-**
-** 1) The algorithm is based on Expr. (70) in Klioner (2003) and
-** Expr. (7.63) in the Explanatory Supplement (Urban & Seidelmann
-** 2013), with some rearrangement to minimize the effects of machine
-** precision.
-**
-** 2) The mass parameter bm can, as required, be adjusted in order to
-** allow for such effects as quadrupole field.
-**
-** 3) The barycentric position of the deflecting body should ideally
-** correspond to the time of closest approach of the light ray to
-** the body.
-**
-** 4) The deflection limiter parameter dlim is phi^2/2, where phi is
-** the angular separation (in radians) between source and body at
-** which limiting is applied. As phi shrinks below the chosen
-** threshold, the deflection is artificially reduced, reaching zero
-** for phi = 0.
-**
-** 5) The returned vector p1 is not normalized, but the consequential
-** departure from unit magnitude is always negligible.
-**
-** 6) The arguments p and p1 can be the same array.
-**
-** 7) To accumulate total light deflection taking into account the
-** contributions from several bodies, call the present function for
-** each body in succession, in decreasing order of distance from the
-** observer.
-**
-** 8) For efficiency, validation is omitted. The supplied vectors must
-** be of unit magnitude, and the deflection limiter non-zero and
-** positive.
-**
-** References:
-**
-** Urban, S. & Seidelmann, P. K. (eds), Explanatory Supplement to
-** the Astronomical Almanac, 3rd ed., University Science Books
-** (2013).
-**
-** Klioner, Sergei A., "A practical relativistic model for micro-
-** arcsecond astrometry in space", Astr. J. 125, 1580-1597 (2003).
-**
-** Called:
-** eraPdp scalar product of two p-vectors
-** eraPxp vector product of two p-vectors
-**
-** Copyright (C) 2013-2016, NumFOCUS Foundation.
-** Derived, with permission, from the SOFA library. See notes at end of file.
-*/
-{
- int i;
- double qpe[3], qdqpe, w, eq[3], peq[3];
-
-
-/* q . (q + e). */
- for (i = 0; i < 3; i++) {
- qpe[i] = q[i] + e[i];
- }
- qdqpe = eraPdp(q, qpe);
-
-/* 2 x G x bm / ( em x c^2 x ( q . (q + e) ) ). */
- w = bm * ERFA_SRS / em / ERFA_GMAX(qdqpe,dlim);
-
-/* p x (e x q). */
- eraPxp(e, q, eq);
- eraPxp(p, eq, peq);
-
-/* Apply the deflection. */
- for (i = 0; i < 3; i++) {
- p1[i] = p[i] + w*peq[i];
- }
-
-/* 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.
-**
-*/