summaryrefslogtreecommitdiffstats
path: root/ast/erfa/c2t00b.c
diff options
context:
space:
mode:
authorWilliam Joye <wjoye@cfa.harvard.edu>2018-01-09 19:06:17 (GMT)
committerWilliam Joye <wjoye@cfa.harvard.edu>2018-01-09 19:06:17 (GMT)
commitd64cf9c0bd23e752867b149be636d1bbd4501cf4 (patch)
treeec600c696fe3dbf15f166d22a95c47a1c0867509 /ast/erfa/c2t00b.c
parent62d555c8f989ab6eb026387cbf52bb46ebb2dfea (diff)
downloadblt-d64cf9c0bd23e752867b149be636d1bbd4501cf4.zip
blt-d64cf9c0bd23e752867b149be636d1bbd4501cf4.tar.gz
blt-d64cf9c0bd23e752867b149be636d1bbd4501cf4.tar.bz2
update ast 8.6.2
Diffstat (limited to 'ast/erfa/c2t00b.c')
-rw-r--r--ast/erfa/c2t00b.c159
1 files changed, 0 insertions, 159 deletions
diff --git a/ast/erfa/c2t00b.c b/ast/erfa/c2t00b.c
deleted file mode 100644
index fe19504..0000000
--- a/ast/erfa/c2t00b.c
+++ /dev/null
@@ -1,159 +0,0 @@
-#include "erfa.h"
-
-void eraC2t00b(double tta, double ttb, double uta, double utb,
- double xp, double yp, double rc2t[3][3])
-/*
-** - - - - - - - - - -
-** e r a C 2 t 0 0 b
-** - - - - - - - - - -
-**
-** Form the celestial to terrestrial matrix given the date, the UT1 and
-** the polar motion, using the IAU 2000B nutation model.
-**
-** Given:
-** tta,ttb double TT as a 2-part Julian Date (Note 1)
-** uta,utb double UT1 as a 2-part Julian Date (Note 1)
-** xp,yp double coordinates of the pole (radians, Note 2)
-**
-** Returned:
-** rc2t double[3][3] celestial-to-terrestrial matrix (Note 3)
-**
-** Notes:
-**
-** 1) The TT and UT1 dates tta+ttb and uta+utb are Julian Dates,
-** apportioned in any convenient way between the arguments uta and
-** utb. For example, JD(UT1)=2450123.7 could be expressed in any of
-** these ways, among others:
-**
-** uta utb
-**
-** 2450123.7 0.0 (JD method)
-** 2451545.0 -1421.3 (J2000 method)
-** 2400000.5 50123.2 (MJD method)
-** 2450123.5 0.2 (date & time method)
-**
-** The JD method is the most natural and convenient to use in
-** cases where the loss of several decimal digits of resolution is
-** acceptable. The J2000 and MJD methods are good compromises
-** between resolution and convenience. In the case of uta,utb, the
-** date & time method is best matched to the Earth rotation angle
-** algorithm used: maximum precision is delivered when the uta
-** argument is for 0hrs UT1 on the day in question and the utb
-** argument lies in the range 0 to 1, or vice versa.
-**
-** 2) The arguments xp and yp are the coordinates (in radians) of the
-** Celestial Intermediate Pole with respect to the International
-** Terrestrial Reference System (see IERS Conventions 2003),
-** measured along the meridians to 0 and 90 deg west respectively.
-**
-** 3) The matrix rc2t transforms from celestial to terrestrial
-** coordinates:
-**
-** [TRS] = RPOM * R_3(ERA) * RC2I * [CRS]
-**
-** = rc2t * [CRS]
-**
-** where [CRS] is a vector in the Geocentric Celestial Reference
-** System and [TRS] is a vector in the International Terrestrial
-** Reference System (see IERS Conventions 2003), RC2I is the
-** celestial-to-intermediate matrix, ERA is the Earth rotation
-** angle and RPOM is the polar motion matrix.
-**
-** 4) The present function is faster, but slightly less accurate (about
-** 1 mas), than the eraC2t00a function.
-**
-** Called:
-** eraC2i00b celestial-to-intermediate matrix, IAU 2000B
-** eraEra00 Earth rotation angle, IAU 2000
-** eraPom00 polar motion matrix
-** eraC2tcio form CIO-based celestial-to-terrestrial matrix
-**
-** Reference:
-**
-** McCarthy, D. D., Petit, G. (eds.), IERS Conventions (2003),
-** IERS Technical Note No. 32, BKG (2004)
-**
-** Copyright (C) 2013-2016, NumFOCUS Foundation.
-** Derived, with permission, from the SOFA library. See notes at end of file.
-*/
-{
- double rc2i[3][3], era, rpom[3][3];
-
-
-/* Form the celestial-to-intermediate matrix for this TT (IAU 2000B). */
- eraC2i00b(tta, ttb, rc2i);
-
-/* Predict the Earth rotation angle for this UT1. */
- era = eraEra00(uta, utb);
-
-/* Form the polar motion matrix (neglecting s'). */
- eraPom00(xp, yp, 0.0, rpom);
-
-/* Combine to form the celestial-to-terrestrial matrix. */
- eraC2tcio(rc2i, era, rpom, rc2t);
-
- return;
-
-}
-/*----------------------------------------------------------------------
-**
-**
-** 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.
-**
-*/