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authorWilliam Joye <wjoye@cfa.harvard.edu>2018-01-09 19:26:44 (GMT)
committerWilliam Joye <wjoye@cfa.harvard.edu>2018-01-09 19:26:44 (GMT)
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update ast 8.6.2
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-#include "erfa.h"
-
-void eraC2i00a(double date1, double date2, double rc2i[3][3])
-/*
-** - - - - - - - - - -
-** e r a C 2 i 0 0 a
-** - - - - - - - - - -
-**
-** Form the celestial-to-intermediate matrix for a given date using the
-** IAU 2000A precession-nutation model.
-**
-** Given:
-** date1,date2 double TT as a 2-part Julian Date (Note 1)
-**
-** Returned:
-** rc2i double[3][3] celestial-to-intermediate matrix (Note 2)
-**
-** Notes:
-**
-** 1) The TT date date1+date2 is a Julian Date, apportioned in any
-** convenient way between the two arguments. For example,
-** JD(TT)=2450123.7 could be expressed in any of these ways,
-** among others:
-**
-** date1 date2
-**
-** 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 method is best matched to the way
-** the argument is handled internally and will deliver the
-** optimum resolution. The MJD method and the date & time methods
-** are both good compromises between resolution and convenience.
-**
-** 2) The matrix rc2i is the first stage in the transformation 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), ERA is the Earth
-** Rotation Angle and RPOM is the polar motion matrix.
-**
-** 3) A faster, but slightly less accurate result (about 1 mas), can be
-** obtained by using instead the eraC2i00b function.
-**
-** Called:
-** eraPnm00a classical NPB matrix, IAU 2000A
-** eraC2ibpn celestial-to-intermediate matrix, given NPB matrix
-**
-** References:
-**
-** "Expressions for the Celestial Intermediate Pole and Celestial
-** Ephemeris Origin consistent with the IAU 2000A precession-
-** nutation model", Astron.Astrophys. 400, 1145-1154
-** (2003)
-**
-** n.b. The celestial ephemeris origin (CEO) was renamed "celestial
-** intermediate origin" (CIO) by IAU 2006 Resolution 2.
-**
-** 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 rbpn[3][3];
-
-
-/* Obtain the celestial-to-true matrix (IAU 2000A). */
- eraPnm00a(date1, date2, rbpn);
-
-/* Form the celestial-to-intermediate matrix. */
- eraC2ibpn(date1, date2, rbpn, rc2i);
-
- 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.
-**
-*/