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author | William Joye <wjoye@cfa.harvard.edu> | 2017-12-08 18:59:21 (GMT) |
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committer | William Joye <wjoye@cfa.harvard.edu> | 2017-12-08 18:59:21 (GMT) |
commit | 4432c8d7e1ccb371db03e13cdb5378fceaa5ad04 (patch) | |
tree | 52449d211eba99b24d2e4f6e66193f9511c60b59 /ast/erfa/s00b.c | |
parent | d8a2dbd825159e4a57ec0c6f4465f62be9e05111 (diff) | |
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upgrade AST
Diffstat (limited to 'ast/erfa/s00b.c')
-rw-r--r-- | ast/erfa/s00b.c | 152 |
1 files changed, 152 insertions, 0 deletions
diff --git a/ast/erfa/s00b.c b/ast/erfa/s00b.c new file mode 100644 index 0000000..370f95b --- /dev/null +++ b/ast/erfa/s00b.c @@ -0,0 +1,152 @@ +#include "erfa.h" + +double eraS00b(double date1, double date2) +/* +** - - - - - - - - +** e r a S 0 0 b +** - - - - - - - - +** +** The CIO locator s, positioning the Celestial Intermediate Origin on +** the equator of the Celestial Intermediate Pole, using the IAU 2000B +** precession-nutation model. +** +** Given: +** date1,date2 double TT as a 2-part Julian Date (Note 1) +** +** Returned (function value): +** double the CIO locator s in radians (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 CIO locator s is the difference between the right ascensions +** of the same point in two systems. The two systems are the GCRS +** and the CIP,CIO, and the point is the ascending node of the +** CIP equator. The CIO locator s remains a small fraction of +** 1 arcsecond throughout 1900-2100. +** +** 3) The series used to compute s is in fact for s+XY/2, where X and Y +** are the x and y components of the CIP unit vector; this series +** is more compact than a direct series for s would be. The present +** function uses the IAU 2000B truncated nutation model when +** predicting the CIP position. The function eraS00a uses instead +** the full IAU 2000A model, but with no significant increase in +** accuracy and at some cost in speed. +** +** Called: +** eraPnm00b classical NPB matrix, IAU 2000B +** eraBnp2xy extract CIP X,Y from the BPN matrix +** eraS00 the CIO locator s, given X,Y, IAU 2000A +** +** References: +** +** Capitaine, N., Chapront, J., Lambert, S. and Wallace, P., +** "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], x, y, s; + + +/* Bias-precession-nutation-matrix, IAU 2000B. */ + eraPnm00b(date1, date2, rbpn); + +/* Extract the CIP coordinates. */ + eraBpn2xy(rbpn, &x, &y); + +/* Compute the CIO locator s, given the CIP coordinates. */ + s = eraS00(date1, date2, x, y); + + return s; + +} +/*---------------------------------------------------------------------- +** +** +** 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. +** +*/ |