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Diffstat (limited to 'ast/erfa/ecm06.c')
| -rw-r--r-- | ast/erfa/ecm06.c | 144 |
1 files changed, 0 insertions, 144 deletions
diff --git a/ast/erfa/ecm06.c b/ast/erfa/ecm06.c deleted file mode 100644 index ce19ba2..0000000 --- a/ast/erfa/ecm06.c +++ /dev/null @@ -1,144 +0,0 @@ -#include "erfa.h" - -void eraEcm06(double date1, double date2, double rm[3][3]) -/* -** - - - - - - - - - -** e r a E c m 0 6 -** - - - - - - - - - -** -** ICRS equatorial to ecliptic rotation matrix, IAU 2006. -** -** Given: -** date1,date2 double TT as a 2-part Julian date (Note 1) -** -** Returned: -** rm double[3][3] ICRS to ecliptic rotation matrix -** -** 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. -** -** 1) The matrix is in the sense -** -** E_ep = rm x P_ICRS, -** -** where P_ICRS is a vector with respect to ICRS right ascension -** and declination axes and E_ep is the same vector with respect to -** the (inertial) ecliptic and equinox of date. -** -** 2) P_ICRS is a free vector, merely a direction, typically of unit -** magnitude, and not bound to any particular spatial origin, such -** as the Earth, Sun or SSB. No assumptions are made about whether -** it represents starlight and embodies astrometric effects such as -** parallax or aberration. The transformation is approximately that -** between mean J2000.0 right ascension and declination and ecliptic -** longitude and latitude, with only frame bias (always less than -** 25 mas) to disturb this classical picture. -** -** Called: -** eraObl06 mean obliquity, IAU 2006 -** eraPmat06 PB matrix, IAU 2006 -** eraIr initialize r-matrix to identity -** eraRx rotate around X-axis -** eraRxr product of two r-matrices -** -** Copyright (C) 2013-2016, NumFOCUS Foundation. -** Derived, with permission, from the SOFA library. See notes at end of file. -*/ -{ - double ob, bp[3][3], e[3][3]; - - -/* Obliquity, IAU 2006. */ - ob = eraObl06(date1, date2); - -/* Precession-bias matrix, IAU 2006. */ - eraPmat06(date1, date2, bp); - -/* Equatorial of date to ecliptic matrix. */ - eraIr(e); - eraRx(ob, e); - -/* ICRS to ecliptic coordinates rotation matrix, IAU 2006. */ - eraRxr(e, bp, rm); - -} -/*---------------------------------------------------------------------- -** -** -** 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. -** -*/ |