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#include "erfa.h" |
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void eraLtecm(double epj, double rm[3][3]) |
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/* |
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** - - - - - - - - - |
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** e r a L t e c m |
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** - - - - - - - - - |
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** |
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** ICRS equatorial to ecliptic rotation matrix, long-term. |
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** |
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** Given: |
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** epj double Julian epoch (TT) |
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** |
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** Returned: |
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** rm double[3][3] ICRS to ecliptic rotation matrix |
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** |
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** Notes: |
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** |
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** 1) The matrix is in the sense |
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** |
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** E_ep = rm x P_ICRS, |
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** |
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** where P_ICRS is a vector with respect to ICRS right ascension |
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** and declination axes and E_ep is the same vector with respect to |
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** the (inertial) ecliptic and equinox of epoch epj. |
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** |
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** 2) P_ICRS is a free vector, merely a direction, typically of unit |
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** magnitude, and not bound to any particular spatial origin, such |
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** as the Earth, Sun or SSB. No assumptions are made about whether |
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** it represents starlight and embodies astrometric effects such as |
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** parallax or aberration. The transformation is approximately that |
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** between mean J2000.0 right ascension and declination and ecliptic |
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** longitude and latitude, with only frame bias (always less than |
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** 25 mas) to disturb this classical picture. |
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** |
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** 3) The Vondrak et al. (2011, 2012) 400 millennia precession model |
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** agrees with the IAU 2006 precession at J2000.0 and stays within |
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** 100 microarcseconds during the 20th and 21st centuries. It is |
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** accurate to a few arcseconds throughout the historical period, |
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** worsening to a few tenths of a degree at the end of the |
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** +/- 200,000 year time span. |
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** |
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** Called: |
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** eraLtpequ equator pole, long term |
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** eraLtpecl ecliptic pole, long term |
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** eraPxp vector product |
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** eraPn normalize vector |
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** |
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** References: |
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** |
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** Vondrak, J., Capitaine, N. and Wallace, P., 2011, New precession |
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** expressions, valid for long time intervals, Astron.Astrophys. 534, |
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** A22 |
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** |
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** Vondrak, J., Capitaine, N. and Wallace, P., 2012, New precession |
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** expressions, valid for long time intervals (Corrigendum), |
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** Astron.Astrophys. 541, C1 |
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** |
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** Copyright (C) 2013-2019, NumFOCUS Foundation. |
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** Derived, with permission, from the SOFA library. See notes at end of file. |
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*/ |
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{ |
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/* Frame bias (IERS Conventions 2010, Eqs. 5.21 and 5.33) */ |
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const double dx = -0.016617 * ERFA_DAS2R, |
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de = -0.0068192 * ERFA_DAS2R, |
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dr = -0.0146 * ERFA_DAS2R; |
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double p[3], z[3], w[3], s, x[3], y[3]; |
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/* Equator pole. */ |
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0
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eraLtpequ(epj, p); |
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/* Ecliptic pole (bottom row of equatorial to ecliptic matrix). */ |
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eraLtpecl(epj, z); |
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/* Equinox (top row of matrix). */ |
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eraPxp(p, z, w); |
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eraPn(w, &s, x); |
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/* Middle row of matrix. */ |
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eraPxp(z, x, y); |
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/* Combine with frame bias. */ |
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0
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rm[0][0] = x[0] - x[1]*dr + x[2]*dx; |
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rm[0][1] = x[0]*dr + x[1] + x[2]*de; |
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rm[0][2] = - x[0]*dx - x[1]*de + x[2]; |
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rm[1][0] = y[0] - y[1]*dr + y[2]*dx; |
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rm[1][1] = y[0]*dr + y[1] + y[2]*de; |
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rm[1][2] = - y[0]*dx - y[1]*de + y[2]; |
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rm[2][0] = z[0] - z[1]*dr + z[2]*dx; |
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rm[2][1] = z[0]*dr + z[1] + z[2]*de; |
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rm[2][2] = - z[0]*dx - z[1]*de + z[2]; |
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} |
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/*---------------------------------------------------------------------- |
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** |
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** |
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** Copyright (C) 2013-2019, NumFOCUS Foundation. |
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** All rights reserved. |
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** |
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** This library is derived, with permission, from the International |
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** Astronomical Union's "Standards of Fundamental Astronomy" library, |
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** available from http://www.iausofa.org. |
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** |
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** The ERFA version is intended to retain identical functionality to |
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** the SOFA library, but made distinct through different function and |
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** file names, as set out in the SOFA license conditions. The SOFA |
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** original has a role as a reference standard for the IAU and IERS, |
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** and consequently redistribution is permitted only in its unaltered |
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** state. The ERFA version is not subject to this restriction and |
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** therefore can be included in distributions which do not support the |
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** concept of "read only" software. |
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** |
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** Although the intent is to replicate the SOFA API (other than |
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** replacement of prefix names) and results (with the exception of |
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** bugs; any that are discovered will be fixed), SOFA is not |
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** responsible for any errors found in this version of the library. |
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** |
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** If you wish to acknowledge the SOFA heritage, please acknowledge |
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** that you are using a library derived from SOFA, rather than SOFA |
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** itself. |
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** |
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** |
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** TERMS AND CONDITIONS |
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** |
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** Redistribution and use in source and binary forms, with or without |
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** modification, are permitted provided that the following conditions |
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** are met: |
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** |
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** 1 Redistributions of source code must retain the above copyright |
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** notice, this list of conditions and the following disclaimer. |
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** |
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** 2 Redistributions in binary form must reproduce the above copyright |
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** notice, this list of conditions and the following disclaimer in |
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** the documentation and/or other materials provided with the |
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** distribution. |
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** |
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** 3 Neither the name of the Standards Of Fundamental Astronomy Board, |
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** the International Astronomical Union nor the names of its |
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** contributors may be used to endorse or promote products derived |
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** from this software without specific prior written permission. |
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** |
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** THIS SOFTWARE IS PROVIDED BY THE COPYRIGHT HOLDERS AND CONTRIBUTORS |
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** "AS IS" AND ANY EXPRESS OR IMPLIED WARRANTIES, INCLUDING, BUT NOT |
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** LIMITED TO, THE IMPLIED WARRANTIES OF MERCHANTABILITY AND FITNESS |
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** FOR A PARTICULAR PURPOSE ARE DISCLAIMED. IN NO EVENT SHALL THE |
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** COPYRIGHT HOLDER OR CONTRIBUTORS BE LIABLE FOR ANY DIRECT, INDIRECT, |
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** INCIDENTAL, SPECIAL, EXEMPLARY, OR CONSEQUENTIAL DAMAGES (INCLUDING, |
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** BUT NOT LIMITED TO, PROCUREMENT OF SUBSTITUTE GOODS OR SERVICES; |
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** LOSS OF USE, DATA, OR PROFITS; OR BUSINESS INTERRUPTION) HOWEVER |
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** CAUSED AND ON ANY THEORY OF LIABILITY, WHETHER IN CONTRACT, STRICT |
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** LIABILITY, OR TORT (INCLUDING NEGLIGENCE OR OTHERWISE) ARISING IN |
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** ANY WAY OUT OF THE USE OF THIS SOFTWARE, EVEN IF ADVISED OF THE |
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** POSSIBILITY OF SUCH DAMAGE. |
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** |
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*/ |