| line | stmt | bran | cond | sub | pod | time | code | 
| 1 |  |  |  |  |  |  | #include "erfa.h" | 
| 2 |  |  |  |  |  |  |  | 
| 3 | 0 |  |  |  |  |  | void eraLtecm(double epj, double rm[3][3]) | 
| 4 |  |  |  |  |  |  | /* | 
| 5 |  |  |  |  |  |  | **  - - - - - - - - - | 
| 6 |  |  |  |  |  |  | **   e r a L t e c m | 
| 7 |  |  |  |  |  |  | **  - - - - - - - - - | 
| 8 |  |  |  |  |  |  | ** | 
| 9 |  |  |  |  |  |  | **  ICRS equatorial to ecliptic rotation matrix, long-term. | 
| 10 |  |  |  |  |  |  | ** | 
| 11 |  |  |  |  |  |  | **  Given: | 
| 12 |  |  |  |  |  |  | **     epj     double         Julian epoch (TT) | 
| 13 |  |  |  |  |  |  | ** | 
| 14 |  |  |  |  |  |  | **  Returned: | 
| 15 |  |  |  |  |  |  | **     rm      double[3][3]   ICRS to ecliptic rotation matrix | 
| 16 |  |  |  |  |  |  | ** | 
| 17 |  |  |  |  |  |  | **  Notes: | 
| 18 |  |  |  |  |  |  | ** | 
| 19 |  |  |  |  |  |  | **  1) The matrix is in the sense | 
| 20 |  |  |  |  |  |  | ** | 
| 21 |  |  |  |  |  |  | **        E_ep = rm x P_ICRS, | 
| 22 |  |  |  |  |  |  | ** | 
| 23 |  |  |  |  |  |  | **     where P_ICRS is a vector with respect to ICRS right ascension | 
| 24 |  |  |  |  |  |  | **     and declination axes and E_ep is the same vector with respect to | 
| 25 |  |  |  |  |  |  | **     the (inertial) ecliptic and equinox of epoch epj. | 
| 26 |  |  |  |  |  |  | ** | 
| 27 |  |  |  |  |  |  | **  2) P_ICRS is a free vector, merely a direction, typically of unit | 
| 28 |  |  |  |  |  |  | **     magnitude, and not bound to any particular spatial origin, such | 
| 29 |  |  |  |  |  |  | **     as the Earth, Sun or SSB.  No assumptions are made about whether | 
| 30 |  |  |  |  |  |  | **     it represents starlight and embodies astrometric effects such as | 
| 31 |  |  |  |  |  |  | **     parallax or aberration.  The transformation is approximately that | 
| 32 |  |  |  |  |  |  | **     between mean J2000.0 right ascension and declination and ecliptic | 
| 33 |  |  |  |  |  |  | **     longitude and latitude, with only frame bias (always less than | 
| 34 |  |  |  |  |  |  | **     25 mas) to disturb this classical picture. | 
| 35 |  |  |  |  |  |  | ** | 
| 36 |  |  |  |  |  |  | **  3) The Vondrak et al. (2011, 2012) 400 millennia precession model | 
| 37 |  |  |  |  |  |  | **     agrees with the IAU 2006 precession at J2000.0 and stays within | 
| 38 |  |  |  |  |  |  | **     100 microarcseconds during the 20th and 21st centuries.  It is | 
| 39 |  |  |  |  |  |  | **     accurate to a few arcseconds throughout the historical period, | 
| 40 |  |  |  |  |  |  | **     worsening to a few tenths of a degree at the end of the | 
| 41 |  |  |  |  |  |  | **     +/- 200,000 year time span. | 
| 42 |  |  |  |  |  |  | ** | 
| 43 |  |  |  |  |  |  | **  Called: | 
| 44 |  |  |  |  |  |  | **     eraLtpequ    equator pole, long term | 
| 45 |  |  |  |  |  |  | **     eraLtpecl    ecliptic pole, long term | 
| 46 |  |  |  |  |  |  | **     eraPxp       vector product | 
| 47 |  |  |  |  |  |  | **     eraPn        normalize vector | 
| 48 |  |  |  |  |  |  | ** | 
| 49 |  |  |  |  |  |  | **  References: | 
| 50 |  |  |  |  |  |  | ** | 
| 51 |  |  |  |  |  |  | **    Vondrak, J., Capitaine, N. and Wallace, P., 2011, New precession | 
| 52 |  |  |  |  |  |  | **    expressions, valid for long time intervals, Astron.Astrophys. 534, | 
| 53 |  |  |  |  |  |  | **    A22 | 
| 54 |  |  |  |  |  |  | ** | 
| 55 |  |  |  |  |  |  | **    Vondrak, J., Capitaine, N. and Wallace, P., 2012, New precession | 
| 56 |  |  |  |  |  |  | **    expressions, valid for long time intervals (Corrigendum), | 
| 57 |  |  |  |  |  |  | **    Astron.Astrophys. 541, C1 | 
| 58 |  |  |  |  |  |  | ** | 
| 59 |  |  |  |  |  |  | **  Copyright (C) 2013-2019, NumFOCUS Foundation. | 
| 60 |  |  |  |  |  |  | **  Derived, with permission, from the SOFA library.  See notes at end of file. | 
| 61 |  |  |  |  |  |  | */ | 
| 62 |  |  |  |  |  |  | { | 
| 63 |  |  |  |  |  |  | /* Frame bias (IERS Conventions 2010, Eqs. 5.21 and 5.33) */ | 
| 64 |  |  |  |  |  |  | const double dx = -0.016617 * ERFA_DAS2R, | 
| 65 |  |  |  |  |  |  | de = -0.0068192 * ERFA_DAS2R, | 
| 66 |  |  |  |  |  |  | dr = -0.0146 * ERFA_DAS2R; | 
| 67 |  |  |  |  |  |  |  | 
| 68 |  |  |  |  |  |  | double p[3], z[3], w[3], s, x[3], y[3]; | 
| 69 |  |  |  |  |  |  |  | 
| 70 |  |  |  |  |  |  |  | 
| 71 |  |  |  |  |  |  | /* Equator pole. */ | 
| 72 | 0 |  |  |  |  |  | eraLtpequ(epj, p); | 
| 73 |  |  |  |  |  |  |  | 
| 74 |  |  |  |  |  |  | /* Ecliptic pole (bottom row of equatorial to ecliptic matrix). */ | 
| 75 | 0 |  |  |  |  |  | eraLtpecl(epj, z); | 
| 76 |  |  |  |  |  |  |  | 
| 77 |  |  |  |  |  |  | /* Equinox (top row of matrix). */ | 
| 78 | 0 |  |  |  |  |  | eraPxp(p, z, w); | 
| 79 | 0 |  |  |  |  |  | eraPn(w, &s, x); | 
| 80 |  |  |  |  |  |  |  | 
| 81 |  |  |  |  |  |  | /* Middle row of matrix. */ | 
| 82 | 0 |  |  |  |  |  | eraPxp(z, x, y); | 
| 83 |  |  |  |  |  |  |  | 
| 84 |  |  |  |  |  |  | /* Combine with frame bias. */ | 
| 85 | 0 |  |  |  |  |  | rm[0][0] =   x[0]    - x[1]*dr + x[2]*dx; | 
| 86 | 0 |  |  |  |  |  | rm[0][1] =   x[0]*dr + x[1]    + x[2]*de; | 
| 87 | 0 |  |  |  |  |  | rm[0][2] = - x[0]*dx - x[1]*de + x[2]; | 
| 88 | 0 |  |  |  |  |  | rm[1][0] =   y[0]    - y[1]*dr + y[2]*dx; | 
| 89 | 0 |  |  |  |  |  | rm[1][1] =   y[0]*dr + y[1]    + y[2]*de; | 
| 90 | 0 |  |  |  |  |  | rm[1][2] = - y[0]*dx - y[1]*de + y[2]; | 
| 91 | 0 |  |  |  |  |  | rm[2][0] =   z[0]    - z[1]*dr + z[2]*dx; | 
| 92 | 0 |  |  |  |  |  | rm[2][1] =   z[0]*dr + z[1]    + z[2]*de; | 
| 93 | 0 |  |  |  |  |  | rm[2][2] = - z[0]*dx - z[1]*de + z[2]; | 
| 94 |  |  |  |  |  |  |  | 
| 95 | 0 |  |  |  |  |  | } | 
| 96 |  |  |  |  |  |  | /*---------------------------------------------------------------------- | 
| 97 |  |  |  |  |  |  | ** | 
| 98 |  |  |  |  |  |  | ** | 
| 99 |  |  |  |  |  |  | **  Copyright (C) 2013-2019, NumFOCUS Foundation. | 
| 100 |  |  |  |  |  |  | **  All rights reserved. | 
| 101 |  |  |  |  |  |  | ** | 
| 102 |  |  |  |  |  |  | **  This library is derived, with permission, from the International | 
| 103 |  |  |  |  |  |  | **  Astronomical Union's "Standards of Fundamental Astronomy" library, | 
| 104 |  |  |  |  |  |  | **  available from http://www.iausofa.org. | 
| 105 |  |  |  |  |  |  | ** | 
| 106 |  |  |  |  |  |  | **  The ERFA version is intended to retain identical functionality to | 
| 107 |  |  |  |  |  |  | **  the SOFA library, but made distinct through different function and | 
| 108 |  |  |  |  |  |  | **  file names, as set out in the SOFA license conditions.  The SOFA | 
| 109 |  |  |  |  |  |  | **  original has a role as a reference standard for the IAU and IERS, | 
| 110 |  |  |  |  |  |  | **  and consequently redistribution is permitted only in its unaltered | 
| 111 |  |  |  |  |  |  | **  state.  The ERFA version is not subject to this restriction and | 
| 112 |  |  |  |  |  |  | **  therefore can be included in distributions which do not support the | 
| 113 |  |  |  |  |  |  | **  concept of "read only" software. | 
| 114 |  |  |  |  |  |  | ** | 
| 115 |  |  |  |  |  |  | **  Although the intent is to replicate the SOFA API (other than | 
| 116 |  |  |  |  |  |  | **  replacement of prefix names) and results (with the exception of | 
| 117 |  |  |  |  |  |  | **  bugs;  any that are discovered will be fixed), SOFA is not | 
| 118 |  |  |  |  |  |  | **  responsible for any errors found in this version of the library. | 
| 119 |  |  |  |  |  |  | ** | 
| 120 |  |  |  |  |  |  | **  If you wish to acknowledge the SOFA heritage, please acknowledge | 
| 121 |  |  |  |  |  |  | **  that you are using a library derived from SOFA, rather than SOFA | 
| 122 |  |  |  |  |  |  | **  itself. | 
| 123 |  |  |  |  |  |  | ** | 
| 124 |  |  |  |  |  |  | ** | 
| 125 |  |  |  |  |  |  | **  TERMS AND CONDITIONS | 
| 126 |  |  |  |  |  |  | ** | 
| 127 |  |  |  |  |  |  | **  Redistribution and use in source and binary forms, with or without | 
| 128 |  |  |  |  |  |  | **  modification, are permitted provided that the following conditions | 
| 129 |  |  |  |  |  |  | **  are met: | 
| 130 |  |  |  |  |  |  | ** | 
| 131 |  |  |  |  |  |  | **  1 Redistributions of source code must retain the above copyright | 
| 132 |  |  |  |  |  |  | **    notice, this list of conditions and the following disclaimer. | 
| 133 |  |  |  |  |  |  | ** | 
| 134 |  |  |  |  |  |  | **  2 Redistributions in binary form must reproduce the above copyright | 
| 135 |  |  |  |  |  |  | **    notice, this list of conditions and the following disclaimer in | 
| 136 |  |  |  |  |  |  | **    the documentation and/or other materials provided with the | 
| 137 |  |  |  |  |  |  | **    distribution. | 
| 138 |  |  |  |  |  |  | ** | 
| 139 |  |  |  |  |  |  | **  3 Neither the name of the Standards Of Fundamental Astronomy Board, | 
| 140 |  |  |  |  |  |  | **    the International Astronomical Union nor the names of its | 
| 141 |  |  |  |  |  |  | **    contributors may be used to endorse or promote products derived | 
| 142 |  |  |  |  |  |  | **    from this software without specific prior written permission. | 
| 143 |  |  |  |  |  |  | ** | 
| 144 |  |  |  |  |  |  | **  THIS SOFTWARE IS PROVIDED BY THE COPYRIGHT HOLDERS AND CONTRIBUTORS | 
| 145 |  |  |  |  |  |  | **  "AS IS" AND ANY EXPRESS OR IMPLIED WARRANTIES, INCLUDING, BUT NOT | 
| 146 |  |  |  |  |  |  | **  LIMITED TO, THE IMPLIED WARRANTIES OF MERCHANTABILITY AND FITNESS | 
| 147 |  |  |  |  |  |  | **  FOR A PARTICULAR PURPOSE ARE DISCLAIMED.  IN NO EVENT SHALL THE | 
| 148 |  |  |  |  |  |  | **  COPYRIGHT HOLDER OR CONTRIBUTORS BE LIABLE FOR ANY DIRECT, INDIRECT, | 
| 149 |  |  |  |  |  |  | **  INCIDENTAL, SPECIAL, EXEMPLARY, OR CONSEQUENTIAL DAMAGES (INCLUDING, | 
| 150 |  |  |  |  |  |  | **  BUT NOT LIMITED TO, PROCUREMENT OF SUBSTITUTE GOODS OR SERVICES; | 
| 151 |  |  |  |  |  |  | **  LOSS OF USE, DATA, OR PROFITS; OR BUSINESS INTERRUPTION) HOWEVER | 
| 152 |  |  |  |  |  |  | **  CAUSED AND ON ANY THEORY OF LIABILITY, WHETHER IN CONTRACT, STRICT | 
| 153 |  |  |  |  |  |  | **  LIABILITY, OR TORT (INCLUDING NEGLIGENCE OR OTHERWISE) ARISING IN | 
| 154 |  |  |  |  |  |  | **  ANY WAY OUT OF THE USE OF THIS SOFTWARE, EVEN IF ADVISED OF THE | 
| 155 |  |  |  |  |  |  | **  POSSIBILITY OF SUCH DAMAGE. | 
| 156 |  |  |  |  |  |  | ** | 
| 157 |  |  |  |  |  |  | */ |