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#include "erfa.h" |
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void eraAper13(double ut11, double ut12, eraASTROM *astrom) |
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/* |
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** - - - - - - - - - - |
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** e r a A p e r 1 3 |
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** - - - - - - - - - - |
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** |
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** In the star-independent astrometry parameters, update only the |
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** Earth rotation angle. The caller provides UT1, (n.b. not UTC). |
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** |
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** Given: |
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** ut11 double UT1 as a 2-part... |
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** ut12 double ...Julian Date (Note 1) |
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** astrom eraASTROM* star-independent astrometry parameters: |
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** pmt double not used |
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** eb double[3] not used |
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** eh double[3] not used |
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** em double not used |
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** v double[3] not used |
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** bm1 double not used |
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** bpn double[3][3] not used |
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** along double longitude + s' (radians) |
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** xpl double not used |
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** ypl double not used |
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** sphi double not used |
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** cphi double not used |
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** diurab double not used |
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** eral double not used |
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** refa double not used |
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** refb double not used |
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** |
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** Returned: |
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** astrom eraASTROM* star-independent astrometry parameters: |
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** pmt double unchanged |
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** eb double[3] unchanged |
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** eh double[3] unchanged |
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** em double unchanged |
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** v double[3] unchanged |
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** bm1 double unchanged |
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** bpn double[3][3] unchanged |
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** along double unchanged |
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** xpl double unchanged |
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** ypl double unchanged |
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** sphi double unchanged |
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** cphi double unchanged |
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** diurab double unchanged |
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** eral double "local" Earth rotation angle (radians) |
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** refa double unchanged |
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** refb double unchanged |
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** |
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** Notes: |
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** |
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** 1) The UT1 date (n.b. not UTC) ut11+ut12 is a Julian Date, |
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** apportioned in any convenient way between the arguments ut11 and |
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** ut12. For example, JD(UT1)=2450123.7 could be expressed in any |
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** of these ways, among others: |
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** |
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** ut11 ut12 |
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** |
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** 2450123.7 0.0 (JD method) |
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** 2451545.0 -1421.3 (J2000 method) |
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** 2400000.5 50123.2 (MJD method) |
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** 2450123.5 0.2 (date & time method) |
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** |
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** The JD method is the most natural and convenient to use in cases |
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** where the loss of several decimal digits of resolution is |
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** acceptable. The J2000 and MJD methods are good compromises |
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** between resolution and convenience. The date & time method is |
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** best matched to the algorithm used: maximum precision is |
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** delivered when the ut11 argument is for 0hrs UT1 on the day in |
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** question and the ut12 argument lies in the range 0 to 1, or vice |
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** versa. |
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** |
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** 2) If the caller wishes to provide the Earth rotation angle itself, |
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** the function eraAper can be used instead. One use of this |
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** technique is to substitute Greenwich apparent sidereal time and |
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** thereby to support equinox based transformations directly. |
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** |
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** 3) This is one of several functions that inserts into the astrom |
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** structure star-independent parameters needed for the chain of |
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** astrometric transformations ICRS <-> GCRS <-> CIRS <-> observed. |
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** |
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** The various functions support different classes of observer and |
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** portions of the transformation chain: |
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** |
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** functions observer transformation |
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** |
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** eraApcg eraApcg13 geocentric ICRS <-> GCRS |
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** eraApci eraApci13 terrestrial ICRS <-> CIRS |
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** eraApco eraApco13 terrestrial ICRS <-> observed |
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** eraApcs eraApcs13 space ICRS <-> GCRS |
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** eraAper eraAper13 terrestrial update Earth rotation |
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** eraApio eraApio13 terrestrial CIRS <-> observed |
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** |
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** Those with names ending in "13" use contemporary ERFA models to |
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** compute the various ephemerides. The others accept ephemerides |
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** supplied by the caller. |
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** |
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** The transformation from ICRS to GCRS covers space motion, |
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** parallax, light deflection, and aberration. From GCRS to CIRS |
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** comprises frame bias and precession-nutation. From CIRS to |
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** observed takes account of Earth rotation, polar motion, diurnal |
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** aberration and parallax (unless subsumed into the ICRS <-> GCRS |
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** transformation), and atmospheric refraction. |
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** |
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** Called: |
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** eraAper astrometry parameters: update ERA |
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** eraEra00 Earth rotation angle, IAU 2000 |
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** |
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** Copyright (C) 2013-2020, 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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eraAper(eraEra00(ut11,ut12), astrom); |
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/* Finished. */ |
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} |
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/*---------------------------------------------------------------------- |
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** |
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** |
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** Copyright (C) 2013-2020, 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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*/ |