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/* |
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*+ |
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* Name: |
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* palPrec |
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* Purpose: |
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* Form the matrix of precession between two epochs (IAU 2006) |
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* Language: |
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* Starlink ANSI C |
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* Type of Module: |
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* Library routine |
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* Invocation: |
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* palPrec( double ep0, double ep1, double rmatp[3][3] ) |
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* Arguments: |
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* ep0 = double (Given) |
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* Beginning epoch |
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* ep1 = double (Given) |
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* Ending epoch |
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* rmatp = double[3][3] (Returned) |
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* Precession matrix |
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* Description: |
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* The IAU 2006 precession matrix from ep0 to ep1 is found and |
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* returned. The matrix is in the sense V(EP1) = RMATP * V(EP0). |
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* The epochs are TDB (loosely TT) Julian epochs. |
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* |
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* Though the matrix method itself is rigorous, the precession |
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* angles are expressed through canonical polynomials which are |
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* valid only for a limited time span of a few hundred years around |
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* the current epoch. |
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* Authors: |
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* PTW: Pat Wallace (STFC) |
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* DSB: David Berry (JAC, Hawaii) |
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* {enter_new_authors_here} |
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* History: |
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* 2012-02-10 (DSB): |
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* Initial version with documentation taken from Fortran SLA |
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* Adapted with permission from the Fortran SLALIB library. |
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* {enter_further_changes_here} |
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* Copyright: |
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* Copyright (C) 1996 Rutherford Appleton Laboratory |
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* Copyright (C) 2012 Science and Technology Facilities Council. |
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* All Rights Reserved. |
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* Licence: |
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* This program is free software: you can redistribute it and/or |
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* modify it under the terms of the GNU Lesser General Public |
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* License as published by the Free Software Foundation, either |
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* version 3 of the License, or (at your option) any later |
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* version. |
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* |
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* This program is distributed in the hope that it will be useful, |
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* but WITHOUT ANY WARRANTY; without even the implied warranty of |
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* MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the |
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* GNU Lesser General Public License for more details. |
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* |
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* You should have received a copy of the GNU Lesser General |
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* License along with this program. If not, see |
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* . |
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* Bugs: |
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* {note_any_bugs_here} |
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*- |
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*/ |
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#include "pal.h" |
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#include "pal1sofa.h" |
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void palPrec( double ep0, double ep1, double rmatp[3][3] ){ |
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/* Local Variables: */ |
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double rmatq[3][3]; |
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double ep0_days; |
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double ep1_days; |
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/* Convert supplied dates to days since J2000 */ |
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182
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ep0_days = ( ep0 - 2000.0 )*ERFA_DJY; |
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ep1_days = ( ep1 - 2000.0 )*ERFA_DJY; |
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/* If beginning epoch is J2000, just return the rotation matrix from |
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J2000 to EP1. */ |
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182
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if( ep0 == 2000.0 ) { |
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eraPmat06( ERFA_DJ00, ep1_days, rmatp ); |
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/* If end epoch is J2000, get the rotation matrix from J2000 to EP0 and |
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then transpose it to get the rotation matrix from EP0 to J2000. */ |
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180
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} else if( ep1 == 2000.0 ) { |
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180
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eraPmat06( ERFA_DJ00, ep0_days, rmatp ); |
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eraTr( rmatp, rmatp ); |
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/* Otherwise. get the two matrices used above and multiply them |
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together. */ |
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} else { |
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eraPmat06( ERFA_DJ00, ep0_days, rmatp ); |
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eraTr( rmatp, rmatp ); |
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eraPmat06( ERFA_DJ00, ep1_days, rmatq ); |
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eraRxr( rmatp, rmatq, rmatp ); |
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} |
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} |