#include "sofam.h"
void iauPn06a(double date1, double date2,
double *dpsi, double *deps, double *epsa,
double rb[3][3], double rp[3][3], double rbp[3][3],
double rn[3][3], double rbpn[3][3])
/*
** - - - - - - - - -
** i a u P n 0 6 a
** - - - - - - - - -
**
** Precession-nutation, IAU 2006/2000A models: a multi-purpose function,
** supporting classical (equinox-based) use directly and CIO-based use
** indirectly.
**
** This function is part of the International Astronomical Union's
** SOFA (Standards Of Fundamental Astronomy) software collection.
**
** Status: support function.
**
** Given:
** date1,date2 double TT as a 2-part Julian Date (Note 1)
**
** Returned:
** dpsi,deps double nutation (Note 2)
** epsa double mean obliquity (Note 3)
** rb double[3][3] frame bias matrix (Note 4)
** rp double[3][3] precession matrix (Note 5)
** rbp double[3][3] bias-precession matrix (Note 6)
** rn double[3][3] nutation matrix (Note 7)
** rbpn double[3][3] GCRS-to-true matrix (Notes 8,9)
**
** 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.
**
** 2) The nutation components (luni-solar + planetary, IAU 2000A) in
** longitude and obliquity are in radians and with respect to the
** equinox and ecliptic of date. Free core nutation is omitted;
** for the utmost accuracy, use the iauPn06 function, where the
** nutation components are caller-specified.
**
** 3) The mean obliquity is consistent with the IAU 2006 precession.
**
** 4) The matrix rb transforms vectors from GCRS to mean J2000.0 by
** applying frame bias.
**
** 5) The matrix rp transforms vectors from mean J2000.0 to mean of
** date by applying precession.
**
** 6) The matrix rbp transforms vectors from GCRS to mean of date by
** applying frame bias then precession. It is the product rp x rb.
**
** 7) The matrix rn transforms vectors from mean of date to true of
** date by applying the nutation (luni-solar + planetary).
**
** 8) The matrix rbpn transforms vectors from GCRS to true of date
** (CIP/equinox). It is the product rn x rbp, applying frame bias,
** precession and nutation in that order.
**
** 9) The X,Y,Z coordinates of the IAU 2006/2000A Celestial
** Intermediate Pole are elements (1,1-3) of the matrix rbpn.
**
** 10) It is permissible to re-use the same array in the returned
** arguments. The arrays are filled in the stated order.
**
** Called:
** iauNut06a nutation, IAU 2006/2000A
** iauPn06 bias/precession/nutation results, IAU 2006
**
** Reference:
**
** Capitaine, N. & Wallace, P.T., 2006, Astron.Astrophys. 450, 855
**
** This revision: 2009 December 18
**
** SOFA release 2012-03-01
**
** Copyright (C) 2012 IAU SOFA Board. See notes at end.
*/
{
/* Nutation. */
iauNut06a(date1, date2, dpsi, deps);
/* Remaining results. */
iauPn06(date1, date2, *dpsi, *deps, epsa, rb, rp, rbp, rn, rbpn);
return;
/*----------------------------------------------------------------------
**
** Copyright (C) 2012
** Standards Of Fundamental Astronomy Board
** of the International Astronomical Union.
**
** =====================
** SOFA Software License
** =====================
**
** NOTICE TO USER:
**
** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
** CONDITIONS WHICH APPLY TO ITS USE.
**
** 1. The Software is owned by the IAU SOFA Board ("SOFA").
**
** 2. Permission is granted to anyone to use the SOFA software for any
** purpose, including commercial applications, free of charge and
** without payment of royalties, subject to the conditions and
** restrictions listed below.
**
** 3. You (the user) may copy and distribute SOFA source code to others,
** and use and adapt its code and algorithms in your own software,
** on a world-wide, royalty-free basis. That portion of your
** distribution that does not consist of intact and unchanged copies
** of SOFA source code files is a "derived work" that must comply
** with the following requirements:
**
** a) Your work shall be marked or carry a statement that it
** (i) uses routines and computations derived by you from
** software provided by SOFA under license to you; and
** (ii) does not itself constitute software provided by and/or
** endorsed by SOFA.
**
** b) The source code of your derived work must contain descriptions
** of how the derived work is based upon, contains and/or differs
** from the original SOFA software.
**
** c) The names of all routines in your derived work shall not
** include the prefix "iau" or "sofa" or trivial modifications
** thereof such as changes of case.
**
** d) The origin of the SOFA components of your derived work must
** not be misrepresented; you must not claim that you wrote the
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**
** e) These requirements must be reproduced intact in any source
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**
** Note that, as originally distributed, the SOFA software is
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** and consequently third-party modifications are discouraged. All
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**
** 4. You shall not cause the SOFA software to be brought into
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**
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**
** 6. The provision of any version of the SOFA software under the terms
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*
** In any published work or commercial product which uses the SOFA
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** appreciated.
**
** Correspondence concerning SOFA software should be addressed as
** follows:
**
** By email: sofa@ukho.gov.uk
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**
**--------------------------------------------------------------------*/
}