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+#include "erfa.h"
+
+void eraPb06(double date1, double date2,
+ double *bzeta, double *bz, double *btheta)
+/*
+** - - - - - - - -
+** e r a P b 0 6
+** - - - - - - - -
+**
+** This function forms three Euler angles which implement general
+** precession from epoch J2000.0, using the IAU 2006 model. Frame
+** bias (the offset between ICRS and mean J2000.0) is included.
+**
+** Given:
+** date1,date2 double TT as a 2-part Julian Date (Note 1)
+**
+** Returned:
+** bzeta double 1st rotation: radians cw around z
+** bz double 3rd rotation: radians cw around z
+** btheta double 2nd rotation: radians ccw around y
+**
+** 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 traditional accumulated precession angles zeta_A, z_A,
+** theta_A cannot be obtained in the usual way, namely through
+** polynomial expressions, because of the frame bias. The latter
+** means that two of the angles undergo rapid changes near this
+** date. They are instead the results of decomposing the
+** precession-bias matrix obtained by using the Fukushima-Williams
+** method, which does not suffer from the problem. The
+** decomposition returns values which can be used in the
+** conventional formulation and which include frame bias.
+**
+** 3) The three angles are returned in the conventional order, which
+** is not the same as the order of the corresponding Euler
+** rotations. The precession-bias matrix is
+** R_3(-z) x R_2(+theta) x R_3(-zeta).
+**
+** 4) Should zeta_A, z_A, theta_A angles be required that do not
+** contain frame bias, they are available by calling the ERFA
+** function eraP06e.
+**
+** Called:
+** eraPmat06 PB matrix, IAU 2006
+** eraRz rotate around Z-axis
+**
+** Copyright (C) 2013-2014, NumFOCUS Foundation.
+** Derived, with permission, from the SOFA library. See notes at end of file.
+*/
+{
+ double r[3][3], r31, r32;
+
+
+/* Precession matrix via Fukushima-Williams angles. */
+ eraPmat06(date1, date2, r);
+
+/* Solve for z. */
+ *bz = atan2(r[1][2], r[0][2]);
+
+/* Remove it from the matrix. */
+ eraRz(*bz, r);
+
+/* Solve for the remaining two angles. */
+ *bzeta = atan2 (r[1][0], r[1][1]);
+ r31 = r[2][0];
+ r32 = r[2][1];
+ *btheta = atan2(-ERFA_DSIGN(sqrt(r31 * r31 + r32 * r32), r[0][2]),
+ r[2][2]);
+
+ return;
+
+}
+/*----------------------------------------------------------------------
+**
+**
+** Copyright (C) 2013-2014, NumFOCUS Foundation.
+** All rights reserved.
+**
+** This library is derived, with permission, from the International
+** Astronomical Union's "Standards of Fundamental Astronomy" library,
+** available from http://www.iausofa.org.
+**
+** The ERFA version is intended to retain identical functionality to
+** the SOFA library, but made distinct through different function and
+** file names, as set out in the SOFA license conditions. The SOFA
+** original has a role as a reference standard for the IAU and IERS,
+** and consequently redistribution is permitted only in its unaltered
+** state. The ERFA version is not subject to this restriction and
+** therefore can be included in distributions which do not support the
+** concept of "read only" software.
+**
+** Although the intent is to replicate the SOFA API (other than
+** replacement of prefix names) and results (with the exception of
+** bugs; any that are discovered will be fixed), SOFA is not
+** responsible for any errors found in this version of the library.
+**
+** If you wish to acknowledge the SOFA heritage, please acknowledge
+** that you are using a library derived from SOFA, rather than SOFA
+** itself.
+**
+**
+** TERMS AND CONDITIONS
+**
+** Redistribution and use in source and binary forms, with or without
+** modification, are permitted provided that the following conditions
+** are met:
+**
+** 1 Redistributions of source code must retain the above copyright
+** notice, this list of conditions and the following disclaimer.
+**
+** 2 Redistributions in binary form must reproduce the above copyright
+** notice, this list of conditions and the following disclaimer in
+** the documentation and/or other materials provided with the
+** distribution.
+**
+** 3 Neither the name of the Standards Of Fundamental Astronomy Board,
+** the International Astronomical Union nor the names of its
+** contributors may be used to endorse or promote products derived
+** from this software without specific prior written permission.
+**
+** THIS SOFTWARE IS PROVIDED BY THE COPYRIGHT HOLDERS AND CONTRIBUTORS
+** "AS IS" AND ANY EXPRESS OR IMPLIED WARRANTIES, INCLUDING, BUT NOT
+** LIMITED TO, THE IMPLIED WARRANTIES OF MERCHANTABILITY AND FITNESS
+** FOR A PARTICULAR PURPOSE ARE DISCLAIMED. IN NO EVENT SHALL THE
+** COPYRIGHT HOLDER OR CONTRIBUTORS BE LIABLE FOR ANY DIRECT, INDIRECT,
+** INCIDENTAL, SPECIAL, EXEMPLARY, OR CONSEQUENTIAL DAMAGES (INCLUDING,
+** BUT NOT LIMITED TO, PROCUREMENT OF SUBSTITUTE GOODS OR SERVICES;
+** LOSS OF USE, DATA, OR PROFITS; OR BUSINESS INTERRUPTION) HOWEVER
+** CAUSED AND ON ANY THEORY OF LIABILITY, WHETHER IN CONTRACT, STRICT
+** LIABILITY, OR TORT (INCLUDING NEGLIGENCE OR OTHERWISE) ARISING IN
+** ANY WAY OUT OF THE USE OF THIS SOFTWARE, EVEN IF ADVISED OF THE
+** POSSIBILITY OF SUCH DAMAGE.
+**
+*/