update ast

1 files changed, 0 insertions, 213 deletions

diff --git a/ast/erfa/apio.c b/ast/erfa/apio.c
deleted file mode 100644
index ebc5569..0000000
--- a/ast/erfa/apio.c
+++ /dev/null
@@ -1,213 +0,0 @@
-#include "erfa.h"
-
-void eraApio(double sp, double theta,
-             double elong, double phi, double hm, double xp, double yp,
-             double refa, double refb,
-             eraASTROM *astrom)
-/*
-**  - - - - - - - -
-**   e r a A p i o
-**  - - - - - - - -
-**
-**  For a terrestrial observer, prepare star-independent astrometry
-**  parameters for transformations between CIRS and observed
-**  coordinates.  The caller supplies the Earth orientation information
-**  and the refraction constants as well as the site coordinates.
-**
-**  Given:
-**     sp     double      the TIO locator s' (radians, Note 1)
-**     theta  double      Earth rotation angle (radians)
-**     elong  double      longitude (radians, east +ve, Note 2)
-**     phi    double      geodetic latitude (radians, Note 2)
-**     hm     double      height above ellipsoid (m, geodetic Note 2)
-**     xp,yp  double      polar motion coordinates (radians, Note 3)
-**     refa   double      refraction constant A (radians, Note 4)
-**     refb   double      refraction constant B (radians, Note 4)
-**
-**  Returned:
-**     astrom eraASTROM*  star-independent astrometry parameters:
-**      pmt    double       unchanged
-**      eb     double[3]    unchanged
-**      eh     double[3]    unchanged
-**      em     double       unchanged
-**      v      double[3]    unchanged
-**      bm1    double       unchanged
-**      bpn    double[3][3] unchanged
-**      along  double       longitude + s' (radians)
-**      xpl    double       polar motion xp wrt local meridian (radians)
-**      ypl    double       polar motion yp wrt local meridian (radians)
-**      sphi   double       sine of geodetic latitude
-**      cphi   double       cosine of geodetic latitude
-**      diurab double       magnitude of diurnal aberration vector
-**      eral   double       "local" Earth rotation angle (radians)
-**      refa   double       refraction constant A (radians)
-**      refb   double       refraction constant B (radians)
-**
-**  Notes:
-**
-**  1) sp, the TIO locator s', is a tiny quantity needed only by the
-**     most precise applications.  It can either be set to zero or
-**     predicted using the ERFA function eraSp00.
-**
-**  2) The geographical coordinates are with respect to the ERFA_WGS84
-**     reference ellipsoid.  TAKE CARE WITH THE LONGITUDE SIGN:  the
-**     longitude required by the present function is east-positive
-**     (i.e. right-handed), in accordance with geographical convention.
-**
-**  3) The polar motion xp,yp can be obtained from IERS bulletins.  The
-**     values are the coordinates (in radians) of the Celestial
-**     Intermediate Pole with respect to the International Terrestrial
-**     Reference System (see IERS Conventions 2003), measured along the
-**     meridians 0 and 90 deg west respectively.  For many applications,
-**     xp and yp can be set to zero.
-**
-**     Internally, the polar motion is stored in a form rotated onto the
-**     local meridian.
-**
-**  4) The refraction constants refa and refb are for use in a
-**     dZ = A*tan(Z)+B*tan^3(Z) model, where Z is the observed
-**     (i.e. refracted) zenith distance and dZ is the amount of
-**     refraction.
-**
-**  5) It is advisable to take great care with units, as even unlikely
-**     values of the input parameters are accepted and processed in
-**     accordance with the models used.
-**
-**  6) In cases where the caller does not wish to provide the Earth
-**     rotation information and refraction constants, the function
-**     eraApio13 can be used instead of the present function.  This
-**     starts from UTC and weather readings etc. and computes suitable
-**     values using other ERFA functions.
-**
-**  7) This is one of several functions that inserts into the astrom
-**     structure star-independent parameters needed for the chain of
-**     astrometric transformations ICRS <-> GCRS <-> CIRS <-> observed.
-**
-**     The various functions support different classes of observer and
-**     portions of the transformation chain:
-**
-**          functions         observer        transformation
-**
-**       eraApcg eraApcg13    geocentric      ICRS <-> GCRS
-**       eraApci eraApci13    terrestrial     ICRS <-> CIRS
-**       eraApco eraApco13    terrestrial     ICRS <-> observed
-**       eraApcs eraApcs13    space           ICRS <-> GCRS
-**       eraAper eraAper13    terrestrial     update Earth rotation
-**       eraApio eraApio13    terrestrial     CIRS <-> observed
-**
-**     Those with names ending in "13" use contemporary ERFA models to
-**     compute the various ephemerides.  The others accept ephemerides
-**     supplied by the caller.
-**
-**     The transformation from ICRS to GCRS covers space motion,
-**     parallax, light deflection, and aberration.  From GCRS to CIRS
-**     comprises frame bias and precession-nutation.  From CIRS to
-**     observed takes account of Earth rotation, polar motion, diurnal
-**     aberration and parallax (unless subsumed into the ICRS <-> GCRS
-**     transformation), and atmospheric refraction.
-**
-**  8) The context structure astrom produced by this function is used by
-**     eraAtioq and eraAtoiq.
-**
-**  Called:
-**     eraPvtob     position/velocity of terrestrial station
-**     eraAper      astrometry parameters: update ERA
-**
-**  Copyright (C) 2013-2016, NumFOCUS Foundation.
-**  Derived, with permission, from the SOFA library.  See notes at end of file.
-*/
-{
-   double sl, cl, pv[2][3];
-
-
-/* Longitude with adjustment for TIO locator s'. */
-   astrom->along = elong + sp;
-
-/* Polar motion, rotated onto the local meridian. */
-   sl = sin(astrom->along);
-   cl = cos(astrom->along);
-   astrom->xpl = xp*cl - yp*sl;
-   astrom->ypl = xp*sl + yp*cl;
-
-/* Functions of latitude. */
-   astrom->sphi = sin(phi);
-   astrom->cphi = cos(phi);
-
-/* Observer's geocentric position and velocity (m, m/s, CIRS). */
-   eraPvtob(elong, phi, hm, xp, yp, sp, theta, pv);
-
-/* Magnitude of diurnal aberration vector. */
-   astrom->diurab = sqrt(pv[1][0]*pv[1][0]+pv[1][1]*pv[1][1]) / ERFA_CMPS;
-
-/* Refraction constants. */
-   astrom->refa = refa;
-   astrom->refb = refb;
-
-/* Local Earth rotation angle. */
-   eraAper(theta, astrom);
-
-/* Finished. */
-
-}
-/*----------------------------------------------------------------------
-**  
-**  
-**  Copyright (C) 2013-2016, 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.
-**  
-*/