update ast 8.6.3

1 files changed, 222 insertions, 0 deletions

diff --git a/ast/erfa/atio13.c b/ast/erfa/atio13.c
new file mode 100644
index 0000000..6201776
--- /dev/null
+++ b/ast/erfa/atio13.c
@@ -0,0 +1,222 @@
+#include "erfa.h"
+
+int eraAtio13(double ri, double di,
+              double utc1, double utc2, double dut1,
+              double elong, double phi, double hm, double xp, double yp,
+              double phpa, double tc, double rh, double wl,
+              double *aob, double *zob, double *hob,
+              double *dob, double *rob)
+/*
+**  - - - - - - - - - -
+**   e r a A t i o 1 3
+**  - - - - - - - - - -
+**
+**  CIRS RA,Dec to observed place.  The caller supplies UTC, site
+**  coordinates, ambient air conditions and observing wavelength.
+**
+**  Given:
+**     ri     double   CIRS right ascension (CIO-based, radians)
+**     di     double   CIRS declination (radians)
+**     utc1   double   UTC as a 2-part...
+**     utc2   double   ...quasi Julian Date (Notes 1,2)
+**     dut1   double   UT1-UTC (seconds, Note 3)
+**     elong  double   longitude (radians, east +ve, Note 4)
+**     phi    double   geodetic latitude (radians, Note 4)
+**     hm     double   height above ellipsoid (m, geodetic Notes 4,6)
+**     xp,yp  double   polar motion coordinates (radians, Note 5)
+**     phpa   double   pressure at the observer (hPa = mB, Note 6)
+**     tc     double   ambient temperature at the observer (deg C)
+**     rh     double   relative humidity at the observer (range 0-1)
+**     wl     double   wavelength (micrometers, Note 7)
+**
+**  Returned:
+**     aob    double*  observed azimuth (radians: N=0,E=90)
+**     zob    double*  observed zenith distance (radians)
+**     hob    double*  observed hour angle (radians)
+**     dob    double*  observed declination (radians)
+**     rob    double*  observed right ascension (CIO-based, radians)
+**
+**  Returned (function value):
+**            int      status: +1 = dubious year (Note 2)
+**                              0 = OK
+**                             -1 = unacceptable date
+**
+**  Notes:
+**
+**  1)  utc1+utc2 is quasi Julian Date (see Note 2), apportioned in any
+**      convenient way between the two arguments, for example where utc1
+**      is the Julian Day Number and utc2 is the fraction of a day.
+**
+**      However, JD cannot unambiguously represent UTC during a leap
+**      second unless special measures are taken.  The convention in the
+**      present function is that the JD day represents UTC days whether
+**      the length is 86399, 86400 or 86401 SI seconds.
+**
+**      Applications should use the function eraDtf2d to convert from
+**      calendar date and time of day into 2-part quasi Julian Date, as
+**      it implements the leap-second-ambiguity convention just
+**      described.
+**
+**  2)  The warning status "dubious year" flags UTCs that predate the
+**      introduction of the time scale or that are too far in the
+**      future to be trusted.  See eraDat for further details.
+**
+**  3)  UT1-UTC is tabulated in IERS bulletins.  It increases by exactly
+**      one second at the end of each positive UTC leap second,
+**      introduced in order to keep UT1-UTC within +/- 0.9s.  n.b. This
+**      practice is under review, and in the future UT1-UTC may grow
+**      essentially without limit.
+**
+**  4)  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.
+**
+**  5)  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.
+**
+**  6)  If hm, the height above the ellipsoid of the observing station
+**      in meters, is not known but phpa, the pressure in hPa (=mB), is
+**      available, an adequate estimate of hm can be obtained from the
+**      expression
+**
+**            hm = -29.3 * tsl * log ( phpa / 1013.25 );
+**
+**      where tsl is the approximate sea-level air temperature in K
+**      (See Astrophysical Quantities, C.W.Allen, 3rd edition, section
+**      52).  Similarly, if the pressure phpa is not known, it can be
+**      estimated from the height of the observing station, hm, as
+**      follows:
+**
+**            phpa = 1013.25 * exp ( -hm / ( 29.3 * tsl ) );
+**
+**      Note, however, that the refraction is nearly proportional to
+**      the pressure and that an accurate phpa value is important for
+**      precise work.
+**
+**  7)  The argument wl specifies the observing wavelength in
+**      micrometers.  The transition from optical to radio is assumed to
+**      occur at 100 micrometers (about 3000 GHz).
+**
+**  8)  "Observed" Az,ZD means the position that would be seen by a
+**      perfect geodetically aligned theodolite.  (Zenith distance is
+**      used rather than altitude in order to reflect the fact that no
+**      allowance is made for depression of the horizon.)  This is
+**      related to the observed HA,Dec via the standard rotation, using
+**      the geodetic latitude (corrected for polar motion), while the
+**      observed HA and RA are related simply through the Earth rotation
+**      angle and the site longitude.  "Observed" RA,Dec or HA,Dec thus
+**      means the position that would be seen by a perfect equatorial
+**      with its polar axis aligned to the Earth's axis of rotation.
+**
+**  9)  The accuracy of the result is limited by the corrections for
+**      refraction, which use a simple A*tan(z) + B*tan^3(z) model.
+**      Providing the meteorological parameters are known accurately and
+**      there are no gross local effects, the predicted astrometric
+**      coordinates should be within 0.05 arcsec (optical) or 1 arcsec
+**      (radio) for a zenith distance of less than 70 degrees, better
+**      than 30 arcsec (optical or radio) at 85 degrees and better
+**      than 20 arcmin (optical) or 30 arcmin (radio) at the horizon.
+**
+**  10) The complementary functions eraAtio13 and eraAtoi13 are self-
+**      consistent to better than 1 microarcsecond all over the
+**      celestial sphere.
+**
+**  11) 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.
+**
+**  Called:
+**     eraApio13    astrometry parameters, CIRS-observed, 2013
+**     eraAtioq     quick CIRS to observed
+**
+**  Copyright (C) 2013-2016, NumFOCUS Foundation.
+**  Derived, with permission, from the SOFA library.  See notes at end of file.
+*/
+{
+   int j;
+   eraASTROM astrom;
+
+
+/* Star-independent astrometry parameters for CIRS->observed. */
+   j = eraApio13(utc1, utc2, dut1, elong, phi, hm, xp, yp,
+                 phpa, tc, rh, wl, &astrom);
+
+/* Abort if bad UTC. */
+   if ( j < 0 ) return j;
+
+/* Transform CIRS to observed. */
+   eraAtioq(ri, di, &astrom, aob, zob, hob, dob, rob);
+
+/* Return OK/warning status. */
+   return j;
+
+/* 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.
+**  
+*/