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#include "erfa.h"
void eraTpstv(double xi, double eta, double v0[3], double v[3])
/*
** - - - - - - - - -
** e r a T p s t v
** - - - - - - - - -
**
** In the tangent plane projection, given the star's rectangular
** coordinates and the direction cosines of the tangent point, solve
** for the direction cosines of the star.
**
** Given:
** xi,eta double rectangular coordinates of star image (Note 2)
** v0 double[3] tangent point's direction cosines
**
** Returned:
** v double[3] star's direction cosines
**
** 1) The tangent plane projection is also called the "gnomonic
** projection" and the "central projection".
**
** 2) The eta axis points due north in the adopted coordinate system.
** If the direction cosines represent observed (RA,Dec), the tangent
** plane coordinates (xi,eta) are conventionally called the
** "standard coordinates". If the direction cosines are with
** respect to a right-handed triad, (xi,eta) are also right-handed.
** The units of (xi,eta) are, effectively, radians at the tangent
** point.
**
** 3) The method used is to complete the star vector in the (xi,eta)
** based triad and normalize it, then rotate the triad to put the
** tangent point at the pole with the x-axis aligned to zero
** longitude. Writing (a0,b0) for the celestial spherical
** coordinates of the tangent point, the sequence of rotations is
** (b-pi/2) around the x-axis followed by (-a-pi/2) around the
** z-axis.
**
** 4) If vector v0 is not of unit length, the returned vector v will
** be wrong.
**
** 5) If vector v0 points at a pole, the returned vector v will be
** based on the arbitrary assumption that the longitude coordinate
** of the tangent point is zero.
**
** 6) This function is a member of the following set:
**
** spherical vector solve for
**
** eraTpxes eraTpxev xi,eta
** eraTpsts > eraTpstv < star
** eraTpors eraTporv origin
**
** References:
**
** Calabretta M.R. & Greisen, E.W., 2002, "Representations of
** celestial coordinates in FITS", Astron.Astrophys. 395, 1077
**
** Green, R.M., "Spherical Astronomy", Cambridge University Press,
** 1987, Chapter 13.
**
** This revision: 2018 January 2
**
** Copyright (C) 2013-2021, NumFOCUS Foundation.
** Derived, with permission, from the SOFA library. See notes at end of file.
*/
{
double x, y, z, f, r;
/* Tangent point. */
x = v0[0];
y = v0[1];
z = v0[2];
/* Deal with polar case. */
r = sqrt(x*x + y*y);
if ( r == 0.0 ) {
r = 1e-20;
x = r;
}
/* Star vector length to tangent plane. */
f = sqrt(1.0 + xi*xi + eta*eta);
/* Apply the transformation and normalize. */
v[0] = (x - (xi*y + eta*x*z) / r) / f;
v[1] = (y + (xi*x - eta*y*z) / r) / f;
v[2] = (z + eta*r) / f;
/* Finished. */
}
/*----------------------------------------------------------------------
**
**
** Copyright (C) 2013-2021, 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.
**
*/