IIINSTRUMENT Pipeline Reference Manual 6.2.5
isaac_physicalmodel.h
1/* $Id: isaac_physicalmodel.h,v 1.6 2013-03-12 08:06:48 llundin Exp $
2 *
3 * This file is part of the ISAAC Pipeline
4 * Copyright (C) 2002,2003 European Southern Observatory
5 *
6 * This program is free software; you can redistribute it and/or modify
7 * it under the terms of the GNU General Public License as published by
8 * the Free Software Foundation; either version 2 of the License, or
9 * (at your option) any later version.
10 *
11 * This program is distributed in the hope that it will be useful,
12 * but WITHOUT ANY WARRANTY; without even the implied warranty of
13 * MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the
14 * GNU General Public License for more details.
15 *
16 * You should have received a copy of the GNU General Public License
17 * along with this program; if not, write to the Free Software
18 * Foundation, Inc., 51 Franklin St, Fifth Floor, Boston, MA 02111-1307 USA
19 */
20
21/*
22 * $Author: llundin $
23 * $Date: 2013-03-12 08:06:48 $
24 * $Revision: 1.6 $
25 * $Name: not supported by cvs2svn $
26 */
27
28#ifndef ISAAC_PHYSICALMODEL_H
29#define ISAAC_PHYSICALMODEL_H
30
31/*-----------------------------------------------------------------------------
32 Includes
33 -----------------------------------------------------------------------------*/
34
35#include <cpl_type.h>
36
37/* TEMPORARY SUPPORT OF CPL 5.x */
38#ifndef CPL_SIZE_FORMAT
39#define CPL_SIZE_FORMAT "d"
40#define cpl_size int
41#endif
42/* END TEMPORARY SUPPORT OF CPL 5.x */
43
44/*-----------------------------------------------------------------------------
45 Prototypes
46 -----------------------------------------------------------------------------*/
47
48double * isaac_get_disprel_estimate(const char *, cpl_size);
49double * isaac_physical_model(double, const char *, const char *, int);
50
51#endif
double * isaac_physical_model(double, const char *, const char *, int)
ISAAC physical model.
double * isaac_get_disprel_estimate(const char *, cpl_size)
Estimate the instrument wavelength range.