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spx.h
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/*============================================================================
WCSLIB 8.9 - an implementation of the FITS WCS standard.
Copyright (C) 1995-2026, Mark Calabretta
This file is part of WCSLIB.
WCSLIB is free software: you can redistribute it and/or modify it under the
terms of the GNU Lesser General Public License as published by the Free
Software Foundation, either version 3 of the License, or (at your option)
any later version.
WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY
WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS
FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for
more details.
You should have received a copy of the GNU Lesser General Public License
along with WCSLIB. If not, see http://www.gnu.org/licenses.
Author: Mark Calabretta, Australia Telescope National Facility, CSIRO.
http://www.atnf.csiro.au/computing/software/wcs
$Id: spx.h,v 8.9 2026/06/18 13:00:03 mcalabre Exp $
*=============================================================================
*
* WCSLIB 8.9 - C routines that implement the FITS World Coordinate System
* (WCS) standard. Refer to the README file provided with WCSLIB for an
* overview of the library.
*
*
* Summary of the spx routines
* ---------------------------
* Routines in this suite implement the spectral coordinate systems recognized
* by the FITS World Coordinate System (WCS) standard, as described in
*
= "Representations of world coordinates in FITS",
= Greisen, E.W., & Calabretta, M.R. 2002, A&A, 395, 1061 (WCS Paper I)
=
= "Representations of spectral coordinates in FITS",
= Greisen, E.W., Calabretta, M.R., Valdes, F.G., & Allen, S.L.
= 2006, A&A, 446, 747 (WCS Paper III)
*
* specx() is a scalar routine that, given one spectral variable (e.g.
* frequency), computes all the others (e.g. wavelength, velocity, etc.) plus
* the required derivatives of each with respect to the others. The results
* are returned in the spxprm struct.
*
* spxperr() prints the error message(s) (if any) stored in a spxprm struct.
*
* The remaining routines are all vector conversions from one spectral
* variable to another. The API of these functions only differ in whether the
* rest frequency or wavelength need be supplied.
*
* Non-linear:
* - freqwave() frequency -> vacuum wavelength
* - wavefreq() vacuum wavelength -> frequency
*
* - freqawav() frequency -> air wavelength
* - awavfreq() air wavelength -> frequency
*
* - freqvelo() frequency -> relativistic velocity
* - velofreq() relativistic velocity -> frequency
*
* - waveawav() vacuum wavelength -> air wavelength
* - awavwave() air wavelength -> vacuum wavelength
*
* - wavevelo() vacuum wavelength -> relativistic velocity
* - velowave() relativistic velocity -> vacuum wavelength
*
* - awavvelo() air wavelength -> relativistic velocity
* - veloawav() relativistic velocity -> air wavelength
*
* Linear:
* - freqafrq() frequency -> angular frequency
* - afrqfreq() angular frequency -> frequency
*
* - freqener() frequency -> energy
* - enerfreq() energy -> frequency
*
* - freqwavn() frequency -> wave number
* - wavnfreq() wave number -> frequency
*
* - freqvrad() frequency -> radio velocity
* - vradfreq() radio velocity -> frequency
*
* - wavevopt() vacuum wavelength -> optical velocity
* - voptwave() optical velocity -> vacuum wavelength
*
* - wavezopt() vacuum wavelength -> redshift
* - zoptwave() redshift -> vacuum wavelength
*
* - velobeta() relativistic velocity -> beta (= v/c)
* - betavelo() beta (= v/c) -> relativistic velocity
*
* These are the workhorse routines, to be used for fast transformations.
* Conversions may be done "in place" by calling the routine with the output
* vector set to the input.
*
* Air-to-vacuum wavelength conversion:
* ------------------------------------
* The air-to-vacuum wavelength conversion in early drafts of WCS Paper III
* cites Cox (ed., 2000, Allen’s Astrophysical Quantities, AIP Press,
* Springer-Verlag, New York), which itself derives from Edlén (1953, Journal
* of the Optical Society of America, 43, 339). This is the IAU standard,
* adopted in 1957 and again in 1991. No more recent IAU resolution replaces
* this relation, and it is the one used by WCSLIB.
*
* However, the Cox relation was replaced in later drafts of Paper III, and as
* eventually published, by the IUGG relation (1999, International Union of
* Geodesy and Geophysics, comptes rendus of the 22nd General Assembly,
* Birmingham UK, p111). There is a nearly constant ratio between the two,
* with IUGG/Cox = 1.000015 over most of the range between 200nm and 10,000nm.
*
* The IUGG relation itself is derived from the work of Ciddor (1996, Applied
* Optics, 35, 1566), which is used directly by the Sloan Digital Sky Survey.
* It agrees closely with Cox; longwards of 2500nm, the ratio Ciddor/Cox is
* fixed at 1.000000021, decreasing only slightly, to 1.000000018, at 1000nm.
*
* The Cox, IUGG, and Ciddor relations all accurately provide the wavelength
* dependence of the air-to-vacuum wavelength conversion. However, for full
* accuracy, the atmospheric temperature, pressure, and partial pressure of
* water vapour must be taken into account. These will determine a small,
* wavelength-independent scale factor and offset, which is not considered by
* WCS Paper III.
*
* WCS Paper III is also silent on the question of the range of validity of the
* air-to-vacuum wavelength conversion. Cox's relation would appear to be
* valid in the range 200nm to 10,000nm. Both the Cox and the Ciddor relations
* have singularities below 200nm, with Cox's at 156nm and 83nm. WCSLIB checks
* neither the range of validity, nor for these singularities.
*
* Argument checking:
* ------------------
* The input spectral values are only checked for values that would result
* in floating point exceptions. In particular, negative frequencies and
* wavelengths are allowed, as are velocities greater than the speed of
* light. The same is true for the spectral parameters - rest frequency and
* wavelength.
*
* Accuracy:
* ---------
* No warranty is given for the accuracy of these routines (refer to the
* copyright notice); intending users must satisfy for themselves their
* adequacy for the intended purpose. However, closure effectively to within
* double precision rounding error was demonstrated by test routine tspec.c
* which accompanies this software.
*
*
* specx() - Spectral cross conversions (scalar)
* ---------------------------------------------
* Given one spectral variable specx() computes all the others, plus the
* required derivatives of each with respect to the others.
*
* Given:
* type const char*
* The type of spectral variable given by spec, FREQ,
* AFRQ, ENER, WAVN, VRAD, WAVE, VOPT, ZOPT, AWAV, VELO,
* or BETA (case sensitive).
*
* spec double The spectral variable given, in SI units.
*
* restfrq,
* restwav double Rest frequency [Hz] or rest wavelength in vacuo [m],
* only one of which need be given. The other should be
* set to zero. If both are zero, only a subset of the
* spectral variables can be computed, the remainder are
* set to zero. Specifically, given one of FREQ, AFRQ,
* ENER, WAVN, WAVE, or AWAV the others can be computed
* without knowledge of the rest frequency. Likewise,
* VRAD, VOPT, ZOPT, VELO, and BETA.
*
* Given and returned:
* specs struct spxprm*
* Data structure containing all spectral variables and
* their derivatives, in SI units.
*
* Function return value:
* int Status return value:
* 0: Success.
* 1: Null spxprm pointer passed.
* 2: Invalid spectral parameters.
* 3: Invalid spectral variable.
*
* For returns > 1, a detailed error message is set in
* spxprm::err if enabled, see wcserr_enable().
*
* freqafrq(), afrqfreq(), freqener(), enerfreq(), freqwavn(), wavnfreq(),
* freqwave(), wavefreq(), freqawav(), awavfreq(), waveawav(), awavwave(),
* velobeta(), and betavelo() implement vector conversions between wave-like
* or velocity-like spectral types (i.e. conversions that do not need the rest
* frequency or wavelength). They all have the same API.
*
*
* spxperr() - Print error messages from a spxprm struct
* -----------------------------------------------------
* spxperr() prints the error message(s) (if any) stored in a spxprm struct.
* If there are no errors then nothing is printed. It uses wcserr_prt(), q.v.
*
* Given:
* spx const struct spxprm*
* Spectral variables and their derivatives.
*
* prefix const char *
* If non-NULL, each output line will be prefixed with
* this string.
*
* Function return value:
* int Status return value:
* 0: Success.
* 1: Null spxprm pointer passed.
*
*
* freqafrq() - Convert frequency to angular frequency (vector)
* ------------------------------------------------------------
* freqafrq() converts frequency to angular frequency.
*
* Given:
* param double Ignored.
*
* nspec int Vector length.
*
* instep,
* outstep int Vector strides.
*
* inspec const double[]
* Input spectral variables, in SI units.
*
* Returned:
* outspec double[] Output spectral variables, in SI units.
*
* stat int[] Status return value for each vector element:
* 0: Success.
* 1: Invalid value of inspec.
*
* Function return value:
* int Status return value:
* 0: Success.
* 2: Invalid spectral parameters.
* 4: One or more of the inspec coordinates were
* invalid, as indicated by the stat vector.
*
*
* freqvelo(), velofreq(), freqvrad(), and vradfreq() implement vector
* conversions between frequency and velocity spectral types. They all have
* the same API.
*
*
* freqvelo() - Convert frequency to relativistic velocity (vector)
* ----------------------------------------------------------------
* freqvelo() converts frequency to relativistic velocity.
*
* Given:
* param double Rest frequency [Hz].
*
* nspec int Vector length.
*
* instep,
* outstep int Vector strides.
*
* inspec const double[]
* Input spectral variables, in SI units.
*
* Returned:
* outspec double[] Output spectral variables, in SI units.
*
* stat int[] Status return value for each vector element:
* 0: Success.
* 1: Invalid value of inspec.
*
* Function return value:
* int Status return value:
* 0: Success.
* 2: Invalid spectral parameters.
* 4: One or more of the inspec coordinates were
* invalid, as indicated by the stat vector.
*
*
* wavevelo(), velowave(), awavvelo(), veloawav(), wavevopt(), voptwave(),
* wavezopt(), and zoptwave() implement vector conversions between wavelength
* and velocity spectral types. They all have the same API.
*
*
* wavevelo() - Conversions between wavelength and velocity types (vector)
* -----------------------------------------------------------------------
* wavevelo() converts vacuum wavelength to relativistic velocity.
*
* Given:
* param double Rest wavelength in vacuo [m].
*
* nspec int Vector length.
*
* instep,
* outstep int Vector strides.
*
* inspec const double[]
* Input spectral variables, in SI units.
*
* Returned:
* outspec double[] Output spectral variables, in SI units.
*
* stat int[] Status return value for each vector element:
* 0: Success.
* 1: Invalid value of inspec.
*
* Function return value:
* int Status return value:
* 0: Success.
* 2: Invalid spectral parameters.
* 4: One or more of the inspec coordinates were
* invalid, as indicated by the stat vector.
*
*
* spxprm struct - Spectral variables and their derivatives
* --------------------------------------------------------
* The spxprm struct contains the value of all spectral variables and their
* derivatives. It is used solely by specx() which constructs it from
* information provided via its function arguments.
*
* This struct should be considered read-only, no members need ever be set nor
* should ever be modified by the user.
*
* double restfrq
* (Returned) Rest frequency [Hz].
*
* double restwav
* (Returned) Rest wavelength [m].
*
* int wavetype
* (Returned) True if wave types have been computed, and ...
*
* int velotype
* (Returned) ... true if velocity types have been computed; types are
* defined below.
*
* If one or other of spxprm::restfrq and spxprm::restwav is given
* (non-zero) then all spectral variables may be computed. If both are
* given, restfrq is used. If restfrq and restwav are both zero, only wave
* characteristic xor velocity type spectral variables may be computed
* depending on the variable given. These flags indicate what is
* available.
*
* double freq
* (Returned) Frequency [Hz] (wavetype).
*
* double afrq
* (Returned) Angular frequency [rad/s] (wavetype).
*
* double ener
* (Returned) Photon energy [J] (wavetype).
*
* double wavn
* (Returned) Wave number [/m] (wavetype).
*
* double vrad
* (Returned) Radio velocity [m/s] (velotype).
*
* double wave
* (Returned) Vacuum wavelength [m] (wavetype).
*
* double vopt
* (Returned) Optical velocity [m/s] (velotype).
*
* double zopt
* (Returned) Redshift [dimensionless] (velotype).
*
* double awav
* (Returned) Air wavelength [m] (wavetype).
*
* double velo
* (Returned) Relativistic velocity [m/s] (velotype).
*
* double beta
* (Returned) Relativistic beta [dimensionless] (velotype).
*
* double dfreqafrq
* (Returned) Derivative of frequency with respect to angular frequency
* [/rad] (constant, = 1 / 2*pi), and ...
* double dafrqfreq
* (Returned) ... vice versa [rad] (constant, = 2*pi, always available).
*
* double dfreqener
* (Returned) Derivative of frequency with respect to photon energy
* [/J/s] (constant, = 1/h), and ...
* double denerfreq
* (Returned) ... vice versa [Js] (constant, = h, Planck's constant,
* always available).
*
* double dfreqwavn
* (Returned) Derivative of frequency with respect to wave number [m/s]
* (constant, = c, the speed of light in vacuo), and ...
* double dwavnfreq
* (Returned) ... vice versa [s/m] (constant, = 1/c, always available).
*
* double dfreqvrad
* (Returned) Derivative of frequency with respect to radio velocity [/m],
* and ...
* double dvradfreq
* (Returned) ... vice versa [m] (wavetype && velotype).
*
* double dfreqwave
* (Returned) Derivative of frequency with respect to vacuum wavelength
* [/m/s], and ...
* double dwavefreq
* (Returned) ... vice versa [m s] (wavetype).
*
* double dfreqawav
* (Returned) Derivative of frequency with respect to air wavelength,
* [/m/s], and ...
* double dawavfreq
* (Returned) ... vice versa [m s] (wavetype).
*
* double dfreqvelo
* (Returned) Derivative of frequency with respect to relativistic
* velocity [/m], and ...
* double dvelofreq
* (Returned) ... vice versa [m] (wavetype && velotype).
*
* double dwavevopt
* (Returned) Derivative of vacuum wavelength with respect to optical
* velocity [s], and ...
* double dvoptwave
* (Returned) ... vice versa [/s] (wavetype && velotype).
*
* double dwavezopt
* (Returned) Derivative of vacuum wavelength with respect to redshift [m],
* and ...
* double dzoptwave
* (Returned) ... vice versa [/m] (wavetype && velotype).
*
* double dwaveawav
* (Returned) Derivative of vacuum wavelength with respect to air
* wavelength [dimensionless], and ...
* double dawavwave
* (Returned) ... vice versa [dimensionless] (wavetype).
*
* double dwavevelo
* (Returned) Derivative of vacuum wavelength with respect to relativistic
* velocity [s], and ...
* double dvelowave
* (Returned) ... vice versa [/s] (wavetype && velotype).
*
* double dawavvelo
* (Returned) Derivative of air wavelength with respect to relativistic
* velocity [s], and ...
* double dveloawav
* (Returned) ... vice versa [/s] (wavetype && velotype).
*
* double dvelobeta
* (Returned) Derivative of relativistic velocity with respect to
* relativistic beta [m/s] (constant, = c, the speed of light in vacuo),
* and ...
* double dbetavelo
* (Returned) ... vice versa [s/m] (constant, = 1/c, always available).
*
* struct wcserr *err
* (Returned) If enabled, when an error status is returned, this struct
* contains detailed information about the error, see wcserr_enable().
*
* void *padding
* (An unused variable inserted for alignment purposes only.)
*
*
* Global variable: const char *spx_errmsg[] - Status return messages
* ------------------------------------------------------------------
* Error messages to match the status value returned from each function.
*
*===========================================================================*/
#ifndef WCSLIB_SPEC
#define WCSLIB_SPEC
#ifdef __cplusplus
extern "C" {
#endif
extern const char *spx_errmsg[];
enum spx_errmsg {
SPXERR_SUCCESS = 0, // Success.
SPXERR_NULL_POINTER = 1, // Null spxprm pointer passed.
SPXERR_BAD_SPEC_PARAMS = 2, // Invalid spectral parameters.
SPXERR_BAD_SPEC_VAR = 3, // Invalid spectral variable.
SPXERR_BAD_INSPEC_COORD = 4 // One or more of the inspec coordinates were
// invalid.
};
struct spxprm {
double restfrq, restwav; // Rest frequency [Hz] and wavelength [m].
int wavetype, velotype; // True if wave/velocity types have been
// computed; types are defined below.
// Spectral variables computed by specx().
//--------------------------------------------------------------------------
double freq, // wavetype: Frequency [Hz].
afrq, // wavetype: Angular frequency [rad/s].
ener, // wavetype: Photon energy [J].
wavn, // wavetype: Wave number [/m].
vrad, // velotype: Radio velocity [m/s].
wave, // wavetype: Vacuum wavelength [m].
vopt, // velotype: Optical velocity [m/s].
zopt, // velotype: Redshift.
awav, // wavetype: Air wavelength [m].
velo, // velotype: Relativistic velocity [m/s].
beta; // velotype: Relativistic beta.
// Derivatives of spectral variables computed by specx().
//--------------------------------------------------------------------------
double dfreqafrq, dafrqfreq, // Constant, always available.
dfreqener, denerfreq, // Constant, always available.
dfreqwavn, dwavnfreq, // Constant, always available.
dfreqvrad, dvradfreq, // wavetype && velotype.
dfreqwave, dwavefreq, // wavetype.
dfreqawav, dawavfreq, // wavetype.
dfreqvelo, dvelofreq, // wavetype && velotype.
dwavevopt, dvoptwave, // wavetype && velotype.
dwavezopt, dzoptwave, // wavetype && velotype.
dwaveawav, dawavwave, // wavetype.
dwavevelo, dvelowave, // wavetype && velotype.
dawavvelo, dveloawav, // wavetype && velotype.
dvelobeta, dbetavelo; // Constant, always available.
// Error handling
//--------------------------------------------------------------------------
struct wcserr *err;
// Private
//--------------------------------------------------------------------------
void *padding; // (Dummy inserted for alignment purposes.)
};
// Size of the spxprm struct in int units, used by the Fortran wrappers.
#define SPXLEN (sizeof(struct spxprm)/sizeof(int))
int specx(const char *type, double spec, double restfrq, double restwav,
struct spxprm *specs);
int spxperr(const struct spxprm *spx, const char *prefix);
// For use in declaring function prototypes, e.g. in spcprm.
#define SPX_ARGS double param, int nspec, int instep, int outstep, \
const double inspec[], double outspec[], int stat[]
int freqafrq(SPX_ARGS);
int afrqfreq(SPX_ARGS);
int freqener(SPX_ARGS);
int enerfreq(SPX_ARGS);
int freqwavn(SPX_ARGS);
int wavnfreq(SPX_ARGS);
int freqwave(SPX_ARGS);
int wavefreq(SPX_ARGS);
int freqawav(SPX_ARGS);
int awavfreq(SPX_ARGS);
int waveawav(SPX_ARGS);
int awavwave(SPX_ARGS);
int velobeta(SPX_ARGS);
int betavelo(SPX_ARGS);
int freqvelo(SPX_ARGS);
int velofreq(SPX_ARGS);
int freqvrad(SPX_ARGS);
int vradfreq(SPX_ARGS);
int wavevelo(SPX_ARGS);
int velowave(SPX_ARGS);
int awavvelo(SPX_ARGS);
int veloawav(SPX_ARGS);
int wavevopt(SPX_ARGS);
int voptwave(SPX_ARGS);
int wavezopt(SPX_ARGS);
int zoptwave(SPX_ARGS);
#ifdef __cplusplus
}
#endif
#endif // WCSLIB_SPEC
wavevelo
int wavevelo(SPX_ARGS)
Conversions between wavelength and velocity types (vector).
betavelo
int betavelo(SPX_ARGS)
Convert relativistic beta to relativistic velocity (vector).
awavfreq
int awavfreq(SPX_ARGS)
Convert air wavelength to frequency (vector).
specx
int specx(const char *type, double spec, double restfrq, double restwav, struct spxprm *specs)
Spectral cross conversions (scalar).
freqawav
int freqawav(SPX_ARGS)
Convert frequency to air wavelength (vector).
awavwave
int awavwave(SPX_ARGS)
Convert air wavelength to vacuum wavelength (vector).
spxperr
int spxperr(const struct spxprm *spx, const char *prefix)
Print error messages from a spxprm struct.
freqwave
int freqwave(SPX_ARGS)
Convert frequency to vacuum wavelength (vector).
wavezopt
int wavezopt(SPX_ARGS)
Convert vacuum wavelength to redshift (vector).
veloawav
int veloawav(SPX_ARGS)
Convert relativistic velocity to air wavelength (vector).
waveawav
int waveawav(SPX_ARGS)
Convert vacuum wavelength to air wavelength (vector).
freqener
int freqener(SPX_ARGS)
Convert frequency to photon energy (vector).
wavnfreq
int wavnfreq(SPX_ARGS)
Convert wave number to frequency (vector).
wavevopt
int wavevopt(SPX_ARGS)
Convert vacuum wavelength to optical velocity (vector).
wavefreq
int wavefreq(SPX_ARGS)
Convert vacuum wavelength to frequency (vector).
freqafrq
int freqafrq(SPX_ARGS)
Convert frequency to angular frequency (vector).
vradfreq
int vradfreq(SPX_ARGS)
Convert radio velocity to frequency (vector).
SPX_ARGS
#define SPX_ARGS
For use in declaring spectral conversion function prototypes.
Definition spx.h:541
enerfreq
int enerfreq(SPX_ARGS)
Convert photon energy to frequency (vector).
velobeta
int velobeta(SPX_ARGS)
Convert relativistic velocity to relativistic beta (vector).
velofreq
int velofreq(SPX_ARGS)
Convert relativistic velocity to frequency (vector).
freqwavn
int freqwavn(SPX_ARGS)
Convert frequency to wave number (vector).
freqvelo
int freqvelo(SPX_ARGS)
Convert frequency to relativistic velocity (vector).
voptwave
int voptwave(SPX_ARGS)
Convert optical velocity to vacuum wavelength (vector).
velowave
int velowave(SPX_ARGS)
Convert relativistic velocity to vacuum wavelength (vector).
afrqfreq
int afrqfreq(SPX_ARGS)
Convert angular frequency to frequency (vector).
spx_errmsg
spx_errmsg
Status return messages.
Definition spx.h:477
SPXERR_BAD_SPEC_PARAMS
@ SPXERR_BAD_SPEC_PARAMS
Definition spx.h:480
SPXERR_SUCCESS
@ SPXERR_SUCCESS
Definition spx.h:478
SPXERR_BAD_SPEC_VAR
@ SPXERR_BAD_SPEC_VAR
Definition spx.h:481
SPXERR_NULL_POINTER
@ SPXERR_NULL_POINTER
Definition spx.h:479
SPXERR_BAD_INSPEC_COORD
@ SPXERR_BAD_INSPEC_COORD
Definition spx.h:482
zoptwave
int zoptwave(SPX_ARGS)
Convert redshift to vacuum wavelength (vector).
freqvrad
int freqvrad(SPX_ARGS)
Convert frequency to radio velocity (vector).
awavvelo
int awavvelo(SPX_ARGS)
Convert air wavelength to relativistic velocity (vector).
spxprm
Spectral variables and their derivatives.
Definition spx.h:486
spxprm::dvelobeta
double dvelobeta
Definition spx.h:520
spxprm::vopt
double vopt
Definition spx.h:500
spxprm::dvradfreq
double dvradfreq
Definition spx.h:511
spxprm::dwavezopt
double dwavezopt
Definition spx.h:516
spxprm::dfreqvelo
double dfreqvelo
Definition spx.h:514
spxprm::wavetype
int wavetype
Definition spx.h:489
spxprm::denerfreq
double denerfreq
Definition spx.h:509
spxprm::dwavevopt
double dwavevopt
Definition spx.h:515
spxprm::dwavnfreq
double dwavnfreq
Definition spx.h:510
spxprm::vrad
double vrad
Definition spx.h:498
spxprm::velo
double velo
Definition spx.h:503
spxprm::restfrq
double restfrq
Definition spx.h:487
spxprm::dveloawav
double dveloawav
Definition spx.h:519
spxprm::afrq
double afrq
Definition spx.h:495
spxprm::dvelofreq
double dvelofreq
Definition spx.h:514
spxprm::dafrqfreq
double dafrqfreq
Definition spx.h:508
spxprm::beta
double beta
Definition spx.h:504
spxprm::dvoptwave
double dvoptwave
Definition spx.h:515
spxprm::dwavevelo
double dwavevelo
Definition spx.h:518
spxprm::dawavwave
double dawavwave
Definition spx.h:517
spxprm::wave
double wave
Definition spx.h:499
spxprm::dawavvelo
double dawavvelo
Definition spx.h:519
spxprm::dzoptwave
double dzoptwave
Definition spx.h:516
spxprm::dwavefreq
double dwavefreq
Definition spx.h:512
spxprm::zopt
double zopt
Definition spx.h:501
spxprm::dfreqvrad
double dfreqvrad
Definition spx.h:511
spxprm::dfreqwave
double dfreqwave
Definition spx.h:512
spxprm::wavn
double wavn
Definition spx.h:497
spxprm::dfreqener
double dfreqener
Definition spx.h:509
spxprm::dfreqawav
double dfreqawav
Definition spx.h:513
spxprm::dfreqafrq
double dfreqafrq
Definition spx.h:508
spxprm::ener
double ener
Definition spx.h:496
spxprm::dfreqwavn
double dfreqwavn
Definition spx.h:510
spxprm::padding
void * padding
Definition spx.h:528
spxprm::dawavfreq
double dawavfreq
Definition spx.h:513
spxprm::dbetavelo
double dbetavelo
Definition spx.h:520
spxprm::dvelowave
double dvelowave
Definition spx.h:518
spxprm::restwav
double restwav
Definition spx.h:487
spxprm::velotype
int velotype
Definition spx.h:489
spxprm::err
struct wcserr * err
Definition spx.h:524
spxprm::awav
double awav
Definition spx.h:502
spxprm::dwaveawav
double dwaveawav
Definition spx.h:517
spxprm::freq
double freq
Definition spx.h:494
wcserr
Error message handling.
Definition wcserr.h:243