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#ifndef XSPECT_H
#define XSPECT_H
/*
* Author: Graeme W. Gill
* Date: 21/6/01
* Version: 1.00
*
* Copyright 2000 - 2010 Graeme W. Gill
* All rights reserved.
*
* This material is licenced under the GNU GENERAL PUBLIC LICENSE Version 2 or later :-
* see the License2.txt file for licencing details.
*/
/*
* This class supports converting spectral samples
* into CIE XYZ or D50 Lab tristimulous values.
*/
/*
* TTBD:
*
*/
#ifndef SALONEINSTLIB
#include "icc.h" /* icclib ICC definitions */
#else /* SALONEINSTLIB */
#include "conv.h" /* fake icclib ICC definitions */
#endif /* SALONEINSTLIB */
#ifdef __cplusplus
extern "C" {
#endif
/* ------------------------------------------------------------------------------ */
/* Structure for conveying spectral information */
/* NOTE :- should ditch norm, and replace it by */
/* "units", ie. reflectance/transmittance 0..1, 0..100%, */
/* W/nm/m^2 or mW/nm/m^2 */
#define XSPECT_MAX_BANDS 601 /* Enought for 1nm from 300 to 900 */
typedef struct {
int spec_n; /* Number of spectral bands, 0 if not valid */
double spec_wl_short; /* First reading wavelength in nm (shortest) */
double spec_wl_long; /* Last reading wavelength in nm (longest) */
double norm; /* Normalising scale value */
double spec[XSPECT_MAX_BANDS]; /* Spectral value, shortest to longest */
} xspect;
/* Some helpful macro's: */
/* Copy everything except the spectral values */
#define XSPECT_COPY_INFO(PDST, PSRC) \
(PDST)->spec_n = (PSRC)->spec_n, \
(PDST)->spec_wl_short = (PSRC)->spec_wl_short, \
(PDST)->spec_wl_long = (PSRC)->spec_wl_long, \
(PDST)->norm = (PSRC)->norm
/* Given an index and the sampling ranges, compute the sample wavelength */
#define XSPECT_WL(SHORT, LONG, N, IX) \
((SHORT) + (double)(IX) * ((LONG) - (SHORT))/((N)-1.0))
/* Given the address of an xspect and an index, compute the sample wavelegth */
#define XSPECT_XWL(PXSP, IX) \
(((PXSP)->spec_wl_short) + (double)(IX) * (((PXSP)->spec_wl_long) - ((PXSP)->spec_wl_short))/(((PXSP)->spec_n)-1.0))
/* Given a wavelength and the sampling ranges, compute the double index */
#define XSPECT_DIX(SHORT, LONG, N, WL) \
(((N)-1.0) * ((WL) - (SHORT))/((LONG) - (SHORT)))
/* Given the wavelength and address of an xspect, compute the double index */
#define XSPECT_XDIX(PXSP, WL) \
(((PXSP)->spec_n-1.0) * ((WL) - ((PXSP)->spec_wl_short))/(((PXSP)->spec_wl_long) - ((PXSP)->spec_wl_short)))
/* Given a wavelength and the sampling ranges, compute the nearest index */
#define XSPECT_IX(SHORT, LONG, N, WL) \
((int)floor(XSPECT_DIX(SHORT, LONG, N, WL) + 0.5))
/* Given a wavelength and address of an xspect, compute the nearest index */
#define XSPECT_XIX(PXSP, WL) \
((int)floor(XSPECT_DIX(PXSP, WL) + 0.5))
#ifndef SALONEINSTLIB
/* Single spectrum utility functions. Return NZ if error */
int write_xspect(char *fname, xspect *s);
int read_xspect(xspect *sp, char *fname);
/* CMF utility functions. Return NZ if error */
int write_cmf(char *fname, xspect cmf[3]);
int read_cmf(xspect cmf[3], char *fname);
/* Save a set of nspec spectrum to a CGATS file. Return NZ if error */
/* type 0 = SPECT, 1 = CMF */
int write_nxspect(char *fname, xspect *sp, int nspec, int type);
/* Restore a set of up to nspec spectrum from a CGATS file. Return NZ if error */
/* type = any, 1 = SPECT, 2 = CMF, 3 = both */
int read_nxspect(xspect *sp, char *fname, int *nret, int off, int nspec, int type);
#endif /* !SALONEINSTLIB*/
/* Get interpolated value at wavelenth (not normalised) */
double value_xspect(xspect *sp, double wl);
/* De-normalize and set normalisation factor to 1.0 */
void xspect_denorm(xspect *sp);
#ifndef SALONEINSTLIB
/* Convert from one xspect type to another */
void xspect2xspect(xspect *dst, xspect *targ, xspect *src);
#endif /* !SALONEINSTLIB*/
/* ------------------------------------------------------------------------------ */
/* Class for converting between spectral and CIE */
/* We build in some useful spectra */
/* Type of illumination */
typedef enum {
icxIT_default = 0, /* Default illuminant (usually D50) */
icxIT_none = 1, /* No illuminant - self luminous spectrum */
icxIT_custom = 2, /* Custom illuminant spectrum */
icxIT_A = 3, /* Standard Illuminant A */
icxIT_C = 4, /* Standard Illuminant C */
icxIT_D50 = 5, /* Daylight 5000K */
icxIT_D50M2 = 6, /* Daylight 5000K, UV filtered (M2) */
icxIT_D65 = 7, /* Daylight 6500K */
icxIT_E = 8, /* Equal Energy */
#ifndef SALONEINSTLIB
icxIT_F5 = 9, /* Fluorescent, Standard, 6350K, CRI 72 */
icxIT_F8 = 10, /* Fluorescent, Broad Band 5000K, CRI 95 */
icxIT_F10 = 11, /* Fluorescent Narrow Band 5000K, CRI 81 */
icxIT_Spectrocam = 12, /* Spectrocam Xenon Lamp */
icxIT_Dtemp = 13, /* Daylight at specified temperature */
icxIT_Ptemp = 14 /* Planckian at specified temperature */
#endif /* !SALONEINSTLIB*/
} icxIllumeType;
/* Fill in an xpsect with a standard illuminant spectrum */
/* return 0 on sucecss, nz if not matched */
int standardIlluminant(
xspect *sp, /* Xspect to fill in */
icxIllumeType ilType, /* Type of illuminant */
double temp); /* Optional temperature in degrees kelvin, for Dtemp and Ptemp */
/* Given an emission spectrum, set the UV output to the given level. */
/* The shape of the UV is taken from FWA1_stim, and the level is */
/* with respect to the average of the input spectrum. */
void xsp_setUV(xspect *out, xspect *in, double uvlevel);
/* Type of observer */
typedef enum {
icxOT_default = 0, /* Default observer (usually CIE_1931_2) */
icxOT_none = 1, /* No observer - (don't compute XYZ) */
icxOT_custom = 2, /* Custom observer type weighting */
icxOT_CIE_1931_2 = 3, /* Standard CIE 1931 2 degree */
icxOT_CIE_1964_10 = 4, /* Standard CIE 1964 10 degree */
#ifndef SALONEINSTLIB
icxOT_Stiles_Burch_2 = 5, /* Stiles & Burch 1955 2 degree */
icxOT_Judd_Voss_2 = 6, /* Judd & Voss 1978 2 degree */
icxOT_CIE_1964_10c = 7, /* Standard CIE 1964 10 degree, 2 degree compatible */
icxOT_Shaw_Fairchild_2 = 8 /* Shaw & Fairchild 1997 2 degree */
#endif /* !SALONEINSTLIB*/
} icxObserverType;
/* Return pointers to three xpsects with a standard observer weighting curves */
/* return 0 on sucecss, nz if not matched */
int standardObserver(xspect *sp[3], icxObserverType obType);
/* Return a string describing the standard observer */
char *standardObserverDescription(icxObserverType obType);
/* Clamping state */
typedef enum {
icxNoClamp = 0, /* Don't clamp XYZ/Lab to +ve */
icxClamp = 1, /* Clamp XYZ/Lab to +ve */
} icxClamping;
/* The conversion object */
struct _xsp2cie {
/* Private: */
xspect illuminant; /* Lookup conversion/observer illuminant */
int isemis; /* nz if we are doing an emission conversion */
xspect observer[3];
int doLab; /* Return D50 Lab result */
icxClamping clamp; /* Clamp XYZ and Lab to be +ve */
#ifndef SALONEINSTLIB
/* FWA compensation */
double bw; /* Integration bandwidth */
xspect iillum; /* Y = 1 Normalised instrument illuminant spectrum */
xspect imedia; /* Instrument measured media */
xspect emits; /* Estimated FWA emmission spectrum */
xspect media; /* Estimated base media (ie. minus FWA) */
xspect tillum; /* Y = 1 Normalised target/simulated instrument illuminant spectrum */
xspect oillum; /* Y = 1 Normalised observer illuminant spectrum */
double Sm; /* FWA Stimulation level for emits contribution */
double FWAc; /* FWA content (informational) */
int insteqtarget; /* iillum == tillum, bypass FWA */
#endif /* !SALONEINSTLIB*/
/* Public: */
void (*del)(struct _xsp2cie *p);
/* Convert (and possibly fwa correct) reflectance spectrum */
/* Note that the input spectrum normalisation value is used. */
/* Note that the returned XYZ is 0..1 range for reflectanc. */
/* Emissive spectral values are assumed to be in mW/nm, and sampled */
/* rather than integrated if they are not at 1nm spacing. */
void (*convert) (struct _xsp2cie *p, /* this */
double *out, /* Return XYZ or D50 Lab value */
xspect *in /* Spectrum to be converted, normalised by norm */
);
/* Convert and also return (possibly corrected) reflectance spectrum */
/* Spectrum will be same wlength range and readings as input spectrum */
/* Note that the returned XYZ is 0..1 range for reflectanc. */
/* Emissive spectral values are assumed to be in mW/nm, and sampled */
/* rather than integrated if they are not at 1nm spacing. */
void (*sconvert) (struct _xsp2cie *p, /* this */
xspect *sout, /* Return corrected refl. spectrum (may be NULL) */
double *out, /* Return XYZ or D50 Lab value (may be NULL) */
xspect *in /* Spectrum to be converted, normalised by norm */
);
#ifndef SALONEINSTLIB
/* Set Media White. This enables extracting and applying the */
/* colorant reflectance value from/to the meadia. */
/* return NZ if error */
int (*set_mw) (struct _xsp2cie *p, /* this */
xspect *white /* Spectrum of plain media */
);
/* Set Fluorescent Whitening Agent compensation */
/* return NZ if error */
int (*set_fwa) (struct _xsp2cie *p, /* this */
xspect *iillum, /* Spectrum of instrument illuminant */
xspect *tillum, /* Spectrum of target/simulated instrument illuminant, */
/* NULL to use observer illuminant. */
xspect *white /* Spectrum of plain media */
);
/* Set FWA given updated conversion illuminant. */
/* (We assume that xsp2cie_set_fwa has been called first) */
/* return NZ if error */
int (*update_fwa_custillum) (struct _xsp2cie *p,
xspect *tillum, /* Spectrum of target/simulated instrument illuminant, */
/* NULL to use set_fwa() value. */
xspect *custIllum /* Spectrum of observer illuminant */
);
/* Get Fluorescent Whitening Agent compensation information */
/* return NZ if error */
void (*get_fwa_info) (struct _xsp2cie *p, /* this */
double *FWAc /* FWA content as a ratio. */
);
/* Extract the colorant reflectance value from the media. Takes FWA */
/* into account if set. Media white or FWA must be set. */
/* return NZ if error */
int (*extract) (struct _xsp2cie *p, /* this */
xspect *out, /* Extracted colorant refl. spectrum */
xspect *in /* Spectrum to be converted, normalised by norm */
);
/* Apply the colorant reflectance value from the media. Takes FWA */
/* into account if set. DOESN'T convert to FWA target illumination! */
/* FWA must be set. */
int (*apply) (struct _xsp2cie *p, /* this */
xspect *out, /* Applied refl. spectrum */
xspect *in /* Colorant reflectance to be applied */
);
#endif /* !SALONEINSTLIB*/
}; typedef struct _xsp2cie xsp2cie;
xsp2cie *new_xsp2cie(
icxIllumeType ilType, /* Observer Illuminant to use */
xspect *custIllum,
icxObserverType obType, /* Observer */
xspect custObserver[3],
icColorSpaceSignature rcs, /* Return color space, icSigXYZData or icSigLabData */
/* ** Must be icSigXYZData if SALONEINSTLIB ** */
icxClamping clamp /* NZ to clamp XYZ/Lab to be +ve */
);
#ifndef SALONEINSTLIB
/* --------------------------- */
/* Spectrum locus */
/* Return the spectrum locus range for the given observer. */
/* return 0 on sucecss, nz if observer not known */
int icx_spectrum_locus_range(double *min_wl, double *max_wl, icxObserverType obType);
/* Return an XYZ that is on the spectrum locus for the given observer. */
/* wl is the input wavelength in the range icx_spectrum_locus_range(), */
/* and return clipped result if outside this range. */
/* Return nz if observer unknown. */
int icx_spectrum_locus(double xyz[3], double in, icxObserverType obType);
/* Determine whether the given XYZ is outside the spectrum locus */
/* Return 0 if within locus */
/* Return 1 if outside locus */
/* Return 2 if unknown (bad observer) */
int icx_outside_spec_locus(double xyz[3], icxObserverType obType);
/* Return an aproximate RGB value for coloring within the spectrum locus */
void icx_spec_locus_color(double rgb[3], double xyz[3], icxObserverType obType);
/* --------------------------- */
/* Density and other functions */
/* Given a reflectance or transmition spectral product, */
/* return status T CMY + V density values */
void xsp_Tdensity(double *out, /* Return CMYV density */
xspect *in /* Spectral product to be converted */
);
/* Given a reflectance or transmission XYZ value, */
/* return approximate status T CMYV log10 density values */
void icx_XYZ2Tdens(
double *out, /* Return aproximate CMYV log10 density */
double *in /* Input XYZ values */
);
/* Given a reflectance or transmission XYZ value, */
/* return log10 XYZ density values */
void icx_XYZ2dens(
double *out, /* Return log10 XYZ density */
double *in /* Input XYZ values */
);
/* Given an XYZ value, */
/* return sRGB values */
void icx_XYZ2sRGB(
double *out, /* Return sRGB value */
double *wp, /* Input XYZ white point (may be NULL) */
double *in /* Input XYZ values */
);
/* Given an illuminant definition and an observer model, return */
/* the normalised XYZ value for that spectrum. */
/* Return 0 on sucess, 1 on error */
int icx_ill_sp2XYZ(
double xyz[3], /* Return XYZ value with Y == 1 */
icxObserverType obType, /* Observer */
xspect custObserver[3], /* Optional custom observer */
icxIllumeType ilType, /* Type of illuminant */
double ct, /* Input temperature in degrees K */
xspect *custIllum); /* Optional custom illuminant */
/* Given a choice of temperature dependent illuminant (icxIT_Dtemp or icxIT_Ptemp), */
/* return the closest correlated color temperature to the given spectrum or XYZ. */
/* An observer type can be chosen for interpretting the spectrum of the input and */
/* the illuminant. */
/* Note we're using CICDE94, rather than the traditional L*u*v* 2/3 space for CCT */
/* Return -1 on erorr */
double icx_XYZ2ill_ct(
double txyz[3], /* If not NULL, return the XYZ of the black body temperature */
icxIllumeType ilType, /* Type of illuminant, icxIT_Dtemp or icxIT_Ptemp */
icxObserverType obType, /* Observer */
xspect custObserver[3], /* Optional custom observer */
double xyz[3], /* Input XYZ value, NULL if spectrum intead */
xspect *insp0, /* Input spectrum value, NULL if xyz[] instead */
int viscct); /* nz to use visual CIEDE2000, 0 to use CCT CIE 1960 UCS. */
/* Compute the CIE1995 CRI: Ra */
/* Return < 0.0 on error */
/* If invalid is not NULL, set it to nz if CRI */
/* is invalid because the sample is not white enough. */
double icx_CIE1995_CRI(
int *invalid, /* if not NULL, set to nz if invalid */
xspect *sample /* Illuminant sample to compute CRI of */
);
#endif /* !SALONEINSTLIB*/
#ifdef __cplusplus
}
#endif
#endif /* XSPECTFM_H */
|