Classes
struct	mx::astro::basicSpectrum< _units >
	A basic spectrum. More...

struct	mx::astro::astroFilter< _units, _rsr >
	A spectrum from the astroFilt filter library. More...

struct	mx::astro::sqWaveFilter< _units, _rsr >
	A square-wave filter spectrum. More...

struct	mx::astro::calspecSpectrum< _units >
	A spectrum from the HST calspec library. More...

struct	mx::astro::picklesSpectrum< _units >
	A spectrum from the Pickles library. More...

struct	mx::astro::earthAlbedo< _units >
	Earth Albedo Spectra. More...

struct	mx::astro::venusAlbedo< _units >
	Venus Spectra. More...

struct	mx::astro::cahoySpectrumRaw< _units >
	An albedo spectrum directly from the Cahoy et al (2010) [2] grid. More...

struct	mx::astro::phoenixSpectrum< _units >
	A spectrum from the Phoenix model, for use with ioutils::astro::astroSpectrum. More...

Functions
template<typename floatT >
void	mx::astro::rewritePhoenixSpectrum (const std::string &filename, floatT lmin, floatT lmax, int sepWavelength=0, floatT DF=-8.0)
	Read in, crop, scale, and re-write a Phoenix spectrum data file. More...

Function Documentation

◆ rewritePhoenixSpectrum()

template<typename floatT >

void mx::astro::rewritePhoenixSpectrum	(	const std::string &	filename,
		floatT	lmin,
		floatT	lmax,
		int	sepWavelength = `0`,
		floatT	DF = `-8.0`
	)

Read in, crop, scale, and re-write a Phoenix spectrum data file.

For working with spectra obtained from: http://perso.ens-lyon.fr/france.allard/

The Phoenix spectra contain many columns of line data which are not often used, are not necessarily sorted by wavelength, and are sometimes formated so that points with leading minus signs are not in a separate column. We also have to change the fortan D to e.

We also want to apply the dilution factor and take the power of 10.

This function deals with these issues, producing a two-column space-delimited file in a specified wavelength range.

References:

NOTE: This overwrites the input file!

Template Parameters

floatT the floating point type in which to work

Parameters

	filename	[in.out] complete name of the file to rewrite
[in]	lmin	minimum wavelength to rewrite [microns]
[in]	lmax	maximum wavelemngth to rewrite [microns]
[in]	sepWavelength	[optional] controls how wavelength is handled. 0=> wavelength is included in file as first column. 1=> wavelength is written to a separate 'wavelength.dat' file. -1=> means don't write wavelength.
[in]	DF	[optional] the dilution factor. See references.

Definition at line 96 of file phoenixSpectrum.hpp.

References mx::ioutils::parentPath(), and mx::math::vectorSortOrder().

Classes

Functions

Function Documentation

◆ rewritePhoenixSpectrum()