SAO2010

Implements the SAO2010 solar spectrum reported by Chance & Kurucz in 2010. The spectrum is a high quality. high resolution solar spectrum going from 200 nm to 1 micron at 0.01 nm spacing and a resolution of 0.04 nm FWHM.

Example

import sasktranif.sasktranif as skif
sun = skif.ISKSolarSpectrum('SAO2010')

References

K. Chance and R.L. Kurucz, “An improved high-resolution solar reference spectrum for earth’s atmosphere measurements in the ultraviolet, visible, and near infrared “, Journal of Quantitative Spectroscopy and Radiative Transfer, 111, 9, pp. 1289-1295, 2010, doi: 10.1016/j.jqsrt.2010.01.036, url = http://www.sciencedirect.com/science/article/pii/S0022407310000610

FONTELA_UVIS_3MICRON

Implements the solar spectrum presented by Fontela et al 2001. We use the 200 nm to 3 micron table at 0.02 nm spacing with 0.1 nm resolution., file -> NUVisIr3irrad1001Lowion00.conv1a.fits.

Example

import sasktranif.sasktranif as skif
sun = skif.ISKSolarSpectrum('FONTELA_UVIS_3MICRON')

References

Fontenla, J. M., Harder, J., Livingston, W., Snow, M. and Woods, T. “High-resolution solar spectral irradiance from extreme ultraviolet to far infrared”, Journal of Geophysical Research: Atmospheres, 116, D20, pp 2156-2202, 2011 doi: 10.1029/2011JD016032, url: http://dx.doi.org/10.1029/2011JD016032

FONTELA_UVIS_100MICRON

Implements the solar spectrum presented by Fontela et al 2001. We use the 200 nm to 100 micron table at 0.2 nm spacing with 1 nm resolution., file -> NUVisIr100irrad1001Lowion00.conv1nm.fits.

Example

import sasktranif.sasktranif as skif
sun = skif.ISKSolarSpectrum('FONTELA_UVIS_100MICRON')

References

Fontenla, J. M., Harder, J., Livingston, W., Snow, M. and Woods, T. “High-resolution solar spectral irradiance from extreme ultraviolet to far infrared”, Journal of Geophysical Research: Atmospheres, 116, D20, pp 2156-2202, 2011 doi: 10.1029/2011JD016032, url: http://dx.doi.org/10.1029/2011JD016032