The Flare Irradiance Spectral Model (FISM) as an Operational Space Weather Product

Details The Flare Irradiance Spectral Model (FISM) as an Operational Space Weather Product The Flare Irradiance Spectral Model (FISM) as an Operational Space Weather Product

Dec 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006agufmsa53a1353c&link_type=abstract

American Geophysical Union, Fall Meeting 2006, abstract #SA53A-1353

Physics

7519 Flares, 7538 Solar Irradiance, 7549 Ultraviolet Emissions, 7900 Space Weather, 7959 Models

Scientific paper

The Flare Irradiance Spectral Model (FISM) is an empirical model of the solar irradiance spectrum from 0.1 to 190 nm at 1 nm spectral resolution and on a 1-minute time cadence. The goal of FISM is to provide accurate solar spectral irradiances over the vacuum ultraviolet (VUV: 0-200 nm) range as input for ionospheric and thermospheric models. The FISM spectra are currently available for historical studies. The FISM algorithms are currently being updated to provide solar VUV irradiance spectra near real-time with less than a 15-minute time lag in order to be used in operational space weather processing. Progress on these updated algorithms as well as near-term improvements to meet these operational goals will be discussed.

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