Physics
Scientific paper
Dec 2004
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004agufmsa13b..02c&link_type=abstract
American Geophysical Union, Fall Meeting 2004, abstract #SA13B-02
Physics
7519 Flares, 7536 Solar Activity Cycle (2162), 7538 Solar Irradiance, 7549 Ultraviolet Emissions, 0358 Thermosphere: Energy Deposition
Scientific paper
The Flare Irradiance Spectral Model (FISM) is an empirical model of the solar irradiance spectrum from 0.1 to 195 nm at 1nm resolution and on a 1-minute time cadence. This model is based on the TIMED SEE data and uses the MgII core-to-wing ratio and GOES XRS data as proxies. FISM accounts for the significant irradiances changes due to solar flares, which includes orders of magnitude increases in the X-rays to factors of two increases in the EUV. The need for FISM arises due to the lack of solar irradiance measurements on minute time scales for the entire XUV and EUV spectral region, and currently available daily models and measurements do not represent or include the irradiance changes due to solar flares. Algorithms and current results from FISM will be discussed, as well as the future improvements that are planned for the model.
Chamberlin Phillip C.
Eparvier Francis G.
Woods Thomas N.
No associations
LandOfFree
Flare Irradiance Spectral Model (FISM): a Model of Solar Vacuum Ultraviolet Irradiance Over Time Scales From Flares to Solar Cycles does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Flare Irradiance Spectral Model (FISM): a Model of Solar Vacuum Ultraviolet Irradiance Over Time Scales From Flares to Solar Cycles, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Flare Irradiance Spectral Model (FISM): a Model of Solar Vacuum Ultraviolet Irradiance Over Time Scales From Flares to Solar Cycles will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1456570