Flare Irradiance Spectral Model (FISM): Flare component algorithms and results

By P. Chamberlin, T. Woods, F. Eparvier. 2008

176 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Atmospheric Science

View Paper: https://www.semanticscholar.org/paper/9c2fe69d3603911df2189a25e173ac304a73fc0b

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In Astronomy and Astrophysics

1. Liying Qian
2. P. Chamberlin
3. T. Woods
4. S. Solomon
5. Han-Li Liu
6. F. Eparvier
7. A. Burns
8. N. Pedatella

In Atmospheric Science

1. Liying Qian
2. P. Chamberlin
3. T. Woods
4. S. Solomon
5. Han-Li Liu
6. F. Eparvier
7. N. Pedatella
8. R. Roble

Citations in the corpus

• How Hospitable Are Space Weather Affected Habitable Zones? The Role of Ion Escape (2017, unknown): “The Vacuum Ultraviolet ( VUV ) contribution of the total radiative output is obtained by implementing the Flare Irradiance Spectral Model ( FISM; Chamberlin et al. 2008 ) , which represents an empirical model developed for space weather applications that estimates the solar irradiance at wavelengths”
• Variability of thermosphere and ionosphere responses to solar flares (2011, methodology): “7 as inputs, to estimate the solar XUV and EUV irradiances at wavelengths from 0.1 to 190 nm at 1 nm resolution with a temporal resolution of 60 s [Chamberlin et al., 2007, 2008].”
• GLOBAL ENERGETICS OF THIRTY-EIGHT LARGE SOLAR ERUPTIVE EVENTS (2012, methodology): “It should be emphasized that the plotted bolometric radiated energies are, with the exception of the five events noted in Table 1, not directly measured but rather estimates made using the FISM model (Chamberlin et al. 2007, 2008), and the magnetic energy is only good to an order of magnitude.”
• NEW SOLAR EXTREME-ULTRAVIOLET IRRADIANCE OBSERVATIONS DURING FLARES (2011, methodology): “…measurements only capture the flare’s main components well, current empirical flare-irradiance models, such as Flare Irradiance Spectral Model (FISM; Chamberlin et al. 2008) and Solar Irradiance Platform (SIP; Tobiska et al. 2000) that use the emission measured by the X-ray as a flare proxy, are…”
• Mars Global Ionosphere‐Thermosphere Model: Solar cycle, seasonal, and diurnal variations of the Mars upper atmosphere (2015, methodology): “…M-GITM is capable of using Earth-based data from the Solar Extreme Ultraviolet Experiment [Woods et al., 2005] or EUV Variability Explorer (EVE) [Woods et al., 2010] instruments as well as model results from the Flare Irradiance Spectral Model [Chamberlin et al., 2008] to drive the EUV heating.”
• Development and Validation of the Whole Atmosphere Community Climate Model With Thermosphere and Ionosphere Extension (WACCM‐X 2.0) (2018, methodology): “Solar spectra estimated by the Flare Irradiance Spectral Model (FISM; Chamberlin et al., 2007, 2008) are used as the default solar flare spectra input in the current version (cf., Qian et al., 2010).”
• Extreme Ultraviolet Variability Experiment (EVE) on the Solar Dynamics Observatory (SDO): Overview of Science Objectives, Instrument Design, Data Products, and Model Developments (2010, methodology): “FISM Model 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 one-minute time cadence (Chamberlin, Woods, and Eparvier, 2007, 2008).”