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

By P. Chamberlin, T. Woods, F. Eparvier. 2007

172 citations recorded by the source corpus.

Subfields: Artificial Intelligence, Astronomy and Astrophysics

View Paper: https://www.semanticscholar.org/paper/cf8a5ffd5972e96fffe39ce901f11fb05537ceee

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Artificial Intelligence

1. P. Chamberlin
2. F. Eparvier
3. T. Woods
4. Liying Qian
5. S. Solomon
6. J. Lean
7. S. Solanki
8. N. Krivova

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

Citations in the corpus

• 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.”
• Flare Irradiance Spectral Model (FISM): Flare component algorithms and results (2008, methodology): “This atmospheric expansion then leads to increased density at a given altitude, increasing the drag on satellites that are in low Earth orbit [Chamberlin et al., 2007].”
• Variability of thermosphere and ionosphere responses to solar flares (2011, methodology): “Flare spectra estimated by the Flare Irradiance Spectral Model (FISM) [Chamberlin et al., 2007, 2008] are used as solar input to the TIME‐GCM for these flare simulations.”
• Extreme Ultraviolet Variability Experiment (EVE) on the Solar Dynamics Observatory (SDO): Overview of Science Objectives, Instrument Design, Data Products, and Model Developments (2010, background): “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).”
• Mars Global Ionosphere‐Thermosphere Model: Solar cycle, seasonal, and diurnal variations of the Mars upper atmosphere (2015, methodology): “Additionally, 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”
• 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).”