The SOLAR2000 empirical solar irradiance model and forecast tool

By W. Tobiska, Tom Woods, F. Eparvier, R. Viereck, Linton Floyd, D. Bouwer, G. Rottman, O. White. 2000

459 citations recorded by the source corpus.

Subfields: Artificial Intelligence, Astronomy and Astrophysics, Atmospheric Science

View Paper: https://www.semanticscholar.org/paper/59cec4d79439efab137f0b4c1ee91afaa6963e04

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. J. Lean
6. S. Solomon
7. G. Rottman
8. D. Webb

In Astronomy and Astrophysics

1. T. Woods
2. P. Chamberlin
3. Liying Qian
4. S. Solomon
5. F. Eparvier
6. J. Lean
7. L. Didkovsky
8. R. Viereck

In Atmospheric Science

1. P. Chamberlin
2. T. Woods
3. Liying Qian
4. S. Solomon
5. F. Eparvier
6. J. Lean
7. Erdal Yiğit
8. R. Viereck

Citations in the corpus

• NEW SOLAR EXTREME-ULTRAVIOLET IRRADIANCE OBSERVATIONS DURING FLARES (2011, background): “…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 improperly estimating the total flare energy.”
• Modeling the effects of gravity wave momentum deposition on the general circulation above the turbopause (2009, methodology): “Thermospheric heating, photodissociation, and photoionization are calculated for the absorption of solar X rays, extreme ultraviolet (EUV), and UV radiation between 1.8 and 184 nm using the SOLAR2000 empirical model of Tobiska et al. [2000] .”
• The convergence of magnetospheric energy flux in the polar atmosphere (2004, background): “The net energy !ux shortward of 200 nm is ∼ 4 orders of magnitude less than at visible wavelengths (e.g., Tobiska et al., 2000), but the !ux convergence at these wavelengths maximizes between 80 and 200 km altitude.”
• Flare Irradiance Spectral Model (FISM): Daily component algorithms and results (2007, methodology): “26 model [Tobiska et al. 2000; Tobiska, 2004], and the NRLEUV model [Warren et al., 1998, 2001; Lean et al., 2003].”
• High Accuracy Satellite Drag Model (HASDM) (2002, methodology): “This model was developed by Space Environment Technologies Inc. for the Space Environment Center and other agencies (Tobiska et al., 2000).”
• Solar extreme‐ultraviolet irradiance for general circulation models (2005, methodology): “These data form the basis for many of the reference spectra and empirical models used in thermosphere/ionosphere research over the intervening years [e.g., Donnelly, 1976; Hinteregger et al., 1981; Richards et al., 1994; Tobiska et al., 2000;Woods and Rottman, 2002].”
• Does the F10.7 index correctly describe solar EUV flux during the deep solar minimum of 2007-2009? (2011, background): “Therefore, different indices were put forward to describe the variations of solar EUV irradiance [e.g., Floyd et al., 2005; Lean et al., 2001; Liu et al., 2006]; and on the basis of these indices, solar EUV irradiance models, such as the EUVAC model [Richards et al., 1994], the SOLAR2000 model [ Tob”
• Diurnal variation of ozone depletion during the October-November 2003 solar proton events (2005, methodology): “[12] The solar flux is estimated by the SOLAR2000 model [ Tobiska et al., 2000 ], version 2.23.”
• Extreme Ultraviolet Variability Experiment (EVE) on the Solar Dynamics Observatory (SDO): Overview of Science Objectives, Instrument Design, Data Products, and Model Developments (2010, methodology): “…EVE data will be used to improve, validate, or constrain solar irradiance models, such as SIP (Tobiska, 2004, 2008; Tobiska and Bouwer, 2006; Tobiska et al., 2000), and atmospheric models, such as CTIPe (Fuller-Rowell et al., 1996), Global Assimilation of Ionospheric Measurements (GAIM;…”
• Solar activity variations of nighttime ionospheric peak electron density (2006, background): “…of the upper atmosphere by solar X-ray and extreme ultraviolet (EUV) radiations of wavelengths less than 1026 Å [Adler et al., 1997], which are known to have different period variations, especially the well-known solar cycle variations [Kane, 1992, 2003; Lean et al., 2001; Tobiska et al., 2000].”
• Solar EUV Experiment (SEE): Mission overview and first results (2005, methodology): “W. K. Tobiska has developed several proxy models of the solar EUV irradiance: SERF 2 by Tobiska and Barth [1990], EUV91 by Tobiska [1991], EUV97 by Tobiska and Eparvier [1998], and the latest version, SOLAR2000, by Tobiska et al. [2000] .”
• Flare Irradiance Spectral Model (FISM): Flare component algorithms and results (2008, methodology): “…model [Hinteregger et al., 1981], the EUVAC model [Richards et al., 1994, 2006], the Solar Irradiance Platform v2_30_63 (formerly SOLAR2000) model [Tobiska et al., 2000; Tobiska, 2004], VUV2002 [Woods and Rottman, 2002], the NRLEUV model [Warren et al., 1998, 2001; Lean et al., 2003] and a model…”