Solar extreme‐ultraviolet irradiance for general circulation models

By S. Solomon, Liying Qian. 2005

301 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Atmospheric Science

View Paper: https://www.semanticscholar.org/paper/8040f3431951089f2abc265f172d3b0140b02442

How researchers see this paper

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

In Astronomy and Astrophysics

In Atmospheric Science

Citations in the corpus

Composition changes after the "Halloween" solar proton event: the High Energy Particle Precipitation in the Atmosphere (HEPPA) model versus MIPAS data intercomparison study (2011, methodology): “Photochemistry involves 7 ionizing and dissociating reactions through solar irradiance of wavelengths shorter than Lyman-alpha using a parametrization of Solomon and Qian (2005) and observed solar spectral irradiance.”
Causes of low thermospheric density during the 2007–2009 solar minimum (2011, methodology): “extended below 5 nm as described by Solomon and Qian [2005] .”
Variability of thermosphere and ionosphere responses to solar flares (2011, methodology): “However, for the XUV and EUV, the TIE‐GCM and TIME‐GCM use the same solar energy deposition scheme [Solomon and Qian, 2005], and photoionization is calculated for the altitude above ∼97 km for both the TIME‐GCM and the TIE‐GCM.”
Extreme Ultraviolet Variability Experiment (EVE) on the Solar Dynamics Observatory (SDO): Overview of Science Objectives, Instrument Design, Data Products, and Model Developments (2010, methodology): “…the band definitions for the PROBA2/Large Yield Radiometer (LYRA) instrument (Hochedez et al., 2006), the EUVAC solar irradiance model (Richards, Fennelly, and Torr, 1994), JB2006 and JB2008 atmospheric models (Bowman et al., 2008a, 2008b), and TIM-GCM model solar input (Solomon and Qian, 2005).”
Hydrodynamic planetary thermosphere model: 1. Response of the Earth's thermosphere to extreme solar EUV conditions and the significance of adiabatic cooling (2008, methodology): “The spectra at X-ray and EUV wavelengths ( 105 nm) are from a low-resolution EUVAC model [Solomon and Qian, 2005].”
Simulation of secular trends in the middle atmosphere, 1950–2003 (2007, background): “7) following Solomon and Qian [2005] for wavelengths shortward of Lyman a, and Woods and Rottman [2002] for wavelengths between Lyman a and 350 nm.”
The Whole Atmosphere Community Climate Model Version 6 (WACCM6) (2019, methodology): “For photoionization and heating rates at wavelengths shorter than Lyman-�, WACCM6 uses the parameterization of Solomon and Qian (2005), that takes as input the F10.”
Development and Validation of the Whole Atmosphere Community Climate Model With Thermosphere and Ionosphere Extension (WACCM‐X 2.0) (2018, background): “…and Heating The solar extreme-ultraviolet (EUV) variability and energy deposition scheme, including photoelectron effects, is described in Solomon and Qian (2005), and is essentially unchanged from earlier versions of WACCM and WACCM-X, except for a correction to the molecular oxygen…”