Astronomy and Astrophysics – Astrophysics
Scientific paper
Aug 2008
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008jgra..11308307s&link_type=abstract
Journal of Geophysical Research, Volume 113, Issue A8, CiteID A08307
Astronomy and Astrophysics
Astrophysics
2
Ionosphere: Ionospheric Disturbances, Ionosphere: Plasma Temperature And Density, Ionosphere: Midlatitude Ionosphere, Ionosphere: Solar Radiation And Cosmic Ray Effects, Solar Physics, Astrophysics, And Astronomy: Flares
Scientific paper
Global ionospheric models typically rely on parameterizations to account for heating of the plasma by photoelectrons. We compare the most commonly used parameterization to a rigorous photoelectron model and find the parameterization under-predicts the thermal electron volume heating rate by 20-30% under nominal solar conditions. When applied to a large solar flare, the parameterized heating rate is more than an order of magnitude smaller than the peak rate calculated with the physical model. To remedy this, we develop a new parameterization of electron heating that eliminates these differences; the resulting heating rates are within 5-15% of the physical model for nominal and solar flare conditions. The new algorithm is incorporated into a 1-D Global Average Ionosphere/Thermosphere (GAIT) model and used to investigate the response to the X17 flare of 28 October 2003. Electron temperatures calculated with the new parameterization are up to 10% higher prior to the flare, and 15% higher at the flare peak. The revised parameterization also leads to a 2% increase in neutral exospheric temperatures in the coupled model. The flare response of the global-average thermosphere is described and found to be similar to the satellite drag results reported by Sutton et al.
Smithtro Christopher G.
Solomon Stanley C.
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