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Mesospheric dynamical changes induced by the solar proton events in October–November 2003
Author(s) -
Jackman Charles H.,
Roble Raymond G.,
Fleming Eric L.
Publication year - 2007
Publication title -
geophysical research letters
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.007
H-Index - 273
eISSN - 1944-8007
pISSN - 0094-8276
DOI - 10.1029/2006gl028328
Subject(s) - thermosphere , mesosphere , atmospheric sciences , proton , solar maximum , physics , mesopause , ozone , solar wind , meridional flow , storm , zonal and meridional , environmental science , solar cycle , ionosphere , stratosphere , meteorology , geophysics , plasma , quantum mechanics
The Thermosphere Ionosphere Mesosphere Electrodynamic General Circulation Model (TIME‐GCM) was used to study the atmospheric dynamical influence of the solar protons that occurred in Oct–Nov 2003, the fourth largest period of solar proton events (SPEs) measured in the past 40 years. The highly energetic solar protons produced odd hydrogen (HO x ) and odd nitrogen (NO y ). Significant short‐lived ozone decreases (10–70%) followed these enhancements of HO x and NO y and led to a cooling of most of the lower mesosphere. Temperature changes up to ±2.6 K were computed as well as wind (zonal, meridional, vertical) perturbations up to 20–25% of the background winds as a result of the solar protons. The solar proton‐induced mesospheric temperature and wind perturbations diminished over a period of 4–6 weeks after the SPEs. The Joule heating in the mesosphere, induced by the solar protons, was computed to be relatively insignificant for these solar storms.