The influence of the several very large solar proton events in years 2000–2003 on the neutral middle atmosphere |
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| Institution: | 1. Code 916, Laboratory for Atmospheres, NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA;2. Science Systems and Applications, Inc., 10210 Greenbelt Road, Suite 400, Lanham, MD 20706, USA;3. Atmospheric and Environmental Research, Inc., 131 Hartwell Avenue, Lexington, MA 02421, USA;4. Mail Stop 401B, NASA Langley Research Center, Hampton, VA 23681, USA;5. Institute of Environmental Physics, University of Bremen, Germany;6. Hampton University, Center for Atmospheric Sciences, Hampton, VA 23668, USA |
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| Abstract: | Solar proton events (SPEs) are known to have caused changes in constituents in the Earth’s polar neutral middle atmosphere. The past four years, 2000–2003, have been replete with SPEs. Huge fluxes of high energy protons entered the Earth’s atmosphere in periods lasting 2–3 days in July and November 2000, September and November 2001 and October 2003. The highly energetic protons produce ionizations, excitations, dissociations and dissociative ionizations of the background constituents, which lead to the production of HOx (H, OH, HO2) and NOy (N, NO, NO2, NO3, N2O5, HNO3, HO2NO2, ClONO2, BrONO2). The HOx increases lead to short-lived ozone decreases in the polar mesosphere and upper stratosphere due to the short lifetimes of the HOx constituents. Large mesospheric ozone depletions (>70%) due to the HOx enhancements were observed and modeled as a result of the very large July 2000 SPE. The NOy increases lead to long-lived stratospheric ozone changes because of the long lifetime of the NOy family in this region. Polar total ozone depletions >1% were simulated in both hemispheres for extended periods of time (several months) as a result of the NOy enhancements due to the very large SPEs. |
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