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Northern Hemisphere Atmospheric Influence of the Solar Proton Events and Ground Level Enhancement in January 2005Solar eruptions in early 2005 led substantial barrage of charged particles on the Earth's atmosphere during the January 16-21 period. Proton fluxes were greatly increased during these several days and led to the production ofHO(x)(H, OH, BO2)and NO(x)(N, NO, NO2), which then caused the destruction of ozone. We focus on the Northern polar region, where satellite measurements and simulations with the Whole Atmosphere Community Climate Model (WACCM3) showed large enhancements in mesospheric HO(x) and NO(x) constituents, and associated ozone reductions, due 10 these solar proton events (SPEs). The WACCM3 simulations show enhanced short-lived OH throughout the mesosphere in the 60-82.5degN latitude band due to the SPEs for most days in the Jan.16-2l,2005 period, in reasonable agreement with the Aura Microwave Limb Sounder (MLS) measurements. Mesospheric HO2 is also predicted to be increased by the SPEs, however, the modeled HO2 results are somewhat larger than the MLS measurements. These HO(x) enhancements led to huge predicted and MLS-measured ozone decreases of greater than 40% throughout most of the Northern polar mesosphere during the SPE period. Envisat Michelson Interferometer for Passive Atmospheric Sounding (MIPAS) measurements of hydrogen peroxide (H2O2) show increases throughout the stratosphere with highest enhancements of about 60 ppt y in the lowermost mesosphere over the Jan. 16-18, 2005 period due to the solar protons. WACCM3 predictions indicate H2O2 enhancements over the same time period of more than twice that amount. Measurements of nitric acid (HNO3) by both MLS and MIPAS show an increase of about 1 ppbv above background levels in the upper stratosphere during January 16-29, 2005. WACCM3 simulations show only minuscule HNO3 changes in the upper stratosphere during this time period. However due to the small loss rates during winter, polar mesospheric enhancements of NO(x) are computed to be greater than 50 ppbv during the SPE period. Computed NO(x)increases, which were statistically significant at the 95% level, lasted about a month past the SPEs. The SCISAT-I Atmospheric Chemistry Experiment Fourier Transform Spectrometer (ACE-FTS) NO(x) measurements and MIPAS NO, measurements for the polar Northern Hemisphere are in reasonable agreement with these predictions. An extremely large ground level enhancement (GLE) occurred during the SPE period on January 20, 2005. We find that protons of energies 300 to 20,000 MeV, not normally included in our computations, led to enhanced lower stratospheric odd nitrogen concentrations of less than 0.1% as a result of this GLE.
Document ID
20110007967
Acquisition Source
Goddard Space Flight Center
Document Type
Preprint (Draft being sent to journal)
Authors
Jackman, C. H. (NASA Goddard Space Flight Center Greenbelt, MD, United States)
Marsh, D. R. (National Center for Atmospheric Research Boulder, CO, United States)
Vitt, F. M. (National Center for Atmospheric Research Boulder, CO, United States)
Roble, R. G. (National Center for Atmospheric Research Boulder, CO, United States)
Randall, C. E. (Colorado Univ. Boulder, CO, United States)
Bernath, P. F. (York Univ. York, United Kingdom)
Funke, B. (Instituto de Astrofisica de Andalucia Granada, Spain)
Lopez-Puertas, M. (Instituto de Astrofisica de Andalucia Granada, Spain)
Versick, S. (Karlsruhe Institute of Technology Karlsruhe, Germany)
Stiller, G. P. (Karlsruhe Institute of Technology Karlsruhe, Germany)
Tylka, A. J. (Naval Research Lab. Washington, DC, United States)
Fleming, E. L. (Science Systems and Applications, Inc. Lanham, MD, United States)
Date Acquired
August 25, 2013
Publication Date
January 1, 2011
Subject Category
Solar Physics
Funding Number(s)
CONTRACT_GRANT: NNX08AU44G
CONTRACT_GRANT: NNX06AC05G
PROJECT: AYA2008-03498/ESP
Distribution Limits
Public
Copyright
Public Use Permitted.

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