HR: 08:15h
AN: GC41B-02    [Abstracts]
TI: Long-term Atmospheric Changes Caused by the Very Large Solar Proton Event in July 2000
AU: * Jackman, C H
EM: Charles.H.Jackman@nasa.gov
AF: NASA Goddard Space Flight Center, Code 613.3 NASA GSFC Greenbelt Road, Greenbelt, MD 20771, United States
AU: Marsh, D R
EM: marsh@ucar.edu
AF: National Center for Atmospheric Research, NCAR P.O. Box 3000, Boulder, CO 80307-3000, United States
AU: Garcia, R R
EM: rgarcia@ucar.edu
AF: National Center for Atmospheric Research, NCAR P.O. Box 3000, Boulder, CO 80307-3000, United States
AU: Vitt, F M
EM: fvitt@ucar.edu
AF: National Center for Atmospheric Research, NCAR P.O. Box 3000, Boulder, CO 80307-3000, United States
AU: Randall, C E
EM: randall@lasp.colorado.edu
AF: University of Colorado, Laboratory for Atmospheric and Space Physics University of Colorado, Boulder, CO 80310, United States
AU: Fleming, E L
EM: fleming@kahuna.gsfc.nasa.gov
AF: NASA Goddard Space Flight Center, Code 613.3 NASA GSFC Greenbelt Road, Greenbelt, MD 20771, United States
AU: Labow, G J
EM: labow@lglass.gsfc.nasa.gov
AF: NASA Goddard Space Flight Center, Code 613.3 NASA GSFC Greenbelt Road, Greenbelt, MD 20771, United States
AB: Solar cycle 23 was accompanied by eight very large solar proton events (SPEs) between 2000 and 2005, along with numerous smaller events. The very large SPE in July 2000, which was associated with the well-known Bastille Day Solar Storm, caused very substantial changes in the polar mesosphere and stratosphere. Significant downward transport of the SPE-produced NOx from the polar lower mesosphere and upper stratosphere during the Southern Hemisphere winter period resulted in huge enhancements (>100%) in middle stratospheric NOx (NO+NO2) during September 2000 in the polar vortex, which were measured by UARS HALOE (C. E. Randall et al., Geophys. Res. Lett., 28, 2385-2388, 2001). We have used the Whole Atmosphere Community Climate Model (WACCM) to study the longer-term impact of the July 2000 SPE, the third largest SPE period in the past 40 years. This very large SPE provided a wonderful opportunity to study the downward transport of energetic particle precipitation effects in the middle atmosphere. Not surprisingly, the WACCM-simulated polar Northern Hemisphere influences from the July (mid-summer) 2000 SPE were significant for a few months, but the constituent changes were not transported below about 20 hPa. However in the polar Southern Hemisphere (SH) region, the persistent downward transport in the vortex during the months of July-August- September resulted in significant modeled influences for about a year past the SPE. The SH odd nitrogen family, NOy (N, NO, NO2, NO3, N2O5, HNO3, HO2NO2, ClONO2, BrONO2), was greatly enhanced by this SPE and these increases were transported to the lower stratosphere. The SPE-enhanced polar NOy resulted in long-lasting ozone decreases (from catalytic NOy destruction of ozone) and ozone increases (from NOy interference in the chlorine and bromine catalytic ozone destruction cycles). These ozone changes resulted in simulated SH polar stratospheric temperature decreases (1-2K) and increases (1-3K).
DE: 0340 Middle atmosphere: composition and chemistry
DE: 0341 Middle atmosphere: constituent transport and chemistry (3334)
DE: 0342 Middle atmosphere: energy deposition (3334)
DE: 1616 Climate variability (1635, 3305, 3309, 4215, 4513)
DE: 3305 Climate change and variability (1616, 1635, 3309, 4215, 4513)
SC: Global Environmental Change [GC]
MN: 2007 Fall Meeting