Abstract
Abstract. Solar eruptions in early 2005 led to a substantial barrage of charged particles on the Earth's atmosphere during the 16–21 January period. Proton fluxes were greatly increased during these several days and led to the production of HOx (H, OH, HO2) and NOx (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 HOx and NOx constituents, and associated ozone reductions, due to these solar proton events (SPEs). The WACCM3 simulations show enhanced short-lived OH and HO2 concentrations throughout the mesosphere in the 60–82.5° N latitude band due to the SPEs for most days in the 16–21 January 2005 period, somewhat higher in abundance than those observed by the Aura Microwave Limb Sounder (MLS). These HOx 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 pptv in the lowermost mesosphere over the 16–18 January 2005 period due to the solar protons. WACCM3 predictions indicate H2O2 enhancements over the same time period of about three times 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 16–29 January 2005. WACCM3 simulations show only minuscule HNO3 increases (<0.05 ppbv) in the upper stratosphere during this time period. Polar mesospheric enhancements of NOx are computed to be greater than 50 ppbv during the SPE period due to the small loss rates during winter. Computed NOx increases, which were statistically significant at the 95 % level, lasted about a month past the SPEs. The SCISAT-1 Atmospheric Chemistry Experiment Fourier Transform Spectrometer NOx measurements and MIPAS NO2 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 20 January 2005. We find that protons of energies 300 to 20 000 MeV, associated with this GLE, led to very small enhanced lower stratospheric odd nitrogen concentrations of less than 0.1 % and ozone decreases of less than 0.01 %.
Highlights
Large solar eruptions during 16–21 January 2005 caused huge fluxes of high-energy solar charged particles to reach Earth
We included the highest energy protons (300 to 20 000 MeV) associated with the ground level enhancement (GLE) of neutrons on 20 January 2005 in some computations with “solar proton events (SPEs) + GLE”. This high energy proton flux was taken from the spectrum given in Usoskin et al (2009, 2011), which was derived using methodology presented in Tylka and Dietrich (2009)
We focus on the northern polar latitudes, a geographic region where HOx constituents are at very small values in January due to minimal or no sunlight
Summary
Large solar eruptions during 16–21 January 2005 caused huge fluxes of high-energy solar charged particles to reach Earth. We recently studied the short- and medium-term (days to a few months) atmospheric constituent effects of the four largest solar proton events (SPEs) in the past 45 years (August 1972, October 1989, July 2000, and October–November 2003) in Jackman et al (2008) with version 3 of the Whole Atmosphere Community Climate Model (WACCM3). The present investigation builds on that study and focuses on the short- and medium-term influences of solar particles on the mesosphere and stratosphere in the time period 1 January through 31 March 2005. 4. The modeled and measured influences of the January 2005 SPEs over the 1 January–31 March 2005 period are shown in Sect.
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