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The Impact of Energetic Particle Precipitation on the Atmosphere
Charles Jackman, NASA Goddard Space Flight Center
Charles Jackman reported on solar energetic precipitating particles (EPPs), which are electrons
and protons generated by solar flares, coronal mass ejections, and geomagnetic storms. They precipitate
in Earth's polar regions, where they enhance the production of HO x and NO x that destroy ozone in the
mesosphere and upper stratosphere (Figure 2.9). Because of the relatively short lifetime of HO x
constituents, most of the atmospheric and climate-relevant EPP focus is on NO x . Solar protons and
electrons have episodic seasonal and solar cycle influence on the polar mesosphere. Measurements and
models show that in years when significant winter-time meteorological events occur, EPP-enhanced NO x
is transported from the upper mesosphere and lower thermosphere to lower altitudes where their impact
may last several months, decreasing ozone by a few percent. There may even be a top-down effect where
by EPP-NO x induced ozone destruction leads to changes in surface air temperature. Jackman noted that
there may be a coupling between electron impact and climate, 28,29 but that these findings need further
work and affirmation. Jackman stated that GCRs (primarily protons and alpha particles) also create NO x
and HO x but at lower altitudes due to their higher energy compared to solar particles. Because the
incidence of GCRs varies inversely with solar activity, their effects on stratospheric chemistry tend to be
out of phase with those of EPPs. Including GCRs in models results in an increase (relative to no GCRs)
in NO y of 10-20 percent in the lower stratosphere, with the greatest effects at high latitudes, and a
decrease is stratospheric ozone by around 1 percent. However, a GCR-driven solar-cycle variation in
polar NO y is less than about 5 percent (greater at solar minimum than at solar maximum), resulting in
annually averaged variations in polar ozone of less than 0.06 percent.
FIGURE 2.9 The atmospheric structure with incoming galactic cosmic rays and solar protons. SOURCE: C.
Jackman, NASA Goddard Space Flight Center, “The Impact of Energetic Particle Precipitation on the
Atmosphere,” presentation to the Workshop on the Effects of Solar Variability on Earth's Climate, September 9,
28 E. Rozanov, L. Callis, M. Schlesinger, F. Yang, N. Andronova, and V. Zubov, Atmospheric response to NO y
source due to energetic electron precipitation, Geophysical Research Letters 32:L14811, 2005.
29 A. Seppälä, C.E. Randall, M.A. Clilverd, E. Rozanov, and C.J. Rodger, Geomagnetic activity and polar
surface air temperature variability, Journal of Geophysical Research 114:A10312, 2009.
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