HR: 11:20h
AN: SH11E-04 INVITED [PDF]
TI: Ultraviolet Radiation and Stratospheric Ozone
AU: * Stolarski, R S
EM: stolar@polska.gsfc.nasa.gov
AF: NASA Goddard Space Flight Center, Mail Code 916, Greenbelt, MD 20771 United States
AB:
Ultraviolet radiation from the sun produces ozone in the stratosphere and it participates in the destruction of ozone.
Absorption of solar ultraviolet radiation by ozone is the primary heating mechanism leading to the maximum in temperature at
the stratopause. Variations of solar ultraviolet radiation on both the 27-day solar rotation period and the 11-year solar
cycle affect ozone by several mechanisms. The temperature and ozone in the upper stratosphere respond to solar uv variations
as a coupled system. An increase in uv leads to an increase in the production of ozone through the photolysis of molecular
oxygen. An increase in uv leads to an increase in temperature through the heating by ozone photolysis.
The increase in temperature leads to a partially-offsetting decrease in ozone through temperature-dependent reaction rate
coefficients. The ozone variation modulates the heating
by ozone photolysis. The increase in ozone at solar maximum enhances the uv heating. The processes are understood and
supported by long-term data sets.
Variation in the upper stratospheric temperatures will lead to a change in the behavior of waves propagating upward from the
troposphere. Changes in the pattern of wave dissipation
will lead to acceleration or deceleration of the mean flow and changes in the residual or transport circulation. This
mechanism could lead to the propagation of the solar cycle
effect of solar uv variation from the upper stratosphere downward to the lower stratosphere. This process is not
well-understood and has been the subject of an increasing number of model studies. I will review the data analyses for solar
cycle and their comparison to model results.
DE: 1610 Atmosphere (0315, 0325)
DE: 1650 Solar variability
SC: SPA - Solar and Heliospheric Physics [SH]
MN: 2003 Fall Meeting