Title: University of Illinois, UrbanaChampaign, USA
1ELECTRON PRECIPITATION EFFECTS ON CHEMICAL
COMPOSITION AND CLIMATE
E. Rozanov, L. Callis, M. Schlesinger, F. Yang,
N. Andronova and V. Zubov
University of Illinois, Urbana-Champaign,
USA PMOD/WRC, Switzerland NASA/Goddard Space
Flight Center, USA University of Michigan, Ann
Arbor, USA Main Geophysical Observatory, Russia
2Outline
- Motivation
- Experimental set-up
- Results
3Motivation
The simulated responses of ozone and
temperature to solar irradiance variation over
the 11-year solar cycle do not agree with the
solar signal extracted from the observational
data
4Ozone (), Solar max - Solar min
Hood (2002)
Rozanov et al 2005
5(No Transcript)
6Mechanism proposed by Callis et al. (1991)
EEP gt NOy gt O3
7GOES gt2MeV
81987, 60-70 N and S
2D model (Callis, 1997)
9UIMESO Model history
MST CCM UIMESO
ST GCM/PC
24L (50 km)
40L (105 km)
10UIMESO what is inherited
- Horizontal grid 4o latitude by 5o longitude
- Dynamical core (FD)
- Representation of the surface and tropospheric
processes - Chemical solver (implicit Newton-Raphson)
- Advective transport (Hybrid scheme)
-
11UIMESO what is new (1)
- Model top at 105 km ( 40 layers in vertical
direction) - Non-orographic GWD according to Alexander and
Dunkerton (1999) - Solar heating due to oxygen absorption
- Chemical heating due to 7 reactions (Mlynczak and
Solomon, 1993) - Heating efficiency for Hartley and Ly-? bands
(Mlynczak and Solomon, 1993) - NonLTE parameterization of Fomichev et al., 1998
12UIMESO what is new (2)
- Photolysis rates for Ly-?, Schumann-Runge
continuum - NO photolysis according to Minschwaner and
Siskind, (1993) - Several new reactions
- Updated reaction coefficients and absorption
cross-sections (JPL-2000 and recent papers) - Additional NOx and HOx source due to EEP events
- NOx and HOx fluxes from the thermosphere
13Experimental set-up
Control run
Experiment
- Two 10-year long run
- SST/SI from AMIP climatology
- NOy source from EEP for 1987
14Annual changes
Rozanov et al (2006)
15Rozanov et al (2006)
16GOES gt2MeV
17Hood (2002)
Rozanov et al (2006)
Rozanov et al (2005)
18Problems
- Too intensive downward motions, too high NOy for
EEP run, too low CH4, H2O and ozone in winter
time over high-latitudes - Too high NOx and too low ozone in the
stratosphere due to probably overestimated O1D
production - Weak GWD from Alexander and Dunkerton (1999)
parameterization - Warm mesopause, absence of westerly winds in the
MLT region in summer
19Problems
20Conclusions
- The electrons have significant effects on the
ozone, temperature and dynamics in the
stratosphere. - Tropospheric changes are observed as well
- The reasons why for EEP run CCM overloads the
stratosphere with NOy are not clear - New runs with strong GWD are necessary