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University of Illinois, Urbana-Champaign, USA. PMOD/WRC, Switzerland. NASA/Goddard Space Flight Center, ... Photolysis rates for Ly- , Schumann-Runge continuum ... – PowerPoint PPT presentation

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Title: University of Illinois, UrbanaChampaign, USA


1
ELECTRON 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
2
Outline
  • Motivation
  • Experimental set-up
  • Results

3
Motivation
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
4
Ozone (), Solar max - Solar min
Hood (2002)
Rozanov et al 2005
5
(No Transcript)
6
Mechanism proposed by Callis et al. (1991)
EEP gt NOy gt O3
7
GOES gt2MeV
8
1987, 60-70 N and S
2D model (Callis, 1997)
9
UIMESO Model history
MST CCM UIMESO
ST GCM/PC
24L (50 km)
40L (105 km)
10
UIMESO 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)

11
UIMESO 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

12
UIMESO 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

13
Experimental set-up
Control run
Experiment
  • Two 10-year long run
  • SST/SI from AMIP climatology
  • No NOy source from EEP
  • NOy source from EEP for 1987

14
Annual changes
Rozanov et al (2006)
15
Rozanov et al (2006)
16
GOES gt2MeV
17
Hood (2002)
Rozanov et al (2006)
Rozanov et al (2005)
18
Problems
  • 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

19
Problems
  • 2D e- gt NOy
  • Non-LTE
  • QBO

20
Conclusions
  • 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
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