Atmospheric response to NO<sub>y</sub> source due to energetic electron precipitation

  • E. Rozanov
    Physical‐Meteorological Observatory/World Radiation Center Davos Switzerland
  • L. Callis
    Suffolk Virginia USA
  • M. Schlesinger
    Climate Research Group, Department of Atmospheric Sciences University of Illinois at Urbana‐Champaign Urbana Illinois USA
  • F. Yang
    National Centers for Environmental Prediction Camp Springs Maryland USA
  • N. Andronova
    Climate Research Group, Department of Atmospheric Sciences University of Illinois at Urbana‐Champaign Urbana Illinois USA
  • V. Zubov
    Department of Dynamical Meteorology A. I. Voeikov Main Geophysical Observatory St. Petersburg Russia

書誌事項

公開日
2005-07-22
権利情報
  • http://onlinelibrary.wiley.com/termsAndConditions#vor
DOI
  • 10.1029/2005gl023041
公開者
American Geophysical Union (AGU)

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説明

<jats:p>We have introduced additional NO<jats:sub>y</jats:sub> sources caused by energetic electron precipitation (EEP) during 1987 into a Chemistry‐Climate model. Comparison of two model runs with and without EEP reveals increase of reactive nitrogen by about 2 ppbv in the middle stratosphere over the tropical and middle latitudes. In the upper stratosphere over the polar winter regions the simulated NO<jats:sub>y</jats:sub> enhancement reaches 10 ppbv. Decreases of the ozone mixing ratio in the stratosphere by up to 5% over midlatitudes and up to 30% over southern high‐latitudes are calculated. A ∼0.5 K cooling in the middle stratosphere over the tropics and up to 2 K over southern high‐latitudes is calculated with detectable changes in the surface air temperatures. These results confirm that the magnitude of the atmospheric response to EEP events can potentially exceed the effects from solar UV fluxes. These mechanisms work in phase outside polar latitudes, but can compensate each other within polar latitudes.</jats:p>

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