The Impact of Energetic Particle Precipitation on the Earths Atmosphere

  • B. Funke
  • M. López-Puertas
  • M. García-Comas
  • D. Bermejo-Pantaleón
  • G. P. Stiller
  • T. von Clarmann
Conference paper
Part of the Astrophysics and Space Science Proceedings book series (ASSSP)

Abstract

Energetic particle precipitation (EPP) represents an important Sun–Earth coupling mechanism with important implications on polar stratospheric ozone chemistry. Solar protons generated during solar storms cause sporadically in situ production of stratospheric NOx and HOx radicals involved in catalytic ozone destruction. Further, NO produced continuously in the mesosphere and lower thermosphere by medium energy electron precipitation (EEP) descends to the stratosphere during the polar winter, where it represents an additional, though variable source of NOx. The capability of the Michelson Interferometer for Passive Atmospheric Sounding (MIPAS) to measure all important NOy species, as well as ClO and HOCl with global coverage including the polar night regions make it an ideal instrument for studying EPP effects on stratospheric chemistry. We present a quantitative assessment of EPP-induced composition changes as observed by MIPAS during 2002–2004, including the unusually strong solar proton event in October/November 2003. The impact of EPP on the stratospheric ozone budget has been studied with chemical models. The stratospheric ozone loss in the polar regions reached 18DU and lasted over months to years.

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Copyright information

© Springer-Verlag Berlin Heidelberg 2010

Authors and Affiliations

  • B. Funke
    • 1
  • M. López-Puertas
    • 1
  • M. García-Comas
    • 1
  • D. Bermejo-Pantaleón
    • 1
  • G. P. Stiller
    • 2
  • T. von Clarmann
    • 2
  1. 1.Instituto de Astrofísica de Andalucía, CSICGranadaSpain
  2. 2.Institut für Meteorologie und KlimaforschungUniversity and Forschungszentrum KarlsruheKarlsruheGermany

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