A model study of the impact of magnetic field structure on atmospheric composition during solar proton events

Author:

Sinnhuber Miriam1,Burrows John P.1,Chipperfield Martyn P.2,Jackman Charles H.3,Kallenrode May-Britt4,Künzi Klaus F.1,Quack Manuel14

Affiliation:

1. Institute of Environmental Physics; University of Bremen; Germany

2. School of the Environment; University of Leeds; UK

3. NASA Goddard Space Flight Center; Greenbelt Maryland USA

4. University of Osnabrück; Germany

Publisher

American Geophysical Union (AGU)

Subject

General Earth and Planetary Sciences,Geophysics

Reference23 articles.

1. Multiannual simulations with a three-dimensional chemical transport model;Chipperfield;J. Geophy. Res.,1999

2. Solar-atmospheric coupling by electrons (SOLACE), 2, Calculated stratospheric effects of precipitating electrons, 1979-1988;Callis;J. Geophys. Res.,1998

3. Solar Proton Events: Stratospheric Sources of Nitric Oxide;Crutzen;Science,1975

4. Possible composition and climatic changes due to past intense energetic particle precipitation;Hauglustaine;Annales Geophysicae,1990

5. Small-scale structure of the geodynamo inferred from the Oersted and Magsat satellite data;Hulot;Nature,2002

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