Tackling Substorm Problems: New Observational and Modeling Capabilities

Details Tackling Substorm Problems: New Observational and Modeling Capabilities Tackling Substorm Problems: New Observational and Modeling Capabilities

Aug 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008eostr..89..324n&link_type=abstract

Eos, Transactions American Geophysical Union, Volume 89, Issue 35, p. 324-324

Physics

Magnetospheric Physics: Substorms, Magnetospheric Physics: Magnetosphere/Ionosphere Interactions (2431), Magnetospheric Physics: Solar Wind/Magnetosphere Interactions

Scientific paper

Ninth International Conference on Substorms; Graz, Austria, 5-9 May 2008; Geomagnetic substorms, responsible for creating brightly lit aurorae that can disrupt satellite communications and electric power grids, comprise a wealth of dynamic plasma processes. These processes and their interplay were discussed by about 130 scientists at a conference at Austria's Seggau Castle, organized by the Space Research Institute of the Austrian Academy of Sciences.

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