A New Method for Identifying SMCs

Details A New Method for Identifying SMCs A New Method for Identifying SMCs

Dec 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009agufmsm13b1602d&link_type=abstract

American Geophysical Union, Fall Meeting 2009, abstract #SM13B-1602

Physics

[2740] Magnetospheric Physics / Magnetospheric Configuration And Dynamics, [2788] Magnetospheric Physics / Magnetic Storms And Substorms, [2799] Magnetospheric Physics / General Or Miscellaneous

Scientific paper

Current methodologies for identifying steady magnetospheric convection events (SMCs) are either not robust enough to find active SMCs or require hand selection of events. This limits the investigations of SMCs to either case studies or limited statistical studies of weaker SMCs. If we want to find the reason that the magnetosphere enters into a global sawtooth oscillation instead of an active SMC, we need a more comprehensive list of SMCs. Thus, we intend to find a new method for identifying SMCs in current and archived data. We have tested and validated three possible new methods for identifying SMC events, using current lists of substorms and SMCs. There will be a discussion of the validation and testing techniques along with a comparison of the different methods.

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