Introduction to special section on Large Geomagnetic Storms

Details Introduction to special section on Large Geomagnetic Storms Introduction to special section on Large Geomagnetic Storms

Mar 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009jgra..11400a00g&link_type=abstract

Journal of Geophysical Research, Volume 114, CiteID A00A00

Physics

Interplanetary Physics: Coronal Mass Ejections (7513), Ionosphere: Ionospheric Storms (7949), Magnetospheric Physics: Solar Wind/Magnetosphere Interactions, Atmospheric Processes: Thermospheric Dynamics (0358), Space Weather: Solar Effects

Scientific paper

Solar cycle 23 witnessed the accumulation of rich data sets that reveal various aspects of geomagnetic storms in unprecedented detail both at the Sun where the storm-causing disturbances originate and in geospace where the effects of the storms are directly felt. During two recent coordinated data analysis workshops (CDAWs) the large geomagnetic storms (Dst <= -100 nT) of solar cycle 23 were studied in order to understand their solar, interplanetary, and geospace connections. This special section grew out of these CDAWs with additional contributions relevant to these storms. Here I provide a brief summary of the results presented in the special section.

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