Multiple-step geomagnetic storms and their interplanetary drivers

Details Multiple-step geomagnetic storms and their interplanetary drivers Multiple-step geomagnetic storms and their interplanetary drivers

Jan 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008georl..3506s07r&link_type=abstract

Geophysical Research Letters, Volume 35, Issue 6, CiteID L06S07

Physics

4

Magnetospheric Physics: Magnetic Storms And Substorms (7954), Magnetospheric Physics: Solar Wind/Magnetosphere Interactions, Interplanetary Physics: Ejecta, Driver Gases, And Magnetic Clouds

Scientific paper

While the classic picture of a geomagnetic storm is of a main phase eventually reaching maximum intensity, followed by a recovery, the profile can often be more complex. This has been recognized in past studies that have classified storms as having ``one'' or ``two'' ``steps'' during the main phase. However, the intense (Dst <= -100 nT) storms studied during the LWS CDAW Workshop may be more complicated. We discuss the variety of interplanetary circumstances that gave rise to several storms of varying complexity.

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