What we can learn from the intensity-time profiles of large gradual solar energetic particle events?

Details What we can learn from the intensity-time profiles of large gradual solar energetic particle events? What we can learn from the intensity-time profiles of large gradual solar energetic particle events?

Apr 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009eguga..1113571t&link_type=abstract

"EGU General Assembly 2009, held 19-24 April, 2009 in Vienna, Austria http://meetings.copernicus.org/egu2009, p.13571"

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Large gradual solar energetic particle events (LGSEPEs, ≥10pfu in the >10MeV channel as measured by GOES) are closely associated with coronal mass ejections (CMEs). The intensity-time profile of a LGSEPE reveals important information on the moving directions of a CME or an interplanetary CME (ICME). This paper analyzes the moving directions of ICMEs, using the intensity-time profiles of 5 typical solar energetic particle events, and discusses their applications in predicting geomagnetic storms.

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