A Statistical Model for the Occurrence Times of Coronal Mass Ejections and Solar Flares

Details A Statistical Model for the Occurrence Times of Coronal Mass Ejections and Solar Flares A Statistical Model for the Occurrence Times of Coronal Mass Ejections and Solar Flares

Dec 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006agufmsh21a0317h&link_type=abstract

American Geophysical Union, Fall Meeting 2006, abstract #SH21A-0317

Physics

7513 Coronal Mass Ejections (2101), 7519 Flares, 7536 Solar Activity Cycle (2162), 7537 Solar And Stellar Variability (1650)

Scientific paper

The rate of occurrence of coronal mass ejections (CMEs) and solar flares is of interest to solar and geomagnetic physicists, as better descriptions of time trends in these processes may lead to more accurate predictions of geomagnetic storms and a better understanding of the process by which magnetic energy is released in the solar corona. In recent years, there has been wide spread debate about whether CMEs and solar flares are temporally associated. This paper presents a statistical model for the superimposed (or joint) process in order to provide insight toward the nature of the correlation between the two individual processes. The temporal relationship between CME velocity and flare intensity is also explored.

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