Quasi-Simultaneous Flux Emergence in the Events of October November 2003

Details Quasi-Simultaneous Flux Emergence in the Events of October November 2003 Quasi-Simultaneous Flux Emergence in the Events of October November 2003

Aug 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007soph..244...13z&link_type=abstract

Solar Physics, Volume 244, Issue 1-2, pp. 13-24

Physics

10

Sun: Activity, Sun: Magnetic Fields, Sun: Interior

Scientific paper

From late October to the beginning of November 2003, a series of intense solar eruptive events took place on the Sun. More than six active regions (ARs), including three large ARs (NOAA numbers AR 10484, AR 10486, and AR 10488), were involved in the activity. Among the six ARs, four of them bear obviously quasi-simultaneous emergence of magnetic flux. Based on the global H α and SOHO/EIT EUV observations, we found that a very long filament channel went through the six ARs. This implies that there is a magnetic connection among these ARs. The idea of large-scale magnetic connectivity among the ARs is supported by the consistency of the same chirality in the three major ARs and in their associated magnetic clouds. Although the detailed mechanisms for the quasi-simultaneous flux emergence and the large-scale flux system formation need to be extensively investigated, the observations provide new clues in studying the global solar activity.

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