Mathematics – Logic
Scientific paper
Aug 2008
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008cosre..46..320s&link_type=abstract
Cosmic Research, Volume 46, Issue 4, pp.320-326
Mathematics
Logic
1
96.60Qe, 96.60Ph
Scientific paper
Based on the analysis of a strong solar flare X1.6/2B on October 19, 2001 in the active region 9661, accompanied by a coronal mass ejection (CME) of the halo type, a topological model of development of this solar event is suggested. The model considers a unified process of development of CME and a chromosphere flare. According to the model, this process has a common source of energy supply: the turbulent current layer lying between the arcade of flare loops and the surface of CME going away. The structures on the ends of flare bands (SEFB) represent in this model chromosphere feet of the system of large-scale coronal magnetic arches at the initial stage of the dynamic processes whose evolution results in CME. Peripheral structures (PS) of the flare (elongated double bright emission strips beyond the limits of the active region) are interpreted as chromosphere bases of magnetic field lines that form an external shell (braid) of the CME at the late stage of the flare.
Sidorov Victor I.
Yazev S. A.
No associations
LandOfFree
Topological model of the solar event including a flare and coronal mass ejection on October 19, 2001 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Topological model of the solar event including a flare and coronal mass ejection on October 19, 2001, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Topological model of the solar event including a flare and coronal mass ejection on October 19, 2001 will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1694096