Evidence of two-stage magnetic reconnection in the 2005 January 15 X2.6 flare

Details Evidence of two-stage magnetic reconnection in the 2005 January 15 X2.6 flare Evidence of two-stage magnetic reconnection in the 2005 January 15 X2.6 flare

Nov 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011newa...16..470w&link_type=abstract

New Astronomy, Volume 16, Issue 7, p. 470-476.

Astronomy and Astrophysics

Astronomy

Scientific paper

We analyze in detail the X2.6 flare that occurred on 2005 January 15 in the NOAA AR 10720 using multiwavelength observations. There are several interesting properties of the flare that reveal possible two-stage magnetic reconnection similar to that in the physical picture of tether-cutting, where the magnetic fields of two separate loop systems reconnect at the flare core region, and subsequently a large flux rope forms, erupts, and breaks open the overlying arcade fields. The observed manifestations include: (1) remote Hα brightenings appear minutes before the main phase of the flare; (2) separation of the flare ribbons has a slow and a fast phase, and the flare hard X-ray emission appears in the later fast phase; (3) rapid transverse field enhancement near the magnetic polarity inversion line (PIL) is found to be associated with the flare. We conclude that the flare occurrence fits the tether-cutting reconnection picture in a special way, in which there are three flare ribbons outlining the sigmoid configuration. We also discuss this event in the context of what was predicted by Hudson et al. (2008), where the Lorentz force near the flaring PIL drops after the flare and consequently the magnetic field lines there turn to be more horizontal as we observed.

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