UCL logo

UCL Discovery

UCL home » Library Services » Electronic resources » UCL Discovery

Multi-scale reconnections in a complex CME

van Driel-Gesztelyi, L; Goff, CP; Demoulin, P; Culhane, JL; Matthews, SA; Harra, LK; Mandrini, CH; ... Kurokawa, H; + view all (2008) Multi-scale reconnections in a complex CME. ADV SPACE RES , 42 (5) 858 - 865. 10.1016/j.asr.2007.04.065.

Full text not available from this repository.


A series of three flares of GOES class M, M and C, and a CME were observed on 20 January 2004 occurring in close succession in NOAA 10540. Types II, III, and N radio bursts were associated. We use the combined observations from TRACE, EIT, H alpha images from Kwasan Observatory, MDI magnetograms, GOES, and radio observations from Culgoora and Wind/WAVES to understand the complex development of this event. We reach three main conclusions. First, we link the first two impulsive flares to tether-cutting reconnections and the launch of the CME. This complex observation shows that impulsive quadrupolar flares can be eruptive. Second, we relate the last of the flares, an LDE, to the relaxation phase following forced reconnections between the erupting flux rope and neighbouring magnetic field lines, when reconnection reverses and restores some of the pre-eruption magnetic connectivities. Finally, we show that reconnection with the magnetic structure of a previous CME launched about 8 h earlier injects electrons into open field lines having a local dip and apex (located at about six solar radii height). This is observed as an N-burst at decametre radio wavelengths. The dipped shape of these field lines is due to large-scale magnetic reconnection between expanding magnetic loops and open field lines of a neighbouring streamer. This particular situation explains why this is the first N-burst ever observed at long radio wavelengths. (C) 2007 COSPAR. Published by Elsevier Ltd. All rights reserved.

Type: Article
Title: Multi-scale reconnections in a complex CME
DOI: 10.1016/j.asr.2007.04.065
Keywords: magnetic reconnection, Sun : magnetic fields, Sun : EUV, Sun : flares, Sun : coronal mass ejection, Sun : radio, radio burst, CORONAL MASS EJECTION, ELECTRON-BEAMS, SOLAR CORONA, RADIO, EVOLUTION, ERUPTIONS, FLARE, PROPAGATION, TOPOLOGY, REGIONS
URI: http://discovery.ucl.ac.uk/id/eprint/114104
Downloads since deposit
Download activity - last month
Download activity - last 12 months
Downloads by country - last 12 months

Archive Staff Only

View Item View Item