Artículo

van Driel-Gesztelyi, L.; Goff, C.P.; Démoulin, P.; Culhane, J.L.; Matthews, S.A.; Harra, L.K.; Mandrini, C.H.; Klein, K.-L.; Kurokawa, H. "Multi-scale reconnections in a complex CME" (2008) Advances in Space Research. 42(5):858-865
El editor solo permite decargar el artículo en su versión post-print desde el repositorio. Por favor, si usted posee dicha versión, enviela a
Consulte el artículo en la página del editor
Consulte la política de Acceso Abierto del editor

Abstract:

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, Hα 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. © 2007 COSPAR.

Registro:

Documento: Artículo
Título:Multi-scale reconnections in a complex CME
Autor:van Driel-Gesztelyi, L.; Goff, C.P.; Démoulin, P.; Culhane, J.L.; Matthews, S.A.; Harra, L.K.; Mandrini, C.H.; Klein, K.-L.; Kurokawa, H.
Filiación:Mullard Space Science Laboratory, University College London, Holmbury St. Mary, Dorking, Surrey RH5 6NT, United Kingdom
Observatoire de Paris, LESIA, UMR 8109 (CNRS), 92195 Meudon, Cedex Principal, France
Konkoly Observatory, the Hungarian Academy of Sciences, Budapest, Hungary
Instituto de Astronomía y Física del Espacio, CONICET-UBA, CC. 67 Suc. 28, 1428 Buenos Aires, Argentina
Hida and Kwasan Observatories, Kyoto University, Yamashina, Kyoto, 607, Japan
Palabras clave:Magnetic reconnection; Radio burst; Sun: coronal mass ejection; Sun: EUV; Sun: flares; Sun: magnetic fields; Sun: radio; Astrophysics; Crystallography; Magnetic fields; Magnetic materials; Magnetic structure; Field lines; Flux ropes; Magnetic (CE); Magnetic loops; Magnetic reconnection (MR); Magnetic-field lines; MDI magnetograms; Multi scaling; Open field lines; radio bursts; radio observations; Radio wavelengths; Solar radius; Magnetism
Año:2008
Volumen:42
Número:5
Página de inicio:858
Página de fin:865
DOI: http://dx.doi.org/10.1016/j.asr.2007.04.065
Título revista:Advances in Space Research
Título revista abreviado:Adv. Space Res.
ISSN:02731177
CODEN:ASRSD
Registro:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_02731177_v42_n5_p858_vanDrielGesztelyi

Referencias:

  • Antiochos, S.K., DeVore, C.R., Klimchuk, J.A., A model for solar coronal mass ejections (1999) ApJ, 510, pp. 485-493
  • Attrill, G.D.R., Harra, L.K., van Driel-Gesztelyi, L., Demoulin, P., Coronal "Wave": magnetic footprint of a coronal mass ejection? (2007) ApJ, 656, pp. L101-L104
  • Attrill, G., Nakwacki, M.S., Harra, L.K., van Driel-Gesztelyi, L., Mandrini, C.H., Dasso, S., Wang, J., Using the evolution of coronal dimming regions to probe the global magnetic field topology (2006) Solar Phys., 238, pp. 117-139
  • Aulanier, G., DeLuca, E.E., Antiochos, S.K., McMullen, R.A., Golub, L., The topology and evolution of the Bastille day flare (2000) ApJ, 540, pp. 1126-1142
  • Aurass, H., Klein, K.-L., Martens, P.C.H., First detection of correlated electron beams and plasma jets in radio and soft X-ray data (1994) Solar Phys., 155, pp. 203-206
  • Bogachev, S.A., Somov, B.V., Kosugi, T., Sakao, T., The motions of the hard X-ray sources in solar flares: images and statistics (2005) ApJ, 630, pp. 561-572
  • Bougeret, J.-L., Kaiser, M.L., Kellogg, P.J., Manning, R., Goetz, K., Monson, S.J., Monge, N., Hoang, S., Waves: the radio and plasma wave investigation on the Wind spacecraft (1995) Space Sci. Rev., 71, pp. 231-263
  • Brueckner, G.E., Howard, R.A., Koomen, M.J., Korendyke, C.M., Michels, D.J., Moses, J.D., Socker, D.G., Eyles, C.J., The large angle spectroscopic coronagraph (LASCO) (1995) Solar Phys., 162, pp. 357-402
  • Buttighoffer, A., Solar electron beams associated with radio type III (1998) A&A, 335, pp. 295-302
  • Caroubalos, C., Poquerusse, M., Bougeret, J.-L., Crepel, R., Radio evidence for a magnetic mirror effect on beams of subrelativistic electrons in the solar corona (1987) ApJ, 319, pp. 503-513
  • Delannée, C., Aulanier, G., CME associated with transequatorial loops and a bald patch flare (1999) Solar Phys., 190, pp. 107-129
  • Démoulin, P., Klein, K.-L., Goff, C., van Driel-Gesztelyi, L., Culhane, J., Mandrini, C., Matthews, S., Harra, L., Decametric N burst: a consequence of the interaction of two coronal mass ejections (2007) Solar Phys., 240, pp. 107-120
  • Démoulin, P., Priest, E.R., Lonie, D.P., Three-dimensional magnetic reconnection without null points 2. Application to twisted flux tubes (1996) JGR, 101, pp. 7631-7646
  • Fazakerley, A.N., Harra, L.K., Culhane, J.L., van Driel-Gesztelyi, L., Lucek, E., Matthews, S.A., Owen, C.J., Rème, H., Relating near-Earth observations of an interplanetary coronal mass ejection to the conditions at its site of origin in the solar corona (2005) GRL, 32, pp. 13105-13108
  • Gary, G.A., Moore, R.L., Eruption of a multiple-turn helical magnetic flux tube in a large flare: evidence for external and internal reconnection that fits the breakout model of solar magnetic eruptions (2004) ApJ, 611, pp. 545-556
  • Goff, C., van Driel-Gesztelyi, L., Démoulin, P., Culhane, J., Matthews, S., Harra, L., Mandrini, C., Kurokawa, H., A multiple flare scenario where the classic long duration flare was not the source of a cme (2007) Solar Phys., 240, pp. 89-106
  • Gopalswamy, N., Yashiro, S., Kaiser, M.L., Howard, R.A., Bougeret, J.-L., Radio signatures of coronal mass ejection interaction: coronal mass ejection cannibalism? (2001) ApJ, 548, pp. L91-L94
  • Grigis, P.C., Benz, A.O., The evolution of reconnection along an arcade of magnetic loops (2005) ApJ, 625, pp. L143-L146
  • Handy, B.N., Acton, L.W., Kankelborg, C.C., Wolfson, C.J., Akin, D.J., Bruner, M.E., The transition region and coronal explorer (1999) Solar Phys., 187, pp. 229-260
  • Harra, L.K., Démoulin, P., Mandrini, C.H., Matthews, S.A., van Driel-Gesztelyi, L., Culhane, J.L., Fletcher, L., Flows in the solar atmosphere due to the eruptions on the 15th July, 2002 (2005) A&A, 438, pp. 1099-1106
  • Koutchmy, S., Coronal physics from eclipse observations (1994) Adv. Space Res., 14, pp. 29-39
  • Leblanc, Y., Dulk, G.A., Kaiser, M.L., Bougeret, J.-L., Type U burst and CME in the solar wind (1999) GRL, 26, pp. 1089-1092
  • Leblanc, Y., Poquerusse, M., Aubier, M.G., Solar-type U bursts and coronal transients (1983) A&A, 123, pp. 307-315
  • Scherrer, P.H., Bogart, R.S., Bush, R.I., Hoeksema, J.T., Kosovichev, A.G., Schou, J., Rosenberg, W., Zayer, I., The solar oscillations investigation - Michelson Doppler imager (1995) Solar Phys., 162, pp. 129-188. , MDI Engineering Team
  • Sheeley Jr., N.R., Howard, R.A., Koomen, M.J., Michels, D.J., Associations between coronal mass ejections and soft X-ray events (1983) ApJ, 272, pp. 349-354
  • Tripathi, D., Bothmer, V., Cremades, H., The basic characteristics of EUV post-eruptive arcades and their role as tracers of coronal mass ejection source regions (2004) A&A, 422, pp. 337-349
  • Tripathi, D., Isobe, H., Mason, H.E., On the propagation of brightening after filament/prominence eruptions, as seen by SoHO-EIT (2006) A&A, 453, pp. 1111-1116

Citas:

---------- APA ----------
van Driel-Gesztelyi, L., Goff, C.P., Démoulin, P., Culhane, J.L., Matthews, S.A., Harra, L.K., Mandrini, C.H.,..., Kurokawa, H. (2008) . Multi-scale reconnections in a complex CME. Advances in Space Research, 42(5), 858-865.
http://dx.doi.org/10.1016/j.asr.2007.04.065
---------- CHICAGO ----------
van Driel-Gesztelyi, L., Goff, C.P., Démoulin, P., Culhane, J.L., Matthews, S.A., Harra, L.K., et al. "Multi-scale reconnections in a complex CME" . Advances in Space Research 42, no. 5 (2008) : 858-865.
http://dx.doi.org/10.1016/j.asr.2007.04.065
---------- MLA ----------
van Driel-Gesztelyi, L., Goff, C.P., Démoulin, P., Culhane, J.L., Matthews, S.A., Harra, L.K., et al. "Multi-scale reconnections in a complex CME" . Advances in Space Research, vol. 42, no. 5, 2008, pp. 858-865.
http://dx.doi.org/10.1016/j.asr.2007.04.065
---------- VANCOUVER ----------
van Driel-Gesztelyi, L., Goff, C.P., Démoulin, P., Culhane, J.L., Matthews, S.A., Harra, L.K., et al. Multi-scale reconnections in a complex CME. Adv. Space Res. 2008;42(5):858-865.
http://dx.doi.org/10.1016/j.asr.2007.04.065