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A&A 423, 11191131 (2004) DOI: 10.1051/0004-6361:20040259
 

Summary: A&A 423, 11191131 (2004)
DOI: 10.1051/0004-6361:20040259
c ESO 2004
Astronomy
&
Astrophysics
Evolution and magnetic topology
of the M 1.0 flare of October 22, 2002
A. Berlicki1,2, B. Schmieder1,3, N. Vilmer1, G. Aulanier1, and G. Del Zanna4
1
Observatoire de Paris, Section de Meudon, LESIA, 92195 Meudon Principal Cedex, France
e-mail: arkadiusz.berlicki@obspm.fr
2
Astronomical Institute of the Wroclaw University, ul. Kopernika 11, 51-622 Wroclaw, Poland
3
Institute of Theoretical Astrophysics, University of Oslo, Blindern, 0315 Oslo, Norway
4
DAMTP, University of Cambridge, Cambridge, UK
Received 12 February 2004 / Accepted 30 April 2004
Abstract. In this paper we analyse an M 1.0 confined flare observed mainly during its gradual phase. We use the data taken

  

Source: Aulanier, Guillaume - Observatoire de Paris

 

Collections: Physics