Title of article :
Energetics of the 18 May 1994 brightening event Original Research Article
Author/Authors :
Y.H. Tang، نويسنده , , Y.N. Li، نويسنده , , C. Fang، نويسنده , , B. Schmieder، نويسنده , , G. Aulanier، نويسنده , , C. H. Mandrini and P. Demoulin، نويسنده ,
Issue Information :
دوهفته نامه با شماره پیاپی سال 2002
Pages :
4
From page :
557
To page :
560
Abstract :
By using YOHKOH soft X-ray images, vector magnetograms and Hα filtergrams, the energetics of the brightening event of May 18, 1994 has been studied. It occurred in a nearly potential magnetic configuration as shown by the comparison between the magnetic extrapolation(linear force free field) and the large scale soft X-ray loops. This event is related to the emergence of a new magnetic flux. The brightening points of Hα and soft X-ray are located at computed separatrices associated with field lines which are tangent to the photosphere. This brightening may be a signature of reconnection taking place between the pre-existing non-potential loops and the new emerging small loops. The magnetic energy provided by reconnection is likely to be stored in the non-potential loops and shearing emerging flux. A phenomenological model is offered.
Journal title :
Advances in Space Research
Serial Year :
2002
Journal title :
Advances in Space Research
Record number :
1128183
Link To Document :
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