• 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