A flood of new observations of the solar corona have been made with high spatial resolution, good temporal coverage and resolution, and large linear dynamic range by the Soft X-ray Telescope (SXT) on Yohkoh. These data are changing our fundamental understanding of how solar magnetic fields emerge, interact, and dissipate. This paper reviews some of the results from Yohkoh in the context of earlier results from the Solar Maximum Mission (SMM) and in comjunction with ground-based optical and radio observations.


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    Titel :

    A new perspective on solar active regions


    Beteiligte:
    Strong, K. T. (Autor:in) / Bruner, M. E. (Autor:in)

    Erschienen in:

    Erscheinungsdatum :

    1996-01-01



    Medientyp :

    Sonstige


    Format :

    Keine Angabe


    Sprache :

    Englisch


    Schlagwörter :


    A New Perspective on Solar Active Regions

    Strong, K.T. | Online Contents | 1995


    A New Perspective on Solar Active Regions

    Strong, K.T. | Online Contents | 1996


    A New Perspective on Solar Active Regions

    Strong, K. T. / Bruner, M. E. / COSPAR et al. | British Library Conference Proceedings | 1995


    Abundance variations in solar active regions

    Strong, K.T. / Lemen, J.R. / Linford, G.A. | Elsevier | 1991


    Magnetic Fields in Solar Active Regions

    Mclntosh, Patrick S. / Dryer, Murray | AIAA | 1972