VLA observations at 91.6 cm wavelength describe large-scale features that either coincide with filaments, seen in emission rather than absorption, or act as large-scale magnetic loops that connect active regions and provide a conduit for relativistic electrons that trigger bursts at remote sites on the solar surface. VLA observations at 20.7 cm wavelength describe smaller, hotter coronal loops within active regions where impulsive bursts originate.


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    Titel :

    VLA observations of the inner corona


    Beteiligte:

    Erschienen in:

    Erscheinungsdatum :

    1991-01-01



    Medientyp :

    Sonstige


    Format :

    Keine Angabe


    Sprache :

    Englisch


    Schlagwörter :


    VLA observations of the inner corona

    Lang, Kenneth R. | Elsevier | 1991


    Inner corona from solar radio observations

    Gelfreikh, G.B. | Elsevier | 1991



    Models for inner corona parameters

    Monsignori Fossi, B.C. / Landini, M. | Elsevier | 1991


    Temperature Measurements in the Inner Corona

    Esser, R. et al. | British Library Online Contents | 1992