The Very Large Array (VLA) and the Nancay Radioheliograph (NR) can be used in the 1990s to provide unique observations of the quiescent and active corona. The combined data can specify the evolution and magnetic structure at a variety of heights in the quiescent corona, from compact to extended structures such as loops, streamers and coronal holes. The scientific potential of simultaneous VLA-NR research is illustrated by observations of solar noise storms with hitherto unavailable resolution in space (VLA) and time (NR). Unique information will also be provided for other types of solar bursts, leading to an improved understanding of solar activity during the coming maximum.


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    Titel :

    High resolution VLA-Nancay observations of the sun


    Beteiligte:
    Kerdraon, A. (Autor:in) / Trottet, G. (Autor:in) / Lang, K. R. (Autor:in) / Willson, R. F. (Autor:in)

    Erschienen in:

    Erscheinungsdatum :

    1988-01-01



    Medientyp :

    Sonstige


    Format :

    Keine Angabe


    Sprache :

    Englisch


    Schlagwörter :


    High resolution VLA-Nancay observations of the sun

    Kerdraon, A. / Lang, K.R. / Trottet, G. et al. | Elsevier | 1989


    The Nancay multifrequency radioheliograph: New observations

    Mercier, C. / Klein, K.-L. / Trottet, G. | Elsevier | 1989


    SETI at the Nançay radiotelescope

    Biraud, François | Elsevier | 1983


    WIND/3DP and Nancay Radioheliograph Observations of Solar Energetic Electron Events

    Klein, K.-L. / Krucker, S. / Trottet, G. et al. | British Library Conference Proceedings | 2003