Abstract The Very Large Array (VLA) and the Nançay 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), 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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    Title :

    High resolution VLA-Nancay observations of the sun


    Contributors:
    Kerdraon, A. (author) / Lang, K.R. (author) / Trottet, G. (author) / Willson, R.F. (author)

    Published in:

    Publication date :

    1989-01-01


    Size :

    4 pages




    Type of media :

    Article (Journal)


    Type of material :

    Electronic Resource


    Language :

    English



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