Abstract Throughout the quiet Sun years 1982–1987, the Clark Lake Radioheliograph routinely mapped the solar corona on a daily basis at frequencies from 30 to 100 MHz. The Clark Lake maps show a variety of features which we have analyzed quantitatively, providing information about the three dimensional nature of large scale structures of the solar corona.


    Access

    Check access

    Check availability in my library

    Order at Subito €


    Export, share and cite



    Title :

    Three dimensional structures of coronal streamers, holes and CME plasmoids from multifrequency imaging observations


    Contributors:
    Kundu, M.R. (author) / Schmahl, E.J. (author) / Gopalswamy, N. (author) / White, S.M. (author)

    Published in:

    Publication date :

    1989-01-01


    Size :

    5 pages




    Type of media :

    Article (Journal)


    Type of material :

    Electronic Resource


    Language :

    English



    Radio Observations of Coronal Streamers

    Kundu, M. R. | British Library Online Contents | 1992


    Modeling Solar Coronal Streamers

    Suess, S. T. | British Library Online Contents | 1992


    Reconnection in Adjoining Coronal Helmet Streamers

    Dahlburg, R. B. / Karpen, J. T. / COSPAR; Scientific Commission D | British Library Conference Proceedings | 1997


    Predicting Ly- Intensities in Coronal Streamers

    Noci, G. et al. | British Library Online Contents | 1992


    Plasma Distribution Functions in Plasmoids: Geotail Observations

    Mukai, T. / International Council of Scientific Unions | British Library Conference Proceedings | 2000