The first high-spatial-resolution interferometric observations of solar flares at millimeter wavelengths are presented. They are of high sensitivity, and events ranging from subflares to X-class flares were detected. One to three baselines with fringe spacings of 2 to 5 arcsec were available, which demonstrated that generally source sizes were in excess of 2 arcsec, but in some events the sources may be about 1 arcsec.


    Access

    Access via TIB

    Check availability in my library


    Export, share and cite



    Title :

    High spatial resolution observations of solar flares at 3.3 mm wavelength


    Contributors:
    Kundu, M. R. (author) / White, S. M. (author) / Welch, W. J. (author) / Bieging, J. H. (author)


    Publication date :

    1991-01-01



    Type of media :

    Miscellaneous


    Type of material :

    No indication


    Language :

    English


    Keywords :


    High spatial resolution observations of solar flares at 3.3 mm wavelength

    Kundu, M.R. / White, S.M. / Welch, W.J. et al. | Elsevier | 1991


    Interferometric observations of solar flares at 3 mm wavelength

    Kundu, M.R. / White, S.M. / Gopalswamy, N. et al. | Elsevier | 1993


    Multi-wavelength observations of the pre-cursor phase of solar flares

    Matthews, S.A. / Harra, L.K. / Culhane, J.L. | Elsevier | 2003



    Multi-Wavelength Observations of the Pre-Cursor Phase of Solar Flares

    Matthews, S. A. / Harra, L. K. / Culhane, J. L. et al. | British Library Conference Proceedings | 2003