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.


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    Titel :

    High spatial resolution observations of solar flares at 3.3 mm wavelength


    Beteiligte:
    Kundu, M. R. (Autor:in) / White, S. M. (Autor:in) / Welch, W. J. (Autor:in) / Bieging, J. H. (Autor:in)


    Erscheinungsdatum :

    01.01.1991



    Medientyp :

    Sonstige


    Format :

    Keine Angabe


    Sprache :

    Englisch


    Schlagwörter :


    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. et al. | British Library Conference Proceedings | 2003



    Extreme Ultraviolet Observations of Solar Flares

    Mclntosh, Patrick S. / Dryer, Murray | AIAA | 1972