Astronomy and Astrophysics – Astronomy
Scientific paper
May 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992aas...180.3403k&link_type=abstract
American Astronomical Society, 180th AAS Meeting, #34.03; Bulletin of the American Astronomical Society, Vol. 24, p.783
Astronomy and Astrophysics
Astronomy
Scientific paper
A summary of all available radio observations made during the 1991 June campaign of the MAX '91/Flare 22 program will be presented. The presentation will be concerned primarily with millimeter wavelength (BIMA and Nobeyama) and centimeter wavelengths (Owens Valley and Nobeyama) observations. Emphasis will be given to the question of millimeter observations as a diagnostic for Mev electrons in solar flares (gamma ray flares --- BATSE and OSSE data), millimeter emission occurring at the steep rise phase of hard X-ray emitting electrons (BATSE data) and delay of millimeter emission onset and 25-100 Kev X-rays (BATSE data). Implications of these results for generation of millimeter emission and particle acceleration process will be discussed. The Nobeyama data consist of non-imaging patrol observations at several frequencies in the frequency range 1--80 GHz, and Owens Valley data were obtained using the frequency agile interferometer in the frequency range 1--18 GHz. Light curves and spectral information of the most energetic flares will be presented.
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