Temporal comparison of nonthermal flare emission and magnetic-flux change rates
نویسندگان
چکیده
منابع مشابه
Nonthermal Flare Emission from MeV - energy
We present analyses of two solar ares observed with high spatial resolution at 86 GHz with the BIMA millimeter{wavelength telescope and at 17 and 34 GHz with the Nobeyama radioheliograph. The ares were observed on Nov. 24, 1998 and May 1, 1999. At millimeter wavelengths these are impulsive events and therefore they must be produced by MeV energy electrons. The present study using simultaneous o...
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We present analyses of two solar ares observed with high spatial resolution at 86 GHz with the BIMA millimeter{wavelength telescope and at 17 and 34 GHz with the Nobeyama radioheliograph. In both events there is evidence for a simple bipolar structure in the radio source: in one case two distinct sources are clearly spatially resolved, while in the second the polarization image at 17 GHz sugges...
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We present analyses of two solar ares observed with high spatial resolution at 86 GHz with the BIMA millimeter{wavelength telescope and at 17 and 34 GHz with the Nobeyama radioheliograph. The ares were observed on Nov. 24, 1998 and May 1, 1999. At millimeter wavelengths these are impulsive events and therefore they must be produced by MeV energy electrons. The present study using simultaneous o...
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ژورنال
عنوان ژورنال: Astronomy & Astrophysics
سال: 2009
ISSN: 0004-6361,1432-0746
DOI: 10.1051/0004-6361/200810947