Progress in Understanding Radio Emission from Solar Flares: Observations with the Nobeyama Radioheliograph 1999-2004

Physics

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Scientific paper

Studies of solar flares based on observations by the Nobeyama Radioheliograph and related instruments such as the Owens Valley Solar Array, the Nançay Radioheliograph, and the Solar Submillimeter Telescope, as well as supporting instruments such as the RHESSI, TRACE, and SOHO missions, are reviewed for the period 1999-2004. Work on the classification of solar radio bursts is briefly discussed. Recent observational work on loop-top radio sources and rapidly propagating emission signatures is summarized and its interpretation in terms of electron anisotropies is described. Possible acceleration processes yielding such anisotropies are also briefly discussed. Recent work on electron acceleration and transport in a relatively dense plasma environment is summarized. Finally, recent work at millimeter and submillimeter wavelengths is described.

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