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- W3102921892 abstract "A statistical analysis of radio flare events was conducted by using the event list of Nobeyama Radioheliograph in the years 1996–2009. We examined center-to-limb variations of 17 GHz and 34 GHz fluxes by dividing the flare events into different groups according to the ``thermal plasma richness'' (ratio of the peak flux of soft X-ray to nonthermal radio emissions) and the duration of radio bursts. It was found that the peak flux at 17 and 34 GHz tended to be higher toward the limb for thermal-rich flares with short durations. We propose that the thermal-rich flares, which are supposed to be associated with an efficient precipitation of high-energy particles into the chromosphere, have a pitch-angle distribution of nonthermal electrons with a higher population along the flare loop." @default.
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- W3102921892 date "2011-12-25" @default.
- W3102921892 modified "2023-10-16" @default.
- W3102921892 title "Center-to-Limb Variation of Radio Emissions from Thermal-Rich and Thermal-Poor Solar Flares" @default.
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- W3102921892 doi "https://doi.org/10.1093/pasj/63.6.1251" @default.
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