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• W2139402008 abstract "Type III solar radiobursts are a form of sporadic solar radioemission originating throughout the solar corona and also in the interplanetary region, to heliocentric distances of 1AU and beyond. They are associated with fluxes of moderately energetic electrons (10–100 keV) which are accelerated either in flares or in active storm regions and which escape along magnetic field lines that penetrate the high corona. The bursts appear to have a frequency corresponding to twice the local plasma frequency (2ω e ) (sometimes, the plasma frequency), their frequency drifts at a rate suggesting a source velocity of 10 10 cm/sec. At a fixed frequency the duration ranges from < at the highest frequencies, to more than 1 hr at the lowest frequencies [Smith 1974; Fainberg and Stone 1974]." @default.
• W2139402008 created "2016-06-24" @default.
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• W2139402008 date "1979-06-01" @default.
• W2139402008 modified "2023-09-27" @default.
• W2139402008 title "Interplanetary type III radiobursts" @default.
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• W2139402008 doi "https://doi.org/10.1029/rg017i004p00624" @default.
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