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Solar wind density model from km-wave type III bursts
Authors:Hector Alvarez  F T Haddock
Institution:(1) Indian Institute of Astrophysics, 3 Kodaikanal, India
Abstract:Solar radio bursts were observed with a 4-channel radiometer and polarization analyser at wavelenghts around 12 m. The time and frequency resolutions were 10 ms and 100 kHz respectively. Observations on the duration, time profile and frequency splitting are described.
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