Solar type V bursts

This is a news story, published by Astronomy & Astrophysics Group | University of Glasgow, that relates primarily to Langmuir news.

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single type III bursts

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type III bursts

Astronomy & Astrophysics Group | University of Glasgow

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Solar Radio Astronomy - CESRA

Summary

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88% Informative

Solar type V radio bursts are broad-band continua associated with type III bursts.

They appear sometimes for 0.2 to 3 minutes as a continuum following an intense type III burst or group of bursts.

Electron beams are two -stream unstable and drive Langmuir waves that couple into radio waves (type III burst).

If the emission is electron cyclotron maser and the magnetic scale height is the same as the density scale height, the velocity is 1/4 of the U-burst beam.

For both cases of emission, the data suggest that the Type V causing electrons have lower velocity than the type III causing electrons.

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