Detection of langmuir solitons: implications for type III burst emission mechanisms at 2ω PE

Details Detection of langmuir solitons: implications for type III burst emission mechanisms at 2ω PE Detection of langmuir solitons: implications for type III burst emission mechanisms at 2ω PE

Mar 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996ap%26ss.243..195t&link_type=abstract

Astrophysics and Space Science, Volume 243, Issue 1, pp.195-198

Astronomy and Astrophysics

Astrophysics

4

Langmuir Solitons, Type Iii Bursts

Scientific paper

We present the experimental verification of existing theoretical models of emission mechanisms of solar type III bursts at the second harmonic of the plasma frequency, ω pe . This study is based on the detection of Langmuir and envelope solitons by the Ulysses spacecraft inside three type III burst source regions. We show that the oscillating-two-stream instability, coherent radiation by Langmuir solitons and stochastic phase mixing of the Langmuir waves in the strong turbulence regime are the appropriate emission mechanisms at 2ω pe .

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