Growth of the Langmuir cavity eigenmodes in the solar wind

Details Growth of the Langmuir cavity eigenmodes in the solar wind Growth of the Langmuir cavity eigenmodes in the solar wind

Oct 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010jgra..11510103h&link_type=abstract

Journal of Geophysical Research, Volume 115, Issue A10, CiteID A10103

Physics

Plasma Physics

2

Interplanetary Physics: Solar Wind Plasma, Interplanetary Physics: Solar Cycle Variations (7536), Space Plasma Physics: Kinetic Waves And Instabilities, Radio Science: Radio Astronomy, Radio Science: Waves In Plasma (7867)

Scientific paper

The Langmuir waves in the solar wind are known to be at the origin of many types of solar radio emissions, in particular solar type II and type III radio bursts. In situ observations have shown that the largest amplitude Langmuir waves often appear as localized wave packets. Several models have been proposed to explain this localization of the waves, such as kinetic localization, nonlinear wave-wave processes, or eigenmode formation. The latter theory states that the wave packets are eigenmodes of density cavities generated by background turbulence. In the present paper we investigate the wave growth of the localized Langmuir eigenmodes.

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