A broadband theory of Langmuir-whistler events in the solar wind

Details A broadband theory of Langmuir-whistler events in the solar wind A broadband theory of Langmuir-whistler events in the solar wind

Aug 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999a%26a...348l..13l&link_type=abstract

Astronomy and Astrophysics, v.348, p.L13-L16 (1999)

Astronomy and Astrophysics

Astrophysics

3

Plasmas, Sun: Solar Wind, Turbulence

Scientific paper

Recent interplanetary observations presented evidence of simultaneous excitation of high-frequency Langmuir waves and low-frequency electromagnetic whistler waves in the magnetic holes of the solar wind. In this letter, we formulate a broadband theory of the interplanetary Langmuir-whistler events. We show that whistler waves can grow exponentially as a result of nonlinear interactions of Langmuir waves and left-hand circularly polarized radio waves. In particular, the growth of whistler waves favors propagation parallel to the Langmuir waves.

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