Origin of low-frequency Alfven waves in the solar wind

Details Origin of low-frequency Alfven waves in the solar wind Origin of low-frequency Alfven waves in the solar wind

Jun 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986azh....63..542c&link_type=abstract

(Astronomicheskii Zhurnal, vol. 63, May-June 1986, p. 542-549) Soviet Astronomy (ISSN 0038-5301), vol. 30, May-June 1986, p. 322

Astronomy and Astrophysics

Astronomy

10

Atmospheric Boundary Layer, Boundary Layer Transition, Low Frequencies, Magnetohydrodynamic Waves, Plasma Dynamics, Solar Wind, Atmospheric Models, Chromosphere, Solar Atmosphere, Solar Corona, Solar Magnetic Field, Stellar Models

Scientific paper

The problem is considered of the localization of the source of Alfvén waves with periods ⪆5 min observed in the solar wind. The conclusion is drawn that the waves are generated in the region near the transition layer (upper chromosphere and lower corona). A comparison is carried out of the models of the solar atmosphere with a homogeneous and a strongly inhomogeneous (tubes) magnetic field. The form of the power spectrum of the outgoing Alfvén waves is discussed.

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