Electron Acoustic Waves: Gyro-tropic Transport Equations of the Solar Wind

Details Electron Acoustic Waves: Gyro-tropic Transport Equations of the Solar Wind Electron Acoustic Waves: Gyro-tropic Transport Equations of the Solar Wind

May 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aas...21631203l&link_type=abstract

American Astronomical Society, AAS Meeting #216, #312.03; Bulletin of the American Astronomical Society, Vol. 41, p.887

Computer Science

Sound

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Linear compressive waves are numerically simulated using two fluid gyro-tropic transport equations for the solar wind flows. A low frequency (much lower than proton gyro-frequency) driver introduced at the corona can excite both ion sound wave and a much faster wave propagating into interplanetary space along the open magnetic field lines. The phase speed of the faster wave is the order of electron thermal speed: the wave can be much faster than an ion sound wave or an Alfvén wave. We will discuss the implications of our result for the corona and solar wind studies.

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