The modified two stream instability at nonmagnetic planets

Details The modified two stream instability at nonmagnetic planets The modified two stream instability at nonmagnetic planets

Dec 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1306....7b&link_type=abstract

NEW FRONTIERS IN ADVANCED PLASMA PHYSICS. AIP Conference Proceedings, Volume 1306, pp. 7-13 (2010).

Physics

Plasma Physics

Plasma Density, Solar Wind, Electron Beams, Disperse Systems, X-Ray Spectra, Dielectric Properties, Particle Emission, Solar Wind, Spin Dependence Of Cross Sections, Polarized Electron Beam Experiments, Emulsions And Suspensions, X-Ray Spectra

Scientific paper

We describe the role the modified two stream instability plays in the
interaction of the solar wind with non-magnetized planets. The
instability leads to the production of energetic electrons that can be
responsible for the observed x-ray emission.

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