Ion Cyclotron Resonant Instability of RH Waves Propagating at an Angle to the Interplanetary Magnetic Field

Details Ion Cyclotron Resonant Instability of RH Waves Propagating at an Angle to the Interplanetary Magnetic Field Ion Cyclotron Resonant Instability of RH Waves Propagating at an Angle to the Interplanetary Magnetic Field

Nov 1969

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1969ap%26ss...5..333c&link_type=abstract

Astrophysics and Space Science, Volume 5, Issue 3, pp.333-341

Astronomy and Astrophysics

Astrophysics

4

Scientific paper

The anomalous Doppler-shift interaction between positive ions and right-hand (RH) polarized E.M. waves propagating at a small angle to a static magnetic field is investigated. The linear rate of growth of the resulting instability is obtained and compared with the growth rate for the parallel propagation case. For conditions typical of the solar wind at about 1 AU, the rate of growth always decreases with increasing propagation angle. For very large ion pressures (β‖≫1) and temperature anisotropies (T ‖ T ⊥≫1), the rate of growth may increase with increasing propagation angle.

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