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Title: Linear instabilities in multicomponent plasmas and their consequences for the auroral zone

Journal Article · · J. Geophys. Res.; (United States)

Ion conics are commonly observed along auroral zone field lines and involve all major terrestrial ion species, including hydrogen, helium, and oxygen. It is believed that low-frequency plasma waves, driven unstable by field-aligned currents, transversely heat the ion distributions via wave-particle interactions, creating the ion conics. Considered here are low-frequency, oblique, electrostatic instabilities found in a mixed plasma that includes an electron beam streaming through a background of electrons, hydrogen, and oxygen. The addition of oxygen not only modifies the lower hybrid frequency, but allows the existence of an ion-ion (Buchsbaum) hybrid mode with a frequency between the hydrogen and oxygen gyrofrequencies. Because of its low frequency, the ion-ion hybrid instability can be effective in transversely heating heavy ions. When the electron beam drift speed is greater than 3 times the background electron thermal velocity (V/sub 0/>3v/sub te/) and the electron gyrofrequency to plasma frequency ratio is less than 10 (..cap omega../sub e/..omega../sub pe/<10), the lower hybrid instability dominates. However, for ..cap omega../sub e/..omega../sub pe/>20, which is a condition commonly found in the auroral zone nightside region, the ion-ion instability has the largest growth rates; in these regions, heavy ion transverse heating can occur. When 10<..cap omega../sub e/..omega../sub pe/<20 the hydrogen to oxygen density ratio determines which instability dominates. copyright American Geophysical Union 198

Research Organization:
Department of Physics, University of California at Los Angeles
OSTI ID:
5190306
Journal Information:
J. Geophys. Res.; (United States), Vol. 93:A4
Country of Publication:
United States
Language:
English