Non-resonant beam instability driven by the ring-beam ion distribution
Source abstract
Abstract
Beams are one of the features that nearly commonly appear in various plasma realizations in nature. A systematic study of non-resonant ion-beam instability is presented for the ring-beam distribution, corresponding to a gyrotropic, helical beam along the large-scale magnetic field. We work on the rationalized, polynomial dispersion relation of the fourth-order and obtain the wave properties (dispersion relation) and the instability profile (the growth rate) at low and high beam speeds. The beam instability shows a smooth transition from the right-hand resonant instability at a moderate beam velocity to the non-resonant instability at a higher beam velocity. Moreover, the non-resonant beam instability occurs both forward and backward with respect to the beam direction. The non-resonant mode reduces to the firehose instability of anisotropic magnetohydrodynamics in the long-wavelength limit, where the beam component virtually serves as the field-aligned pressure. Simultaneous excitation of both the resonant and the non-resonant beam instabilities is possible at distinct wavelengths if the beam has a ring distribution, indicating that the set of the excited wave frequencies or wavelengths serves as a fingerprint of the ring-beam distribution.
Source: crossref · Quality: baseline
Research context
OpenAlex topics: Magnetic confinement fusion research · Dust and Plasma Wave Phenomena · Ionosphere and magnetosphere dynamics
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
Affiliations
Institut für Theoretische Physik, Technische Universität Braunschweig 1 , Mendelssohnstr. 3, D-38106 Braunschweig,
Max Planck Institute for Solar System Research 2 , Justus-von-Liebig-Weg 3, D-37077 Göttingen,
References (27)
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