Spatial localization and azimuthal wave numbers of Alfvén waves generated by drift-bounce resonance in the magnetosphere
Spatial localization and azimuthal wave numbers <i>m</i> of poloidal Alfvén waves generated by energetic particles in the magnetosphere are studied in the paper. There are two factors that cause the wave localization across magnetic shells. First, the instability growth rate...
Main Authors: | P. N. Mager, D. Yu. Klimushkin |
---|---|
Format: | Article |
Language: | English |
Published: |
Copernicus Publications
2005-12-01
|
Series: | Annales Geophysicae |
Online Access: | https://www.ann-geophys.net/23/3775/2005/angeo-23-3775-2005.pdf |
Similar Items
-
The spatio-temporal structure of impulse-generated azimuthalsmall-scale Alfvén waves interacting with high-energy chargedparticles in the magnetosphere
by: D. Yu. Klimushkin, et al.
Published: (2004-03-01) -
Numerical analysis of the spatial structure of Alfvén waves in a finite pressure plasma in a dipole magnetosphere
by: Petrashchuk A. V., et al.
Published: (2022-09-01) -
Alfvén ship waves: high-<I>m</I> ULF pulsations in the magnetosphere generated by a moving plasma inhomogeneity
by: P. N. Mager, et al.
Published: (2008-06-01) -
Generation of resonant Alfvén waves in the auroral oval
by: V. A. Pilipenko, et al.
Published: (2016-02-01) -
Theory of azimuthally small-scale hydromagnetic waves in the axisymmetric magnetosphere with finite plasma pressure
by: D. Y. Klimushkin, et al.
Published: (1998-03-01)