Perpendicular electron trapping associated with nonlinear whistlers
- 1. Department of Physics, University of Pisa and INFM, Pz. Torricelli 2, Pisa (Italy)
- 2. International Centre for Theoretical Physics, P.O. Box 586, I-34100 Trieste (Italy)
- 3. Institute of Physics, P.O. Box 57, Yu-11001 Belgrade (Serbia and Montenegro)
Description
Kinetic effects leading to the particle trapping are studied in a magnetized, inhomogeneous plasma configuration within the framework of the gyrokinetic theory in the frequency and spatial scale range that corresponds to the whistler waves. This treatment accounts for finite electron Larmor radius and polarization effects. A coherent nonlinear structure is found, which is identified as a magnetic vortex coupled with an electron hole. This novel electron hole is characterized by a strong magnetic field, and has a typical perpendicular size somewhat shorter than the electron collisionless skin depth. Electrons are trapped in the perpendicular direction by the combination of the electrostatic field, arising from the charge separation, and of the Lorentz force resulting from the propagation of the structure relative to the perturbed magnetic field lines. The trapping effects are restricted to the region at the center of the vortex. The size of this region is related to the electron Larmor-radius and to the Debye length
Additional details
Identifiers
- DOI
- 10.1063/1.1374586;
Publishing Information
- Journal Title
- Physics of Plasmas
- Journal Volume
- 8
- Journal Issue
- 7
- Journal Page Range
- p. 3217-3226
- ISSN
- 1070-664X
- CODEN
- PHPAEN
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 35035914
- Subject category
- S70: PLASMA PHYSICS AND FUSION TECHNOLOGY;
- Descriptors DEI
- LARMOR RADIUS; PLASMA WAVES; POLARIZATION; TRAPPED ELECTRONS; WAVE PROPAGATION; WHISTLERS
- Descriptors DEC
- ELECTROMAGNETIC RADIATION; ELECTRONS; ELEMENTARY PARTICLES; FERMIONS; LEPTONS; NOISE; RADIATIONS; RADIO NOISE; RADIOWAVE RADIATION
Optional Information
- Notes
- (c) 2001 American Institute of Physics.