Collisionless Dynamo
- 12 September 1994
- journal article
- research article
- Published by American Physical Society (APS) in Physical Review Letters
- Vol. 73 (11) , 1509-1512
- https://doi.org/10.1103/physrevlett.73.1509
Abstract
Electron inertia is shown to dramatically impact the generation of a magnetic field by a flowing collisionless plasma. The rate at which magnetic field energy is created by the flow remains large as the magnetic Reynolds number , for both chaotic and nonchaotic flows. Importantly, a continuous nonchaotic laminar flow generates a magnetic field in a collisionless (zero collisional diffusion) plasma because of electron inertia. The magnetic field generated lies in a series of flux bundles with a scale size given by the collisionless electron skin depth.
This publication has 17 references indexed in Scilit:
- Fast dynamos with finite resistivity in steady flows with stagnation pointsPhysics of Fluids B: Plasma Physics, 1993
- Chaotic flows and fast magnetic dynamosPhysics of Fluids, 1988
- Chaotic flows and magnetic dynamosPhysical Review Letters, 1988
- Fast dynamo action in unsteady flows and maps in three dimensionsPhysical Review Letters, 1987
- Fast dynamo action in a steady flowJournal of Fluid Mechanics, 1987
- A high magnetic Reynolds number dynamoPhysics of Fluids, 1987
- Dynamo action in a family of flows with chaotic streamlinesGeophysical & Astrophysical Fluid Dynamics, 1986
- Topological constraints associated with fast dynamo actionJournal of Fluid Mechanics, 1985
- Kinematic dynamo in random flowSoviet Physics Uspekhi, 1985
- Alpha-effect in flux ropes and sheetsPhysics of the Earth and Planetary Interiors, 1979