Magnetic mirror force in plasma fluid models
Creators
Description
In the past decade, there have been several attempts to include the magnetic mirror force in the equation of motion for a plasma in a fluid formalism. In the process, some confusion has been evident regarding when and how this should be done. This problem has been addressed in the literature, but these treatments appear to have been forgotten or misunderstood. The mathematical arguments are summarized so that the physical consequences are readily perceived. It is shown that for an isotropic plasma fluid, in the direction parallel or anti-parallel to a magnetic field, the forces associated with a diverging magnetic field cancel out. Only for anisotropies in the fluid properties does the diverging field influence the plasma dynamics. 12 references
Additional details
Publishing Information
- Publisher
- American Geophysical Union.
- Imprint Place
- Washington, DC (USA)
- Imprint Title
- Modeling magnetospheric plasma; Proceedings of the First Huntsville Workshop on Magnetosphere/Ionosphere Plasma Models, Guntersville, AL, Oct. 14-16, 1987
- Journal Page Range
- p. 51-53.
Conference
- Title
- 1. Huntsville workshop on magnetosphere/ionosphere plasma models.
- Dates
- 14-16 Oct 1987.
- Place
- Guntersville, AL (USA).
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 20033409
- Subject category
- S58: GEOSCIENCES;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- DYNAMICS; EARTH MAGNETOSPHERE; EQUATIONS OF MOTION; ISOTROPY; KINETIC EQUATIONS; MAGNETIC FIELDS; MAGNETIC MIRRORS; MATHEMATICAL MODELS; PLASMA
- Descriptors DEC
- DIFFERENTIAL EQUATIONS; EARTH ATMOSPHERE; EQUATIONS; MECHANICS; OPEN PLASMA DEVICES; PARTIAL DIFFERENTIAL EQUATIONS; THERMONUCLEAR DEVICES