Analytic solutions of the magnetic annihilation and reconnection problems. II. Three-dimensional flows
Description
Analytic solutions for magnetic annihilation and reconnection in three-dimensional velocity fields are constructed. Exact and approximate solutions for three-dimensional fan current reconnection can be derived using prototype fields based on simple, one-component magnetic annihilation models. Certain reconnection solutions are found to be open-quotes fast,close quotes in the sense that the Ohmic dissipation rate scales independently of any positive power of the plasma resistivity η. Three-dimensional models can also possess novel features not contained in two-dimensional planar reconnection solutions. In particular, classes of solutions involving separated field nulls are found to possess multiple scalings for the Ohmic dissipation rate emdash a feature that has not been observed before. Several solutions are shown to have the potential to meet the extreme energy release characteristics of the solar flare. copyright 1997 American Institute of Physics
Additional details
Publishing Information
- Journal Title
- Physics of Plasmas
- Journal Volume
- 4
- Journal Issue
- 1
- Journal Page Range
- p. 110-119.
- ISSN
- 1070-664X
- CODEN
- PHPAEN
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 28032775
- Subject category
- S70: PLASMA PHYSICS AND FUSION TECHNOLOGY;
- Descriptors DEI
- ANALYTICAL SOLUTION; ELECTRIC CONDUCTIVITY; FLUID FLOW; MAGNETIC RECONNECTION; PLASMA DENSITY; PLASMA FLUID EQUATIONS; SOLAR FLARES; THREE-DIMENSIONAL CALCULATIONS
- Descriptors DEC
- BOLTZMANN-VLASOV EQUATION; DIFFERENTIAL EQUATIONS; ELECTRICAL PROPERTIES; EQUATIONS; PARTIAL DIFFERENTIAL EQUATIONS; PHYSICAL PROPERTIES; SOLAR ACTIVITY; STELLAR ACTIVITY; STELLAR FLARES