Energy spectrum of particles accelerated near a magnetic x line
- 1 July 1992
- journal article
- Published by American Geophysical Union (AGU) in Journal of Geophysical Research
- Vol. 97 (A7) , 10825-10830
- https://doi.org/10.1029/92ja00828
Abstract
We study the acceleration of test particles near a static magnetic x line with a uniform electric field and a strong component of the magnetic field, B∥, parallel to the x line. The energy spectrum of the accelerated particles is found analytically in the nonrelativistic limit, showing good agreement with numerical simulations. At high energies, the spectrum decays exponentially with a characteristic energy very different from that found in studies assuming B∥ = 0.Keywords
This publication has 8 references indexed in Scilit:
- Magnetic reconnection in collisionless plasmas: Prescribed fieldsJournal of Geophysical Research, 1990
- Symplectic integration of Hamiltonian systemsNonlinearity, 1990
- The structure and dissipation of forced current sheets in the solar atmosphereThe Astrophysical Journal, 1987
- Chaotic particle dynamics near a two‐dimensional magnetic neutral point with application to the geomagnetic tailJournal of Geophysical Research, 1986
- Solar flares and plasma instabilities: Observations, mechanisms and experimentsSolar Physics, 1976
- Possible Mechanism for the Acceleration of Ions in Some Astrophysical PhenomenaPhysical Review B, 1969
- 14. The neutral point theory of solar flaresSymposium - International Astronomical Union, 1958
- Sweet's mechanism for merging magnetic fields in conducting fluidsJournal of Geophysical Research, 1957