Abstract
An equation describing ballooning modes localized to a magnetic field line embedded in rotating plasma is derived and analyzed. On a typical ballooning growth time these modes may be completely stabilized by shear in the flow, in a way which appears to be simple to achieve experimentally. Their long-time behavior is more complicated.
Original language | English (US) |
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Pages (from-to) | 1186-1189 |
Number of pages | 4 |
Journal | Physical Review A |
Volume | 41 |
Issue number | 2 |
DOIs | |
State | Published - 1990 |
ASJC Scopus subject areas
- Atomic and Molecular Physics, and Optics