NASA NTRS · 19840064010
Nonlinear computations of a solar flare model
Abstract
A cylindrical axisymmetric tearing mode model for solar flares is investigated numerically. Large magnetic energy release only occurs when there are at least two mode rational surfaces in the current-carrying plasma.
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Strauss, H., Van Hoven, G.. 1984-08-01. Nonlinear computations of a solar flare model. https://ntrs.nasa.gov/citations/19840064010
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