NASA NTRS · 19730002063
Magnetic field merging in the solar wind
Abstract
Magnetic field merging in the solar wind is discussed in terms of steady-state merging, which involves a steady flow field, and of spontaneous merging, which involves an instability such as the tearing instability. Spontaneous merging is found to be more effective than steady-state merging.
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Schindler, K.. 1972-01-01. Magnetic field merging in the solar wind. https://ntrs.nasa.gov/citations/19730002063
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