Magnetic reconnection in high-temperatur
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B. V. Somov; A. I. Verneta
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Article
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1988
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Springer
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English
โ 327 KB
Quasi-steady high-temperature current sheets are an energy source during the 'main' or 'hot' phase of solar flares. Such sheets are shown to be stabilized with respect to the tearing instability by a small transverse component of magnetic field existing in the sheets. \* Send offprint requests to B.