Abstract
In the late phase of some complex flare events which produce type IV radio emission, a narrow-band decimetric component with generally a high abundance of spectral fine structures is observed. We identify this late dm continuum as a hypothetical ‘switch-off’ signature of the equivalent two-ribbon flare current system. The quasi-periodic and highly dynamic fiber-burst pattern studied in the February 5, 1986 example is understood as radio evidence for a final reactivation of a cyclic sequence of instabilities in the driven reconnecting current sheet below the rising prominence.
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Aurass, H., Kliem, B. Fiber bursts in type IV dm radio continua as a signature of coronal current sheet dynamics. Sol Phys 141, 371–379 (1992). https://doi.org/10.1007/BF00155186
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DOI: https://doi.org/10.1007/BF00155186