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Microwave Burst of November 17, 1991: Evidence of Fragmented Particle Injection into a Coronal Loop

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Abstract

The unusual event of November 17, 1991 07:04 UT, observed at 2.5 and 2.85 GHz, is analysed. The event reveals the sophisticated superfine time structure including sudden reductions and quasi-periodic pulsations. We shown that the sudden reductions (≈ 30–100 ms) can be driven by upward injected ≳ 100 keV electron beams filling the loss-cone of the coronal magnetic trap. The nonlinear oscillations of Langmuir waves provide the best fit for the pulsation observed. A reduced steady-state level of the pulsation phase is connected with quasi-continuous injection of electrons. The physical parameters of the radio source are found for the event.

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© 1994 Springer Science+Business Media Dordrecht

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Fleishman, G.D., Stepanov, A.V., Yurovsky, Y.F. (1994). Microwave Burst of November 17, 1991: Evidence of Fragmented Particle Injection into a Coronal Loop. In: Van den Oord, G.H.J. (eds) Fragmented Energy Release in Sun and Stars. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-1014-3_28

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  • DOI: https://doi.org/10.1007/978-94-011-1014-3_28

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-010-4441-7

  • Online ISBN: 978-94-011-1014-3

  • eBook Packages: Springer Book Archive

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