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A possible observational test to distinguish between slow and transient current buildup prior to solar flares

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Abstract

A possible diagnostic for differentiating between a slow and a transient buildup of current prior to a flare is developed. It is noted that if this diagnostic can be realized in practice, it will yield information not only on the rate the current is built up, but also on the magnitude of the electric field that is precipitating the buildup.

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References

  • Dreicer, H.: 1959, Phys. Rev. 115, 238.

    Google Scholar 

  • Jordan, C.: 1976, Philos. Trans. Roy. Soc. London A281, 391.

    Google Scholar 

  • Kadomtsev, B. B. and Pogutse, O. P.: 1968, Soviet Phys. JETP 26, 1146.

    Google Scholar 

  • Kruskal, M. and Bernstein, I. B.: 1964, Phys. Fluids 7, 407.

    Google Scholar 

  • Liu, C. S. and Mok, Y.: 1977, Phys. Rev. Letters 38, 168.

    Google Scholar 

  • Liu, C. S., Mok, Y. C., Papadopoulos, K., Engelmann, F., and Bornatici, M.: 1977, Phys. Rev. Letters 39, 701.

    Google Scholar 

  • Spitzer, L.: 1962, Physics of Fully Ionized Gases, Wiley, New York.

    Google Scholar 

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Spicer, D.S. A possible observational test to distinguish between slow and transient current buildup prior to solar flares. Sol Phys 64, 121–128 (1979). https://doi.org/10.1007/BF00151120

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  • DOI: https://doi.org/10.1007/BF00151120

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