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The birth of giant post-flare arches

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Abstract

Using short accumulation times, we have succeeded in the detection in HXIS images of the initial growth of the giant post-flare arch of 6 November, 1980 at 14:44 UT and part of the initial growth of the giant arch of 7 November, 1980 at 04:30 UT. These observations are relevant to the problem of the origin of giant arches: the fact that the arch of 6 November was imaged more than half an hour before the first flare loops had been recorded in the associated flare, proves that giant arches cannot: be interpreted as upper products of the reconnection process that creates the growing systems of flare loops (as the original interpretation by Švestka et al. (1982a) suggested). However, also the alternative hypothesis by Poletto and Kopp (1988) that these structures originate through a reconnection process in a peripheral, large-scale configuration meets with difficulties: after the initial rise, the maximum brightness in both arches seems to descend, until a much slower rise was resumed about two hours later.

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References

  • Achterberg, A. and Kuijpers, J.: 1984, Astron. Astrophys. 130, 111.

    Google Scholar 

  • Cargill, P. J. and Priest, E. R.: 1982, Solar Phys. 76, 357.

    Google Scholar 

  • Cargill, P. J. and Priest, E. R.: 1983, Astrophys. J. 266, 383.

    Google Scholar 

  • Fárník, F. Van Beek, H. F., and Švestka, Z.: 1986, Solar Phys. 104, 321.

    Google Scholar 

  • Heinzel, P. and Karlický, M.: 1987, Solar Phys. 110, 343.

    Google Scholar 

  • Hick, P.: 1988, ‘Interpretations of Energetic Phenomena in the Solar Corona’, Thesis, University of Utrecht.

  • Hick, P. and Priest, E. R.: 1989, Solar Phys. 122, 111.

    Google Scholar 

  • Hick, P. and Švestka, Z.: 1985, Solar Phys. 102, 147.

    Google Scholar 

  • Hick, P. and Švestka, Z.: 1987, Solar Phys. 108, 315.

    Google Scholar 

  • Hick, P., Švestka, Z., Smith, K. L., and Strong, K. T.: 1987, Solar Phys. 114, 329.

    Google Scholar 

  • Kopp, R. A. and Pneuman, G. W.: 1976, Solar Phys. 50, 85.

    Google Scholar 

  • Kopp, R. A. and Poletto, G.: 1990, Solar Phys. 127, 267.

    Google Scholar 

  • Martin, S. F., Švestka, Z., and Bhatnagar, A.: 1989, Solar Phys. 124, 339.

    Google Scholar 

  • Poletto, G. and Kopp, R. A.: 1988, Solar Phys. 116, 163.

    Google Scholar 

  • Poletto, G. and Švestka, Z.: 1990, Solar Phys. 129, 363.

    Google Scholar 

  • Švestka, Z.: 1984, Solar Phys. 94, 171.

    Google Scholar 

  • Švestka, Z.: 1986, in D. F. Neidig (ed.), The Lower Atmosphere of Solar Flares, National Solar Observatory/Sacramento Peak, p. 332.

  • Švestka, Z., Stewart, R., Hoyng, P., Van Tend, W., Acton, L. W., Gabriel, A. H., Rapley, C. G., and 8 co-authors: 1982a, Solar Phys. 75, 305.

    Google Scholar 

  • Švestka, Z., Dennis, B. R., Pick, M., Raoult, A., Rapley, C. G., Stewart, R. T., and Woodgate, B. E.: 1982b, Solar Phys. 80, 143.

    Google Scholar 

  • Švestka, Z., Fontenla, J. M., Machado, M. E., Martin, S. F., Neidig, D. F., and Poletto, G.: 1987, Solar Phys. 108, 237.

    Google Scholar 

  • Švestka, Z., Fárník, F., Fontenla, J. M., and Martin, S. F.: 1989, Solar Phys. 123, 317.

    Google Scholar 

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Poletto, G., Švestka, Z. The birth of giant post-flare arches. Sol Phys 138, 189–199 (1992). https://doi.org/10.1007/BF00146203

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  • DOI: https://doi.org/10.1007/BF00146203

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