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The lifetime and evolution of fibrils

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Abstract

A detailed study has been made of the lifetimes and evolution of fibrils in McMath 12417, using high resolution filtergrams in Hα and Ca ii K made at Big Bear Solar Observatory. It was found that when viewed near disk centre, the lifetime of a fibril is a monotonically increasing function of its maximum apparent length. This relationship, together with the form of the variation of fibril lengths as a function of time, suggests that fibrils result from material being impulsively injected into magnetic field lines at approximately 30 km s, and returning under gravity. The lifetimes and apparent lengths of fibrils are then a function of the inclination of the field lines only. A study of wavelength scans through the Hα line confirms that the apparent extension and retraction of fibrils represents true mass motion.

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References

  • Beckers, J. M. 1964, Thesis, Utrecht.

  • Beckers, J. M. 1968, Solar Phys. 3, 367.

    Google Scholar 

  • Beckers, J. M. 1972, Ann. Rev. Astron. Astrophys. 10, 73.

    Google Scholar 

  • Bray, R. J. 1973, Solar Phys. 29, 317.

    Google Scholar 

  • Bray, R. J. 1974, Solar Phys. 38, 377.

    Google Scholar 

  • Bray, R. J., and Loughhead, R. E. 1974, The Solar Chromosphere, Chapman and Hall (London), p. 214.

    Google Scholar 

  • Foukal, P. 1971, Solar Phys. 20, 298.

    Google Scholar 

  • Grossman-Doerth, V., and von Uexküll, M. 1971, Solar Phys. 20, 31.

    Google Scholar 

  • Loughhead, R. E. 1968, Solar Phys. 5, 489.

    Google Scholar 

  • Smith, S. F. 1968, in K. O. Kiepenheuer (ed.), ‘Structure and Development of Solar Active Regions’, IAU Symp. 35, 267.

  • Tanaka, K. 1972, Big Bear Solar Observatory preprint #0125.

  • Tanaka, K. 1974, in R. Grant Athay (ed.), ‘Chromospheric Fine Structure’, IAU Symp. 56, 239.

  • Zirin, H. 1974, Solar Phys. 38, 91.

    Google Scholar 

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Marsh, K.A. The lifetime and evolution of fibrils. Sol Phys 50, 37–48 (1976). https://doi.org/10.1007/BF00206188

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  • DOI: https://doi.org/10.1007/BF00206188

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