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Mass motion in and around prominences

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Dynamics of Quiescent Prominences

Part of the book series: Lecture Notes in Physics ((LNP,volume 363))

Abstract

The mass of a quiescent prominence is equivalent to one-tenth of the all coronal plasma. It is obvious that this crucial problem is resolved, now if we consider the dynamical nature of prominences. Observations of motions of filaments will be reviewed in regard to their time scales:

  1. .

    solar cycle (slow migration of filaments, pivot points, convection)

  2. .

    days or hours (stationary motions, oscillations)

  3. .

    hours or minutes (appearance or disparition brusque, eruption)

These motions will be discussed in view of a better understanding of the formation of filaments (chromospheric injection or coronal plasma condensation), stability of the fine structures, existence of the feet, relationship of the DB, and the coronal mass ejections.

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V. Ruždjak E. Tandberg-Hanssen

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Schmieder, B. (1990). Mass motion in and around prominences. In: Ruždjak, V., Tandberg-Hanssen, E. (eds) Dynamics of Quiescent Prominences. Lecture Notes in Physics, vol 363. Springer, Berlin, Heidelberg. https://doi.org/10.1007/BFb0025644

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  • DOI: https://doi.org/10.1007/BFb0025644

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