Abstract
As a summary of this paper I am presenting a table which is in a very similar format as I have presented in the former IAU colloquium (Hirayama, 1978), and according change was made. Though the present study did not cover much about post flare loops, and erupting prominences (and nothing was said on surges and active region filaments), they are also included for comparison.
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Hirayama, T. (1990). Physical conditions in 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/BFb0025649
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DOI: https://doi.org/10.1007/BFb0025649
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