Abstract
We have studied three pairs of prominences, two of them clearly showing the effect of interaction by a dynamical plasma bridge. The other one was a superimposed optical pair which also showed, after being spectroscopically studied, the possible effect of interaction. We have calculated the atom density in the prominence and bridges, and applied the Goldberg-Unno method for the determination of Doppler-widths of the calcium H and K lines.
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References
Dunn, A. R. and Olson, E. C.: 1971, Solar Phys. 16, 272.
Engvold, O. and Livingston, W.: 1971, Solar Phys. 20, 375.
Goldberg, L.: 1958, Astrophys. J. 127, 308.
Goldberg, L., Mohler, O. C., and Müller, E. A.: 1959, Astrophys. J. 129, 119.
Gurtovenko, E. and Troyan, V.: 1971, Solar Phys. 20, 264.
Kleczek, J.: 1963, Bull. Astron. Inst. Czech. 14, 86.
Krat, V. A. and Krat, T. V.: 1971, Solar Phys. 17, 355.
Machado, M. E.: 1972, Solar Phys. 23, 353.
Olson, E. C.: 1966, Astrophys. J. 143, 912.
Roddier, F.: 1965, Ann. Astrophys. 28, 478.
Tandberg-Hanssen, E.: 1960, Astrophys. Norvegica 6, 161.
Unno, W.: 1959, Astrophys. J. 129, 375.
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Gallegos, H.G., Machado, M.E. Macroscopic motions in prominences. Sol Phys 31, 427–436 (1973). https://doi.org/10.1007/BF00152818
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DOI: https://doi.org/10.1007/BF00152818