Abstract
A quiescent polar crown prominence was observed at Meudon in Hα and Ca ii lines, and by EIT and SUMER on board SOHO in UV lines from 9 to 10 March 1996. SUMER observed the prominence continuously in a scanning mode between 21:40 UT on 9 March, and 18:13 UT on 10 March, in the nitrogen line N v (λ1238) with a 1 arc sec2 resolution. Altogether 190 prominence images (121×108 pixels) were obtained. These are presented in a movie. The prominence is highly dynamic. Large-scale features, such as mixed loop systems and dark cavities are changing on time scales of a few hours. Filamentary structure is evident and is changing within a few frames of the movie. A lifetime of 20–25 min for the fine structure has been found by the autocorrelation method. We have statistically analysed the three moments of the N v line in the prominence: line intensity, Doppler shift and linewidth, in the context of a multiple-thread model. We find that the data are consistent with a model where the prominence is assumed to be an ensemble of small threads. In the brightest parts of the prominence it is possible that there are many unresolved threads (15–20) along the line of sight with diameters smaller than a few hundred kilometers. The filling factor is probably very small and in that case the structures occupy only a fraction of the volume.
This is a preview of subscription content, log in via an institution to check access.
Similar content being viewed by others
References
Chae, J., Yun, H. S., and Poland, A.I.: 1998, Astrophys. J. Suppl. Series 114, 151.
Dammasch, I. E., Wilhelm, K., Curdt, W., and Hassler, D. M.: 1999, Astron. Astrophys., in press.
Delaboudinière, J. P, Artzner, G. E., Brunaud, J., Gabriel, A. H., Hochedez J. F. et al.: 1995, Solar Phys. 162, 291.
Dere, K. P., Bartoe, J. D. F., Brueckner, G. E., Cook, J.W., and Socker, D. G.: 1987, Solar Phys. 114, 223.
Engvold, O.: 1976, Solar Phys. 49, 283.
Engvold, O., Jensen, E., Yi, Z., and Brynildsen, N.: 1989, in V. Ruždjak and E. Tandberg-Hanssen (eds.), IAU Colloq. 117, Hvar Bull. 13, 205.
Fontenla, J., Rovira, M., Vial, J. C., and Gouttebroze, P.: 1996, Astrophys. J. 466, 496.
Lemaire, P., Wilhelm, K., Curdt, W., Schühl, U., Marsch, E. et al.: 1997, Solar Phys. 170, 105.
Mein, P. and Mein, N.: 1991, Solar Phys. 136, 317.
Mein, N., Mein, P., and Wiik, J. E.: 1994, Solar Phys. 151, 75.
Mein, P., Mein, N., Schmieder, B., and Noëns, J. C.: 1989, in V. Ruždjak and E. Tandberg-Hanssen (eds.), IAU Colloq. 117, Hvar Bull. 13, 133.
Pojoga, S., Nikoghossian, A. G., and Mouradian, Z.: 1998, Astron. Astrophys. 332, 325.
Poland, A. I. and Tandberg-Hanssen, E.: 1983, Solar Phys. 84, 63.
Schmieder, B.: 1992, Solar Phys. 141, 275.
Tandberg-Hanssen, E.: 1974, Solar Prominences, D. Reidel Publ. Co., Dordrecht, Holland
Tandberg-Hanssen, E., Cheng, C. C., Woodgate, B. E., Brandt, J. C., Chapman, R. D. et al.: 1981, Adv. Space Res. 1 (13), 275.
Widing, K. G., Feldman, U., and Bhatia, A. K.: 1986, Astrophys. J. 308, 982.
Wiik, J. E., Dere, K., and Schmieder, B.: 1993, Astron. Astrophys. 273, 267.
Wilhelm, K., Curdt, W., Marsch, E., Schühle, U., Lemaire, P., Gabriel, A., Vial, J.-C., Grewing, M., Huber, M. C. E., Jordan, S. D., Poland, A. I., Thomas, R. J., Kühne, M., Timothy, J. G., Hassler, D. M., and Siegmund, O. H. W.: 1995, Solar Phys. 162, 189.
Wilhelm, K., Lemaire, P., Curdt, W., Schühle, U., Marsch, E., Poland, A. I., Jordan, S. D., Thomas, R. J., Hassler, D. M., Huber, M. C. E., Vial, J.-C., Kühne, M., Siegmund, O. H. W., Gabriel, A. H., Timothy, J. G., Grewing, M., Feldman, U., Hollandt, J., and Brekke, P.: 1997, Solar Phys. 170, 75.
Zirker, J. B. and Koutchmy, S: 1991, Solar Phys. 131, 107.
Author information
Authors and Affiliations
Electronic supplementary material
Rights and permissions
About this article
Cite this article
Wiik, J., Dammasch, I., Schmieder, B. et al. Multiple-Thread Model of a Prominence Observed by Sumer and eit on Soho. Sol Phys 187, 405–426 (1999). https://doi.org/10.1023/A:1005151015043
Issue Date:
DOI: https://doi.org/10.1023/A:1005151015043