Abstract
A statistical large-scale study of filaments has revealed the existence of a functional dependence of the length of filaments (the angular distance between the ends of a filament, measured on a great circle on a sphere) on their inclination to lines of solar latitude. A cluster analysis method has been applied to the study of filament evolution and an evolutionary classification of filaments is proposed. The results depend on the differential velocity of filaments. Different types of evolution sequences were obtained, and the evolution of some particular filaments was specially analyzed.
Similar content being viewed by others
References
Adams, F. M. and Tang, F.: 1977, Solar Phys. 55, 499.
d’Azambuja, L. and d’Azambuja, M.: 1948, Ann. Obs. Paris, tome 6, fascicule 7.
Brajša et al.: 1989, Hvar Obs. Bull. 13, 448.
Craiu, V.: 1972, Verificarea ipotezelor statistice, Editura Didactica si Pedagogica, Bucharest.
de Jager, C.: 1959, in S. Fl¨ugge (ed.), Handbuch der Physik 52, 80.
Démoulin, P. and Priest, E. R.: 1989, Astron. Astrophys. 214, 360.
Démoulin, P. and Vial, J. C.: 1992, Solar Phys. 141, 289.
Démoulin, P., Raadu, M. A., and Malherbe, J. M.: 1992, Astron. Astrophys. 257, 278.
Dumitrache, C.: 1994, in A. v. Alvensleben (ed.), JOSO Ann. Report, p. 134.
Dumitrache, C.: 1995a, in P. Saniga (eds.), JOSO Ann. Report p. 181.
Dumitrache, C.: 1995b, Contribution to JENAM’95.
Dumitrache, C., Dinulescu, S., and Priest, E. R.: 1994, in G. Belvedere, M. Rodono, Schmieder, and G. M. Simnett (eds.), Publ. Obs. Astrof. Catania, Special Volume, p. 65.
Fisher, N. I., Lewis, T., and Embleton, B. J. J.: 1993, Statistical Analysis of Spherical Data, Cambridge University Press, Cambridge.
Hirayama, T.: 1985, Solar Phys. 100, 415.
Hood, A. W. and Priest, E. R.: 1979a, Astron. Astrophys. 77, 233.
Hood, A. W. and Priest, E. R.: 1979b, Solar Phys. 64, 303.
Howard, R. F.: 1992, Solar Phys. 123, 271.
Howard, R. F.: 1993, Solar Phys. 140, 95.
Iosifescu, M., Moineanu C., Trebici V., and Ursianu, E.: 1985, Mica enciclopedie de statistica, Editura Stiintifica si Enciclopedica, Bucharest.
Kiepenheuer, K. O.: 1953, in G. Kuiper (ed.), The Sun, Chicago University Press, Chicago, Ch. 4.
Kim, I.: 1989, preprint 11, GAIS, Sternberg State Astronomical Institute.
Kuperus, M. and Tandberg-Hanssen, E.: 1967, Solar Phys. 2, 39.
Kuperus, M. and Raadu, M. A.: 1974, Astron. Astrophys. 31, 189.
Leroy, J. L.: 1989, in E. R. Priest (ed.), Dynamics and Structures of Quiescent Solar Prominences, D. Reidel Publ. Co., Dordrecht, Holland, p. 77.
Leroy, J. L., Bommier, V., Sahal-Bréchot, S.: 1984, Astron. Astrophys. 13, 33.
Malherbe, J. H. and Priest, E. R.: 1983, Astron. Astrophys. 123, 80.
Martin, S. F.: 1973, Solar Phys. 31, 3.
Mouradian, Z. and Soru-Escaut, I.: 1989, Astron. Astrophys. 210, 410.
Priest, E. R.: 1982, Solar Magnetohydrodynamics, D. Reidel Publ. Co., Dordrecht, Holland.
Priest, E. R. (ed.): 1988, The Structure and Dynamics of Quiescent Solar Prominences, D. Reidel Publ. Co., Dordrecht, Holland, p. 6.
Priest, E. R. and Smith, E. A.: 1979, Solar Phys. 64, 267.
Priest, E. R., Hood, A. W., and Anzer, U.: 1989, Astrophys J. 344, 1010.
Rausaria, R. R., Sundara Raman, K., Aleen, P. S. M., and Singh, J.: 1993, Solar Phys. 146, 137.
Smith, E. A. and Priest, E. R.: 1977, Solar Phys. 53, 25.
Solnechnye Dannye Bulletin: 1987-1989, Pulkovo Observatory.
Wright, C. S.: 1991, Catalogue of Solar Filament Disappearances 1964-1980, in Rep. UAG-100, WDC-A, NGDC, U.S.A.
Zwaan, C.: 1990, Publ. Debrecen Heliophys. Obs. 7, 67.
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Dumitrache, C. ON THE EVOLUTION OF FILAMENTS. Solar Physics 173, 281–304 (1997). https://doi.org/10.1023/A:1004900127858
Issue Date:
DOI: https://doi.org/10.1023/A:1004900127858