Abstract
Methods for the observation of chromospheric spicules with the large coronagraph mounted at the High Altitude Astronomical Station near Kislovodsk are described. The Hα-spectrograms and the filtergrams obtained by an Hα-Halle birefringent filter are shown. Some results of the observations and some conclusions on the structure of the chromosphere are reported.
This is a preview of subscription content, log in via an institution to check access.
Similar content being viewed by others
References
Beckers, J. M.: 1968, Solar Phys. 3, 367.
Bhavilai, R., Norton, G., and Giovanelli, R. G.: 1965, Astrophys. J., 141, 274.
Gnevyshev, M. N., Nikolsky, G. M., and Sazanov, A. A.: 1967, Solar Phys. 2, 233.
Lyot, B.: 1932, L'Astronomie 46, 272; Compt. Rend. Acad. Sci. (France) 194, 443.
Nikolsky, G. M. and Sazanov, A. A.: 1966, Astron. Zh. 43, 928.
Pasachoff, J. M., Noyes, R. W., and Beckers, J. M.: 1969, Solar Phys. 5, 131.
Sazanov, A. A.: 1967, Soln. Dann. No. 12, 90.
Simon, G. W. and White, O. R.: 1966, Astrophys. J. 143, 38.
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Nikolsky, G.M. The observation of the chromospheric fine structure by the 53-cm lyot coronagraph. Sol Phys 12, 379–390 (1970). https://doi.org/10.1007/BF00148021
Received:
Issue Date:
DOI: https://doi.org/10.1007/BF00148021