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The White-Light, Far-Red (600-700 nm) and Emission Coronae at the July 11, 1991 Eclipse

Published online by Cambridge University Press:  03 August 2017

V. Rušin ,
M. Rybanský ,
M Minarovjech  and
T. Pintér
V. Rušin
Affiliation:
Astronomical Institute, Slovak Academy of Sciences, 059 60 Tatranská Lomnica, Czecho-Slovakia
M. Rybanský
Affiliation:
Astronomical Institute, Slovak Academy of Sciences, 059 60 Tatranská Lomnica, Czecho-Slovakia
M Minarovjech
Affiliation:
Astronomical Institute, Slovak Academy of Sciences, 059 60 Tatranská Lomnica, Czecho-Slovakia
T. Pintér
Affiliation:
The Slovak Centre of Amateur Astronomy, 947 01 Hurbanovo, Czecho-Slovakia

Abstract

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Preliminary results of the analysis of the white-light, emission (green and red), and far red (600-700 nm) corona during the July 11, 1991 eclipse are given. Even though the corona is of nearly-maximum type, four different principal coronal structures are seen, combined with faint, small-scale structures (loops, arches, cavities, voids or plasmoids). Scattered light is seen up to 10 R ⊙ in helmet streamers. The Ludendorff index of the corona shape turns out to be a + b = −0.02, and the estimated brightness of JK = 1.47 × 10–6B ⊙. Some aspects of multiwavelength observations are discussed.

Keywords

eclipsesSun: corona
Type
Part 2: Infrared Observations of the 1991 Total Solar Eclipse
Information
Symposium - International Astronomical Union , Volume 154: Infrared Solar Physics , 1994 , pp. 211 - 215
Copyright
Copyright © Kluwer 1994 

References

Chochol, D., Rušin, V., Kulčár, L., and Vanýsek, V.: 1983, Astrophys. Space Sci. 91, 71.Google Scholar
Koutchmy, S.: 1977, in Durrant, C. J. and Bruzek, A. (eds.), Illustrated Glossary for Solar and Solar-Terrestrial Physics, Reidel, Dordrecht, p. 39.Google Scholar
MacQueen, R.M., Hodapp, K-W., and Hall, D.N.B.: 1993, these proceedings.Google Scholar
Marková, E., Vyskočil, L., Rušin, V., and Rybanský, M.: 1992, Solnechnyje Dannyje, in press.Google Scholar
Rušin, V., and Rybanský, M.: 1985, Bull. Astron. Inst. Czechosl., 77, 81.Google Scholar
Zirker, J.B., Koutchmy, S., Nitschelm, C., Stellmacher, G., Zimmermann, J.P., Martinez, P., Kim, I., Dzjubenko, N., Kurochka, L., Makarov, V., Fatianov, M., Rusin, V., Klocok, L., and Matsuura, O.T.: 1992, Astron. Astrophys., in press.Google Scholar