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Polarization properties of the June 21, 2001 solar corona

Published online by Cambridge University Press:  01 November 2006

N. G. Kapanadze ,
V. I. Kulijanishvili  and
Ahmed A. Hady
N. G. Kapanadze
Affiliation:
E. Kharadze Abastumani Astrophysical Observatory, Al. Kazbegi ave.2a, 380060 Tbilisi, Georgia email: kvazha@yahoo.com
V. I. Kulijanishvili
Affiliation:
E. Kharadze Abastumani Astrophysical Observatory, Al. Kazbegi ave.2a, 380060 Tbilisi, Georgia email: kvazha@yahoo.com
Ahmed A. Hady
Affiliation:
Astronomy Dept., Faculty of Sciences Cairo University, 12613 – Giza, Egypt
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Abstract

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Five series of coronal images have been obtained by V.Kulijanishvili during the total solar eclipse of the June 21, 2001, in Zambia, Lusaka. A photographic mirror-lens coronagraph-polarimeter (D=100 mm, F=1000 mm) was used. The absolute brightness, polarization and direction of polarization of the inner corona were measured. Standard techniques are used for the separation of the F- and K-coronas and for determination of coronal electron densities and temperatures. The background skylight polarization and intensity are calculated.

Keywords

CoronaEclipsesPolarimetersHydrodynamics
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Symposium S233: Solar Activity and its Magnetic Origin , March 2006 , pp. 255 - 256
Copyright
© 2006 International Astronomical Union