Physics – Optics
Scientific paper
Aug 2006
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006iaujd...8e..41h&link_type=abstract
Solar and Stellar Activity Cycles, 26th meeting of the IAU, Joint Discussion 8, 17-18 August 2006, Prague, Czech Republic, JD08,
Physics
Optics
Scientific paper
White light observations of the inner and outer corona during the 29th March, 2006 total solar eclipse have been made by advanced observing technology consisting of a top quality William's optics 110mm/0.715mn refractor and Cannon Eos MARCII digital camera controlled by computer. The whole observing complex was mounted on the Losmandy parallactic mount, precisely following the sun path on the sky. The achieved resolution on the focal plane of the camera is about one arc sec. The photographed white light corona shows extension up to 5 solar radii and displays many arcade structures, Helmet streamers and polar streamers which can be identified with calculated magnetic field lines.
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