A Comparison of the Red and Green Coronal Line Intensities at the 29 March 2006 and the 1 August 2008 Total Solar Eclipses: Considerations of the Temperature of the Solar Corona

During the total solar eclipse at Akademgorodok, Siberia, Russia, on 1 August 2008, we imaged the flash spectrum with a slitless spectrograph. We have spectroscopically determined the duration of totality, the epoch of the second and third contacts and the duration of the flash spectrum. Here we com...

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Veröffentlicht in:Solar physics 2010-06, Vol.264 (1), p.45-55
Hauptverfasser: Voulgaris, A., Athanasiadis, T., Seiradakis, J. H., Pasachoff, J. M.
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Sprache:eng
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