Coronal temperature during total solar eclipses at the extended solar minimum of solar cycle 23

Details Coronal temperature during total solar eclipses at the extended solar minimum of solar cycle 23 Coronal temperature during total solar eclipses at the extended solar minimum of solar cycle 23

Jan 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012hell.confr..13s&link_type=abstract

10th Hellenic Astronomical Conference, Proceedings of the conference held at Ioannina, Greece, 5-8 September 2011. Edited by Io

Astronomy and Astrophysics

Astronomy

Scientific paper

Coronal temperature diagnostics are essential for the general understanding of coronal properties during a solar cycle. With spectroscopic measurements during total solar eclipses, temperature can be derived from the forbidden iron lines ratio. We will present our results of temperature variations from the measurements of FeXIV/FeX line ratio during 2006-2010 total solar eclipses. Also a correlation of temperature with sunspot number, radio flux and flare occurrence will be presented.

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