Temperature structure from Ca II H wing inversions

Details Temperature structure from Ca II H wing inversions Temperature structure from Ca II H wing inversions

Sep 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008espm...12.2.76h&link_type=abstract

"12th European Solar Physics Meeting, Freiburg, Germany, held September, 8-12, 2008. Online at http://espm.kis.uni-freiburg.de/,

Physics

Scientific paper

A method in development to extract temperature at different depths from the Ca II H&K lines using filtergrams is presented along with preliminary inversion results. The inversions give information up to a height of 200-300 km.
We make use of the Swedish 1-m Solar Telescope (SST) blue filter setup which allows for simultaneous observations in four filter positions including a 1-Å tunable filter that scans through the Ca H blue wing.

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