AbstractThe LASCO-C1 telescope was designed to perform spectral analysis of coronal structures by means of a tunable Fabry–Pérot interferometer acquiring images at different wavelengths. Results from spectral scans of the Fe xiv 5303Å green coronal emission line are presented. Physical quantities like the ion temperature (line widths), and the flow velocity along the line of sight (Doppler shifts) are obtained over the entire corona.
Using LASCO-C1 spectroscopy for coronal diagnostics
Advances in Space Research ; 35 , 12 ; 2199-2203
2005-04-11
5 pages
Aufsatz (Zeitschrift)
Elektronische Ressource
Englisch
Using LASCO-C1 spectroscopy for coronal diagnostics
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