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.


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    Titel :

    Using LASCO-C1 spectroscopy for coronal diagnostics


    Beteiligte:
    Mierla, M. (Autor:in) / Schwenn, R. (Autor:in) / Teriaca, L. (Autor:in) / Stenborg, G. (Autor:in) / Podlipnik, B. (Autor:in)

    Erschienen in:

    Advances in Space Research ; 35 , 12 ; 2199-2203


    Erscheinungsdatum :

    2005-04-11


    Format / Umfang :

    5 pages




    Medientyp :

    Aufsatz (Zeitschrift)


    Format :

    Elektronische Ressource


    Sprache :

    Englisch




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