Format:
162 S. = 1810 KB, text, images
Edition:
Electronic edition
Content:
With both German Solar Telescopes in Tenerife polar faculae were observed in the FeI Lines of 630,15 and 630,25 nm. Out of the GCTs data an analytical model of the dependence of the parameters with diameter was derived. Images of the VTT were image-reconstructed and an inversion using the SIR-Code was performed. Models of faculae were derived, discussed and compared to plages.
Note:
Göttingen, Univ., Diss., 2001
Language:
German
Keywords:
Sonnenaktivität
;
Polarimetrie
;
Inversionsalgorithmus
;
Hochschulschrift
URN:
urn:nbn:de:gbv:7-webdoc-1065-0
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