Comparison of the 530.3 NM coronal brightness estimates of the Wendelstein solar observatory and of the 530.3 NM coronal measurements of Alma-Ata, Kislovodsk, Lomnicky Stit, Norikura, with the Wendelstein 530.3 nm-coronal photometer

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Luminous Intensity, Solar Corona, Solar Instruments, Electrophotometers, Stellar Spectrophotometry

Scientific paper

A first comparison is made of Wendelstein visual coronal estimates with measurements from other coronal stations. The Wendelstein measurements were at 530.3 nm intensities at the standard height of 60 arcsec above the solar limb. The correlation coefficient between the estimates and the photoelectric measurement is 0.83, distinctly better than those between photoelectric measurements and spectrographic observations at other stations. Comparisons are made among coronal intensities from other stations and the Wendelstein data.

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Comparison of the 530.3 NM coronal brightness estimates of the Wendelstein solar observatory and of the 530.3 NM coronal measurements of Alma-Ata, Kislovodsk, Lomnicky Stit, Norikura, with the Wendelstein 530.3 nm-coronal photometer does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

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