๐”– Bobbio Scriptorium
โœฆ   LIBER   โœฆ

Identification of Solar Coronal Emission Lines

โœ Scribed by COLLINS, P. D. B.; PRYCE, M. H. L.

Book ID
109635000
Publisher
Nature Publishing Group
Year
1964
Tongue
English
Weight
91 KB
Volume
202
Category
Article
ISSN
0028-0836

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๐Ÿ“œ SIMILAR VOLUMES

On the polarization of the solar coronal
On the polarization of the solar coronal emission lines
โœ E. Mogilevsky; B. Ioshpa; V. Obridko ๐Ÿ“‚ Article ๐Ÿ“… 1973 ๐Ÿ› Springer ๐ŸŒ English โš– 694 KB

The results of the spectrophotometrical measurements of the polarization in the coronal lines Fe xIv 5303 fit and Fe x 6374 fit are given. Polarization spectrograms were obtained by two spectrographs (prism and echelle types) during the solar eclipse in Mexico on 7 March, 1970 near the region of the

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๐Ÿ“‚ Article ๐Ÿ“… 1933 ๐Ÿ› Nature Publishing Group ๐ŸŒ English โš– 116 KB
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โœ D. H. Liebenberg; R. J. Bessey; B. Watson ๐Ÿ“‚ Article ๐Ÿ“… 1975 ๐Ÿ› Springer ๐ŸŒ English โš– 834 KB

High resolution spectra of the coronal emission line Fe xIv at 530.3 nm obtained at the 30 May 1965 total solar eclipse are analyzed and interpreted. Deconvolution techniques that preserve the line intensity vs wavelength profile shape are developed to obtain further resolution improvement. The west

The polarization of coronal emission lin
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โœ J. M. Beckers; W. J. Wagner ๐Ÿ“‚ Article ๐Ÿ“… 1971 ๐Ÿ› Springer ๐ŸŒ English โš– 711 KB

By means of a photographic polarimeter, we attempted to measure both the amount and direction of linear polarization of all emission lines between 3400 and 9000 A~ in the inner corona (l.034<<\_r/ro < 1.085). Only the green and red coronal lines have been analyzed in detail. Neither of these lines s