A series of spectrograms of the inner solar corona were obtained at the total solar eclipse of 30 May 1965 using a fast spectrograph with a circular slit that recorded the spectrum from 23000 to 29000 at all position angles around the limb simultaneously. In this paper absolute intensity is given as
โฆ LIBER โฆ
The visible spectrum of the lower corona during the total eclipse of May 30, 1965
โ Scribed by F. Magnant-Crifo
- Publisher
- Springer
- Year
- 1973
- Tongue
- English
- Weight
- 801 KB
- Volume
- 31
- Category
- Article
- ISSN
- 0038-0938
No coin nor oath required. For personal study only.
โฆ Synopsis
Spectra obtained during the May 30, 1965 eclipse by Dunn aboard the NASA aircraft are presented and analyzed. Equivalent widths and absolute intensities are given for 39 coronal lines between 3300 and 8200/~ around the west limb of the Sun at two heights. Details are given on the reduction process, and comparisons are made with other observations from the same eclipse. Some line identifications are discussed.
๐ SIMILAR VOLUMES
The spectrum of the inner corona observe
โ
John T. Jefferies; Frank Q. Orrall; J. B. Zirker
๐
Article
๐
1971
๐
Springer
๐
English
โ 444 KB
Spectropolarimetric analysis of the sola
โ
B. Caccin; G. Moschi; M. Rigutti; R. Falciani
๐
Article
๐
1971
๐
Springer
๐
English
โ 376 KB
Magnetic observation during the total ec
๐
Article
๐
1883
๐
Elsevier Science
๐
English
โ 61 KB