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,
โฆ LIBER โฆ
The spectrum of the inner corona observed during the total solar eclipse of 30 May 1965
โ Scribed by John T. Jefferies; Frank Q. Orrall; J. B. Zirker
- Publisher
- Springer
- Year
- 1971
- Tongue
- English
- Weight
- 444 KB
- Volume
- 16
- Category
- Article
- ISSN
- 0038-0938
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โฆ Synopsis
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 a function of position angle for the stronger lines and the continuum. In the coronal enhancement or condensation centered at heliocentric position angle 293 ~ absolute intensity is given for 34 forbidden emission lines and the continuum.
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