𝔖 Bobbio Scriptorium
✦   LIBER   ✦

Spectrophotometry of the corona and a quiescent prominence based on observations of the total solar eclipse of 7 March, 1970 in Mexico

✍ Scribed by G. M. Nikolsky; R. A. Gulyaev; K. I. Nikolskaya


Publisher
Springer
Year
1971
Tongue
English
Weight
998 KB
Volume
21
Category
Article
ISSN
0038-0938

No coin nor oath required. For personal study only.


πŸ“œ SIMILAR VOLUMES


Observations of the 7 March, 1970 total
✍ John P. Hagen; Paul N. Swanson; Robert W. Haas; Fred L. Wefer; Raymond W. Vogt πŸ“‚ Article πŸ“… 1971 πŸ› Springer 🌐 English βš– 992 KB

The 7 March, 1970 total solar eclipse was observed at wavelengths of 3.2 and 8.3 mm; the object being to use the knife edge of the Moon as it passed across the Sun to improve angular resolution on the Sun. This in turn would provide a radial brightness distribution of the Sun with an angular resolut

The physical conditions in inner corona
✍ E. A. Gurtovenko; K. V. Alikayeva πŸ“‚ Article πŸ“… 1971 πŸ› Springer 🌐 English βš– 442 KB

The spectrum of the solar corona obtained during the eclipse of 7 March, 1970 has been studied. From the analysis of the line halfwidths it is concluded that the emission of coronal lines of various groups arises in different volumes of the corona. The lines 15303 and 14231 are analyzed in detail an

The radial brightness distribution of th
✍ Paul N. Swanson; John P. Hagen πŸ“‚ Article πŸ“… 1975 πŸ› Springer 🌐 English βš– 222 KB

The radial brightness distribution of the Sun at 3.2 mm is recalculated for the 7 March, 1970 total solar eclipse by an improved method. The results from the first contact of the 30 June, 1973 total eclipse are also analyzed. Limb brightening is apparent for the 1970 eclipse when all four contacts a