𝔖 Bobbio Scriptorium
✦   LIBER   ✦

Micrometeorological observations of a soil surface during the partial phases of the total solar eclipse of March 7, 1970

✍ Scribed by S. I. Outcalt; D. D. Meisel


Publisher
Springer
Year
1970
Tongue
English
Weight
414 KB
Volume
18
Category
Article
ISSN
1434-4483

No coin nor oath required. For personal study only.


πŸ“œ SIMILAR VOLUMES


Observations of coronal polarization at
✍ J. DΓΌrst πŸ“‚ Article πŸ“… 1976 πŸ› Springer 🌐 English βš– 346 KB

Polarigraphic observations of the 7 March, 1970 eclipse were made at Miahuatlfin (Mexico) with a camera of 120 cm focal length. A polarizing filter in front of the objective could be adjusted at 8 different positions, 22.5 ~ apart. Reduction of eight photographs of the white light corona yields pola

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 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

Some newly discovered coronal emission l
✍ Kenneth H. Olsen; Charles R. Anderson; John N. Stewart πŸ“‚ Article πŸ“… 1971 πŸ› Springer 🌐 English βš– 780 KB

A survey of the infrared coronal spectrum between 1 /~ and 3 ~ was made from a high altitude aircraft during the 7 March, 1970, solar eclipse. The observations were made with a Fourier transform spectrometer and were confined to the outer chromosphere and inner corona. In addition to well known chro

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