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
β¦ LIBER β¦
Mauna loa coronagraph observations around the 7 March 1970 eclipse
β Scribed by Richard T. Hansen; Shirley F. Hansen; Charles J. Garcia
- Book ID
- 104644183
- Publisher
- Springer
- Year
- 1970
- Tongue
- English
- Weight
- 801 KB
- Volume
- 15
- Category
- Article
- ISSN
- 0038-0938
No coin nor oath required. For personal study only.
β¦ Synopsis
The locations of seven principal coronal features observed in projection at the 7 March 1970 eclipse are established from synoptic coronagraphic measurements.
π SIMILAR VOLUMES
Observations of coronal polarization at
β
J. DΓΌrst
π
Article
π
1976
π
Springer
π
English
β 346 KB
Observations of Ionospheric Electron Con
β
ALMEIDA, O. G.; DA ROSA, A. V.
π
Article
π
1970
π
Nature Publishing Group
π
English
β 186 KB
VLF Radio Signals observed in Newfoundla
β
RYCROFT, M. J.; REEVE, C. D.
π
Article
π
1970
π
Nature Publishing Group
π
English
β 302 KB
The chromosphere in continuum emission o
β
Mitsugu Makita
π
Article
π
1972
π
Springer
π
English
β 710 KB
Prediction and Observation of the Corona
β
WALDMEIER, M.
π
Article
π
1970
π
Nature Publishing Group
π
English
β 273 KB
Observations of the 7 March, 1970 total
β
John P. Hagen; Paul N. Swanson; Robert W. Haas; Fred L. Wefer; Raymond W. Vogt
π
Article
π
1971
π
Springer
π
English
β 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