The two-element interferometer at Hat Creek Observatory was used at 1.3 cm wavelength to study the fine structure of the radio emissive regions on the Sun. Observations of the quiet Sun at 1.3 cm show sudden changes in the fringe amplitude and phase, lasting for typically about 5-8 min. Assuming tha
β¦ LIBER β¦
1.0 arc second structure on the Sun at 3.71 cm wavelength
β Scribed by Robert W. Hobbs; Stuart D. Jordan; William J. Webster; Stephen P. Maran; Howard M. Caulk
- Publisher
- Springer
- Year
- 1974
- Tongue
- English
- Weight
- 78 KB
- Volume
- 36
- Category
- Article
- ISSN
- 0038-0938
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