Radiospectroheliograms obtained at millimeter wavelengths were used to determine the rotation of the solar atmosphere. Regions observed in both emission as well as absorption (associated with Ha dark filaments) were followed across the disk. The average sidereal rotation rate deduced from emissive r
β¦ LIBER β¦
On the differential rotation with height in the solar atmosphere
β Scribed by W. C. Livingston
- Publisher
- Springer
- Year
- 1969
- Tongue
- English
- Weight
- 230 KB
- Volume
- 9
- Category
- Article
- ISSN
- 0038-0938
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