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Brightness distribution at the base of a coronal hole

✍ Scribed by R. B. Teplitskaya; O. A. Ozhogina; I. P. Turova


Book ID
111437044
Publisher
Springer
Year
2006
Tongue
English
Weight
553 KB
Volume
32
Category
Article
ISSN
1063-7737

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πŸ“œ SIMILAR VOLUMES


Observation of a coronal hole at 85 GHz
✍ M. R. Kundu; Sou-Yang Liu πŸ“‚ Article πŸ“… 1976 πŸ› Springer 🌐 English βš– 253 KB

A coronal hole was observed at 85 GHz(3.5 mm-h) on November 24, 1970, when a spectacular coronal hole was observed in soft X-rays by AS&E. The miUimeter counterpart of the hole is much weaker and less widespread than in X-rays. The brightness temperature inside the hole was in most places about 100-