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A coronal hole observed at 10.7 GHz with a large single dish

✍ Scribed by E. Fürst; W. Hirth


Publisher
Springer
Year
1975
Tongue
English
Weight
214 KB
Volume
42
Category
Article
ISSN
0038-0938

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✦ Synopsis


On July 24, 1973, a coronal hole was observed at 10.69 GHz (2.8 cm) with the Bonn 100-m telescope. The difference of the brightness temperature between outside and inside the hole was about 400 to 500 K. It is shown that this lack of emission can be explained by usually adopted values of the electron density at the bottom of the corona.


📜 SIMILAR VOLUMES


Observation of a coronal hole at 85 GHz
✍ M. R. Kundu; Sou-Yang Liu 📂 Article 📅 1976 🏛 Springer 🌐 English ⚖ 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-