Active regions that are sources of microwave solar emission should appear displaced in latitude relative to the associated optical feature and from this displacement it should be possible to deduce the height. Although the displacement is only about one-third of a rain of' arc at the most, it was fo
The height of the 9 cm solar emission
โ Scribed by M. Waldmeier
- Publisher
- Springer
- Year
- 1978
- Tongue
- English
- Weight
- 126 KB
- Volume
- 57
- Category
- Article
- ISSN
- 0038-0938
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