We describe a new model of the chromosphere based on Lyman-continuum observations by Harvard spectrometers aboard the satellites OSO 4 and OSO 6. The model assumes (a) that a random distribution of optically thick inhomogeneities overlies a plane-parallel homogeneous atmosphere, and (b) that the Lym
โฆ LIBER โฆ
The Derivation of a Model Solar Chromosphere from Radio Data
โ Scribed by Piddington, J. H.
- Book ID
- 120146810
- Publisher
- The Royal Society
- Year
- 1950
- Tongue
- English
- Weight
- 750 KB
- Volume
- 203
- Category
- Article
- ISSN
- 0962-8444
No coin nor oath required. For personal study only.
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