The model is that of . This model is in MHSE and includes tension forces. Results are presented in the form of contour maps, cross-sections of the contrast on axis, and integrated contrast as a function of viewing angle. Results are generally consistent with those of , but not with observations of .
The contrast of faculae near the solar limb
โ Scribed by H. Wang; H. Zirin
- Publisher
- Springer
- Year
- 1987
- Tongue
- English
- Weight
- 654 KB
- Volume
- 110
- Category
- Article
- ISSN
- 0038-0938
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