In order to obtain a better agreement between observed and computed values of the solar intensity, an improved temperature distribution is deduced for the range 0.02 < 30 < 10. The intensity observations here considered refer to the wavelength region between ). 1980 and ,I. 129500, and the center-li
The UV continuum 1450–2100 Å and the problem of the solar temperature minimum
✍ Scribed by K. G. Widing; J. D. Purcell; G. D. Sandlin
- Book ID
- 105522611
- Publisher
- Springer
- Year
- 1970
- Tongue
- English
- Weight
- 747 KB
- Volume
- 12
- Category
- Article
- ISSN
- 0038-0938
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