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The solar continuum from 900 to 130 000 Å and the photospheric temperature model

✍ Scribed by A. Sauval

Book ID
104645649
Publisher
Springer
Year
1968
Tongue
English
Weight
716 KB
Volume
3
Category
Article
ISSN
0038-0938

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✦ Synopsis

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-limb variations generally go down to cos 0-0.1. The improved model, given in Figure 4 and

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Interpretation of the solar continuum from 1680 to 600 Å. Model of the transition region photosphere-chromosphere and of the chromosphere
✍ Yvette Cuny 📂 Article 📅 1971 🏛 Springer 🌐 English ⚖ 867 KB

An interpretation is given of the observations of the continuous solar radiation in the spectral range 600-1700 A. The model allows for deviations from LTE of H, C, Si and S, and is in hydrostatic equilibrium. The predicted intensity from 1680 to 1520/~ has virtually no dependence on the electron te