Existing models of the solar atmosphere predict a limb brightening in the far infrared wavelengths. At shorter wavelengths this effect is confined to the extreme limb but at 25 a it extends inward from the limb to cos 0 = 0.3. Observations of I(a)/I(1.0) were made with the McMath Solar Telescope thr
On the center-to-limb variation of sunspot brightness
β Scribed by W. Mattig
- Publisher
- Springer
- Year
- 1969
- Tongue
- English
- Weight
- 232 KB
- Volume
- 6
- Category
- Article
- ISSN
- 0038-0938
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β¦ Synopsis
A preliminary analysis of recent measurements of the brightness ratio spot-photosphere of various authors leads to the result, that the limb-darkening of the umbra is considerably less than that of the photosphere. The small value of the center-to-limb variation implies a very small temperature gradient, which is, for optical depths r~.0.2, about one order of magnitude smaller than previously thought (Figure 3). This result would seem to rule out radiative equilibrium in the deeper layers (rT~. 0.2) of sunspot umbrae.
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