On the solar oblateness: The combined ef
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B. R. Durney; N. E. Werner
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Article
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1971
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Springer
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English
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With the help of a model atmosphere of the Sun we evaluate the pole-equator difference in flux (as measured by Dicke and Goldenberg) assuming the following type of pole-equator temperature difference (A T = Te --T~) : (a) A T ~ 2 K for r > r0 (r0 ~ 0.05); (b) A T ~ 10 K for r < r 0. The small ATat