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The horizontal variation of temperature in the low solar photosphere

✍ Scribed by Richard C. Altrock

Publisher
Springer
Year
1976
Tongue
English
Weight
384 KB
Volume
47
Category
Article
ISSN
0038-0938

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✦ Synopsis

Observations of the rms intensity fluctuations in the continuum obtained by Pravdjuk et al. (Solnechnye Dannye, No. 2, p. 70, 1974) from white-light photographs made with the Soviet Stratospheric Solar Observatory are analyzed to obtain a horizontal temperature-fluctuation amplitude as a function of depth. The results indicate that temperature fluctuations increase with depth monotonically from a small value at ~'sooo~0.5 (cf. Figure 2). The initial rise of AT appears quite steep, having a slope of approximately 20 K km -~. The model of Wilson (Solar Phys. 9, 303, 1969) is incompatible with the data. Convective flux in the present model is approximately 6% of the total flux at Zsooo = 1.

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