Temperature stratification in sunspots

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Solar Temperature, Sunspots, Astronomical Models, Infrared Spectra, Temperature Gradients, Umbras

Scientific paper

Various mechanisms to explain the lower temperature of sunspots in relation to their surroundings are considered. The investigation of the physical characteristics of sunspots is significant for other aspects of solar research, as in the determination of the frequency of easily ionized elements (e.g., Li, Be, B, and Cs). The recent development of methods that permit the measurement of individual linear profiles in the umbra of the sunspots is examined, along with the falsification of spectra through stray light interference from the surroundings. The use of an additional absorber effective at lower temperatures of the umbra is discussed.

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