Abstract
NUMEROUS attempts have been made to find the physical mechanism responsible for the sunspot cycle. Present theoretical discussions of the basic mechanism of solar activity are usually based on a dynamo theory with a reversing magnetic field1, but objections and alternative interpretations1,2 have recently been advanced. Our understanding of the sunspot cycle seems to be in a stage where new observational insight may be valuable. We report here a variation in the infrared umbra intensity of large sunspots with the phase in the solar cycle.
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References
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ALBREGTSEN, F., MALTBY, P. New light on sunspot darkness and the solar cycle. Nature 274, 41–42 (1978). https://doi.org/10.1038/274041a0
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DOI: https://doi.org/10.1038/274041a0
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