Abstract
The angular velocity of solar rotation tracers, has been observed to decrease systematically with their age (Godoli et al., 1978); such a decrease is different at different latitudes and results therefore in variations of both faculae (Belvedere et al., 1977) and sunspots (Ternullo et al., 1981) velocity profiles.
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References
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© 1982 D. Reidel Publishing Company
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Ternullo, M. (1982). Subphotospheric Velocity Fields Inferred by Sunspots Motions. In: Fricke, W., Teleki, G. (eds) Sun and Planetary System. Astrophysics and Space Science Library, vol 96. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-7846-1_17
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DOI: https://doi.org/10.1007/978-94-009-7846-1_17
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