Physics
Scientific paper
May 1986
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986soph..105..197t&link_type=abstract
Solar Physics (ISSN 0038-0938), vol. 105, May 1986, p. 197-204.
Physics
13
Calcium, Faculae, Solar Rotation, Chromosphere, Solar Cycles
Scientific paper
Ca II spectroheliograms obtained at Catania Observatory for the 1967-1970 period are examined, and the latitudinal differential rotation profile of chromospheric plages in the first four days of lifetime was found to be steeper than the average profile determined from the whole solar cycle. The rigidity of rotation is shown to increase with the object's age, with plages lying around the Equator and in the strips of latitude between 15 and 25 deg slowing down, while the ones lying poleward more than + or - 30 deg accelerate. A correspondence between the locations of both speeding-up plages with westward streams, and slowing down plages with eastward streams, is noted. The results are consistent with the existence of deep layers affected by a differential rotation latitudinal profile which is steeper than that of surface layers and which tends to flatten during the decay phase of the solar activity cycle.
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