Differential rotation of coronal holes

Details Differential rotation of coronal holes Differential rotation of coronal holes

Jan 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985soph...95..193s&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 95, Jan. 1985, p. 193-197.

Physics

22

Coronal Holes, Rotating Environments, Solar Activity, Latitude, Northern Hemisphere, Southern Hemisphere, Time Response

Scientific paper

Using KPNO helium synoptic charts of Carrington rotations 1716 through 1739, and by assembling a time sequence representing a single latitude zone, the rotational properties of coronal holes for five latitude zones (+ or - 10 deg, + or - 20 deg minus + or - 40 deg, and + or - 40 deg minus + or - 60 deg) have been examined. It is shown that the rotation period of coronal holes is a function of latitude, thus reflecting differential rotation of coronal holes.

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