Differential rotation of coronal holes

descriptionPublicationkeyboard_double_arrow_right Article 01 Jan 1985 English Publisher:Springer Science and Business Media LLCJournal:Solar Physics, volume 95, pages 193-197 (issn: 0038-0938, eissn: 1573-093X,

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Authors: Rajendra N. Shelke; M. C. Pande;

doi: 10.1007/bf00162647

Differential rotation of coronal holes

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Abstract

Using KPNO helium 10830 A synoptic charts of Carrington rotations 1716 through 1739, and by assembling a time sequence representing single latitude zone, rotational properties of coronal holes for five zones of latitudes (±10°, ±20° – ±40°, and ±40° – ±60°) have been examined. It seems that the rotation period of coronal holes is a function of latitude, thus reflecting differential rotation of coronal holes.

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