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- W85933085 abstract "Motions of slowly evolving sunspots and the rotation velocity of the plasma around them were determined within periods of one to three weeks each year from 1990 until 1992. The sunspots were divided into two classes depending on the size and number of proceeding and/or following umbrae. Most of the sunspots were of Zurich type H, too large and complex sunspots were rejected. The main aim was a determination of plasma and sunspot velocities within larger fields of activity and a search for special patterns of plasma flows, which may be caused by interaction of the magnetized and unmagnetized plasmas. Around a total of 34 sunspots about 130 plasma velocity fields with sizes of about 120 by 70 arcseconds could be scanned" @default.
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- W85933085 date "1993-11-01" @default.
- W85933085 modified "2023-09-23" @default.
- W85933085 title "Large-scale solar plasma rotation around stable sunspots" @default.
- W85933085 hasPublicationYear "1993" @default.
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