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Study of supergranulesResults of a detailed study on supergranule lifetime and velocity fields are presented. The correlation between the observed downdraft velocity and the network magnetic flux elements on the quiet sun is shown. After excluding areas with magnetic flux density 25 G or greater, it is found that the upper limit of the supergranule vertical speed is 0.1 km/s for both downdraft and updraft, and the rms speed is 0.03 km/s. By observing the evolution of individual supergranules, it is found that the average lifetime of supergranules might be 50 hours or greater. Different ways of formation and decay of supergranular cells are described. New cells usually form in an area containing no preexisting supergranule velocity fields. Cells may disappear in two ways: fragmentation and fading away.
Document ID
19890064431
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Wang, Haiman
(California Inst. of Tech. Pasadena, CA, United States)
Zirin, Harold
(Big Bear Solar Observatory Pasadena, CA, United States)
Date Acquired
August 14, 2013
Publication Date
January 1, 1989
Publication Information
Publication: Solar Physics
Volume: 120
Issue: 1 19
ISSN: 0038-0938
Subject Category
Solar Physics
Report/Patent Number
ISSN: 0038-0938
Accession Number
89A51802
Funding Number(s)
CONTRACT_GRANT: NSF ATM-85-13577
CONTRACT_GRANT: NGL-05-002-034
Distribution Limits
Public
Copyright
Other

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