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Magnetic shear. IV - Hale regions 16740, 16815, and 16850Dopplergrams made in C IV 1548 A are studied for evidence of velocity shear near H-alpha dark filaments and for large-scale flow convergent on active regions. The three regions studied support earlier conclusions that shear is a common property of active regions and that active regions may be the foci of converging plasma flow. Flow patterns near filaments show divergence or convergence as well as shear. Also the sense of the shear can be either cyclonic or anticyclonic. No preference is noted for convergence or divergence or for a particular sense of shear, and there appears to be no correlation between the sense of the shear and the sign of the velocity gradient normal to the filament. The close association of H-alpha dark filaments with shear lines leads to the suggestion that the filaments may arise from a cooling instability induced by the Bernoulli effect.
Document ID
19860051049
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Athay, R. G.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Klimchuk, J. A.
(High Altitude Observatory Boulder, CO, United States)
Jones, H. P.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Zirin, H.
(Big Bear Solar Observatory Pasadena, CA, United States)
Date Acquired
August 12, 2013
Publication Date
April 15, 1986
Publication Information
Publication: Astrophysical Journal, Part 1
Volume: 303
ISSN: 0004-637X
Subject Category
Solar Physics
Accession Number
86A35787
Distribution Limits
Public
Copyright
Other

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