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Flow-tube dynamics and coronal holes

โœ Scribed by D. Summers


Book ID
104642231
Publisher
Springer
Year
1983
Tongue
English
Weight
195 KB
Volume
85
Category
Article
ISSN
0038-0938

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โœฆ Synopsis


We reexamine the well-known polytropic flow-tube model of the expanding solar corona, and find that as the divergence of the flow tube increases the expansion speed increases throughout the flow, over a stated parameter range. Corresponding to a specified flow-tube geometry the terminal speed of the fluid may be far in excess of the value corresponding to purely spherically symmetric flow. The implications of the results for the modelling of high-speed streams emanating from coronal holes are discussed.


๐Ÿ“œ SIMILAR VOLUMES


Dynamics of coronal hole regions
โœ Roger A. Kopp; Thomas E. Holzer ๐Ÿ“‚ Article ๐Ÿ“… 1976 ๐Ÿ› Springer ๐ŸŒ English โš– 745 KB
Thermally conductive flows in coronal ho
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Polytropic solar wind flows in flow tubes whose cross-sectional area increases faster with radius than for a radial expansion have been studied by Kopp and Holzer (1976). Their use of a faster-than-radial expansion proved promising in analytically associating the high-speed streams observed near i A

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โœ Herbert Kalisch; Wolfram Neutsch; Horst Fichtner; S. Ranga Sreenivasan; Maurice ๐Ÿ“‚ Article ๐Ÿ“… 2003 ๐Ÿ› Springer Netherlands ๐ŸŒ English โš– 487 KB
Coronal Holes and Icosahedral Symmetry
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