Flow-tube dynamics and coronal holes
โ 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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โฆ 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.
๐ SIMILAR VOLUMES
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