Stellar wind models and flow-tube geometry.

Details Stellar wind models and flow-tube geometry. Stellar wind models and flow-tube geometry.

Nov 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983nascp2280..295s&link_type=abstract

NASA Conf. Publ., NASA CP-2280, p. 295 - 297

Physics

Stellar Winds:Hydrodynamics, Stellar Winds:Models

Scientific paper

The author examines the influence of flow-tube geometry on a fluid-dynamic model of a solar wind type flow (i.e. a thermal wind). He finds that as the divergence of the flow-tube increases the expansion speed of the wind increases throughout the flow, over a given parameter range. Further, corresponding to a specified flow-tube geometry the terminal velocity of the wind may be far in excess of the value corresponding to purely spherically symmetric flow.

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