No CrossRef data available.
Article contents
Plasma Flow and Solar Wind Acceleration in Non-Radial Coronal Magnetic Fields
Published online by Cambridge University Press: 04 August 2017
Extract
In the vicinity of the Sun — especially above coronal holes — the magnetic field lines show strong non-radial divergence and considerable curvature (see e.g. Kopp and Holzer, 1976; Munro and Jackson, 1977; Ripken, 1977). In the following we study the influence of these characteristics on the expansion velocity of the solar wind.
- Type
- V. Stellar Winds and Spindown in Late — Type Stars
- Information
- Copyright
- Copyright © Reidel 1983