No CrossRef data available.
Article contents
The Application of Mesoturbulence to Stellar Atmospheres
Published online by Cambridge University Press: 12 April 2016
Abstract
For realistic stellar atmospheres the equations describing mesoturbulent line formation are solved numerically. The general dependence of theoretical line profiles and equivalent widths on the correlation length 1 and the mean square turbulent velocity a is demonstrated. Also empirical relations between the basic parameters of the micro-macroturbulence description (vmic, vmac) and the fundamental mesoturbulence parameters (1,σ) are derived.
- Type
- 3. Conceptualizations of Turbulence
- Information
- Copyright
- Copyright © Springer-Verlag 1980