
On Rossby waves in spiral galaxies
Abstract
Galactostrophic eddy velocities are used to eliminate the dependence of the potential vorticity equation on the velocities. The resultant time dependent equation involves the mass densities alone.
DOI: https://doi.org/10.3402/tellusa.v16i3.8975 | Journal eISSN: 3035-9554
Language: English
Page range: 359 - 362
Submitted on: Apr 21, 1964
Published on: Jan 1, 1964
Published by: Stockholm University Press
In partnership with: Paradigm Publishing Services
© 1964 Robert E. Dickinson, published by Stockholm University Press
This work is licensed under the Creative Commons Attribution 4.0 License.