z-logo
open-access-imgOpen Access
Convective Models of Jupiter’s Zonal Jets with Realistic and Hyper-Energetic Excitation Source
Author(s) -
H. G. Mayr,
K. L. Chan
Publication year - 2019
Publication title -
international journal of astronomy and astrophysics
Language(s) - English
Resource type - Journals
eISSN - 2161-4725
pISSN - 2161-4717
DOI - 10.4236/ijaa.2019.93021
Subject(s) - physics , zonal and meridional , zonal flow (plasma) , geostrophic wind , jupiter (rocket family) , rossby number , meridional flow , convection , jet (fluid) , atmospheric sciences , latitude , geophysics , astrophysics , mechanics , plasma , astronomy , space shuttle , quantum mechanics , turbulence , tokamak

The content you want is available to Zendy users.

Already have an account? Click here to sign in.
Having issues? You can contact us here
Accelerating Research

Address

John Eccles House
Robert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom