Mathematical Research Data Initiative
Main page
Recent changes
Random page
Help about MediaWiki
Create a new Item
Create a new Property
Create a new EntitySchema
Merge two items
In other projects
Discussion
View source
View history
Purge
English
Log in

The nature of one mechanism of solar differential rotation

From MaRDI portal
Publication:1249878
Jump to:navigation, search

DOI10.1007/BF00651051zbMath0386.76089MaRDI QIDQ1249878

S. I. Vainshtein, Alexander Ruzmaikin

Publication date: 1978

Published in: Astrophysics and Space Science (Search for Journal in Brave)



Mathematics Subject Classification ID

Anisotropy in solid mechanics (74E10) General theory of rotating fluids (76U05) Magnetohydrodynamics and electrohydrodynamics (76W05) Reaction effects in flows (76V05) Diffusion and convection (76R99) Geophysical solid mechanics (74L05)


Related Items (3)

Turbulent transport of angular momentum and differential rotation ⋮ On the nature of the core-envelope boundary layer in a slowly rotating star ⋮ Reynolds stresses and differential rotation. I. On recent calculations of zonal fluxes in slowly rotating stars



Cites Work

  • Unnamed Item
  • On the R<scp>EYNOLDS</scp> stresses in mean‐field hydrodynamics III. Two‐dimensional turbulence and the problem of differential rotation
  • Differential Rotation in Stars with Convective Envelopes.
  • Zur Dynamotheorie stellarer und planetarer Magnetfelder I. Berechnung sonnenähnlicher Wechselfeldgeneratoren


This page was built for publication: The nature of one mechanism of solar differential rotation

Retrieved from "https://portal.mardi4nfdi.de/w/index.php?title=Publication:1249878&oldid=13339123"
Tools
What links here
Related changes
Special pages
Printable version
Permanent link
Page information
MaRDI portal item
This page was last edited on 31 January 2024, at 08:48.
Privacy policy
About MaRDI portal
Disclaimers
Imprint
Powered by MediaWiki