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

Thermal effects on slow viscous flow between rotating eccentric spheres with axial gravitational field

From MaRDI portal
Publication:1064249
Jump to:navigation, search

DOI10.1016/0020-7225(86)90089-3zbMath0575.76105OpenAlexW2002382770MaRDI QIDQ1064249

B. George

Publication date: 1986

Published in: International Journal of Engineering Science (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1016/0020-7225(86)90089-3


zbMATH Keywords

steady flowheat transfer characteristicsviscous stratified fluidexpansion in powers of Reynolds numberflow between two eccentric spheresslow axisymmetric flow


Mathematics Subject Classification ID

Hydrology, hydrography, oceanography (86A05) General theory of rotating fluids (76U05) Reaction effects in flows (76V05)


Related Items (1)

Micropolar fluid flow between two eccentric coaxially rotating spheres




Cites Work

  • Thermal convection in rotating spherical annuli - II. Stratified flows
  • Thermal effects on slow viscous flow between rotating concentric spheres
  • Viscous incompressible flow between eccentric coaxially rotating spheres
  • Axially symmetric motion of a stratified, rotating fluid in a spherical annulus of narrow gap




This page was built for publication: Thermal effects on slow viscous flow between rotating eccentric spheres with axial gravitational field

Retrieved from "https://portal.mardi4nfdi.de/w/index.php?title=Publication:1064249&oldid=13088247"
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 00:10.
Privacy policy
About MaRDI portal
Disclaimers
Imprint
Powered by MediaWiki