Ekman pumping in astrophysical bodies

Apr, 1995
23 pages
Published in:
  • J.Fluid Mech. 312 (1996) 327-340
e-Print:
Report number:
  • FERMILAB-PUB-95-074-A

Citations per year

1996200320102017202401234
Abstract: (arXiv)
We examine the dynamics of a rotating viscous fluid following an abrupt change in the angular velocity of the solid bounding surface. We include the effects of a density stratification and compressibility which are important in astrophysical objects such as neutron stars. We confirm and extend the conclusions of previous studies that stratification restricts the Ekman pumping process to a relatively thin layer near the boundary, leaving much of the interior fluid unaffected. We find that finite compressibility further inhibits Ekman pumping by decreasing the extent of the pumped layer and by increasing the time for spin-up. The results of this paper are important for interpreting the spin period discontinuities (``glitches'') observed in rotating neutron stars.
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