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木星上的开尔文-亥姆霍兹不稳定性,發生在行星大氣中兩個層的介面

流體動力學中,流体动力稳定性是一個研究流體流動的穩定性及不穩定性的領域,流體的不穩定進一步可能會產生紊流[2]。流体动力稳定性在理論及實驗上的基礎,主要是由十九世紀的亥姆霍茲开尔文瑞利雷諾等科學家所奠定[2]

目录

相關條目编辑

腳註编辑

  1. ^ Li, Shengtai and Hui Li. Parallel AMR Code for Compressible MHD or HD Equations. Los Alamos National Laboratory. [2006-09-05]. (原始内容存档于2016-03-03). 
  2. ^ 2.0 2.1 See Drazin (2002), Introduction to hydrodynamic stability, p. 1.

參考資料编辑

  • Chandrasekhar, S., Hydrodynamic and hydromagnetic stability, Dover, 1981, ISBN 0-486-64071-X 
  • Charru, F., Hydrodynamic instabilities, Cambridge University Press, 2011, ISBN 1139500546 
  • Drazin, P. G., Introduction to hydrodynamic stability, Cambridge University Press, 2002, ISBN 0-521-00965-0 
  • Drazin, P.G.; Reid, W.H., Hydrodynamic stability, Cambridge University Press, 1981, ISBN 0-521-28980-7 
  • Godreche, C.; Manneville, P. (编), Hydrodynamics and nonlinear instabilities, Cambridge University Press, 1998, ISBN 0521455030 
  • Lin, C.C., The theory of hydrodynamic stability corrected, Cambridge University Press, 1966, OCLC 952854 
  • Joseph, D.D., Stability of fluid motions I, Tracts in Natural Philosophy 27, Springer-Verlag, 1976, ISBN 3-540-07514-3 
    Joseph, D.D., Stability of fluid motions II, Tracts in Natural Philosophy 28, Springer-Verlag, 1976, ISBN 3-540-07516-X 
  • Sritharan, S.S., Invariant manifold theory for hydrodynamic transition, Pitman research notes in mathematics series 241, Wiley, 1990, ISBN 0-582-06781-2 [1]
  • Swinney, H.L.; Gollub, J.P. (编), Hydrodynamic instabilities and the transition to turbulence 2d, Springer, 1985, ISBN 978-3-540-13319-3 

外部連結编辑