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  • 2005-2009  (49)
  • 1970-1974  (6)
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Year
  • 1
    In: Journal of fluid mechanics, Cambridge [u.a.] : Cambridge Univ. Press, 1956, 632(2009), Seite 457-474, 1469-7645
    In: volume:632
    In: year:2009
    In: pages:457-474
    Description / Table of Contents: The generalized temporal residual mean (TRM-G) framework is reviewed and illustrated using a numerical simulation of vertical shear instability. It is shown how TRM-G reveals the physically relevant amount of diapycnal eddy fluxes and implied diapycnal mixing, and how TRM-G relates to the OsbornCox relation, which is often used to obtain observational estimates of the diapycnal diffusivity. An exact expression for the diapycnal diffusivity in the TRM-G is given in the presence of molecular diffusion, based on acknowledging and summing up an entire hierarchy of eddy buoyancy moments. In this revised form of the OsbornCox relation, diapycnal diffusivity is related only to irreversible mixing of buoyancy, since all advective and molecular flux terms are converted to dissipation of variance and higher order moments. An approximate but closed analytical expression can be given for the revised OsbornCox relation with the caveat that this closed expression implies unphysical cross-boundary rotational fluxes. It is demonstrated that the original OsbornCox relation, in which advective and molecular flux terms are simply neglected, is an approximation to the full form valid to first order. In the numerical simulation the original OsbornCox relation holds to a surprisingly good approximation despite large advective fluxes of variance and large lateral inhomogeneity in the turbulent mixing.
    Type of Medium: Online Resource
    Pages: graph. Darst
    ISSN: 1469-7645
    Language: English
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  • 2
    Electronic Resource
    Electronic Resource
    Springer
    Astrophysics and space science 26 (1974), S. 95-105 
    ISSN: 1572-946X
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract The equations of motion of all relevant parameters of Alfvén waves propagating from the sun outwardly into the expanding interplanetary medium are discussed for the case of a quiet, ideal, isotropic, one-fluid solar wind plasma. It is found that the frequency of the wave reamains constant, while the wave vector and the amplitudes depend, in general, on the evolution of the background medium and on the angle between the wave vector and the interplanetary magnetic field. This latter dependence cancels approximately for the evolution of the amplitudes in the case of a pure, overall spiral magnetic field. It is shown that in this case the results of earlier discussions can be derived by less decisive restrictions.
    Type of Medium: Electronic Resource
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  • 3
    Electronic Resource
    Electronic Resource
    Springer
    Astrophysics and space science 20 (1973), S. 373-389 
    ISSN: 1572-946X
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract The main results of Whitham's averaged Lagrangian method for the treatment of linear wave-trains in a weakly inhomogeneous, moving medium are presented briefly. This method is then applied to an ideal, isotropic, one-fluid plasma which can be taken for the lowest order approximation for the interplanetary solar wind expansion.
    Type of Medium: Electronic Resource
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  • 4
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    Cambridge Univ. Pr.
    In:  Journal of Fluid Mechanics, 632 . pp. 457-474.
    Publication Date: 2019-09-23
    Description: The generalized temporal residual mean (TRM-G) framework is reviewed and Illustrated using a numerical Simulation of vertical shear instability. It is shown how TRM-G reveals the physically relevant amount of diapycnal eddy fluxes and implied diapycnal mixing, and how TRM-G relates to the Osborn-Cox relation, which is often used to obtain observational estimates of the diapycnal diffusivity. An exact expression for the diapycnal diffusivity in the TRM-G is given in the presence of molecular diffusion, based on acknowledging and summing Lip an entire hierarchy of eddy buoyancy moments. In this revised form of the Osborn-Cox relation, diapycnal diffusivity is related only to irreversible mixing of buoyancy, since all advective and molecular flux terms are converted to dissipation of variance and higher order moments. An approximate but closed analytical expression can be given for the revised Osborn-Cox relation with the caveat that this closed expression implies unphysical cross-boundary rotational fluxes.It is demonstrated that the original Osborn-Cox relation, in which advective and molecular flux terms are simply neglected, is an approximation to the full form valid to first order. In the numerical simulation the original Osborn-Cox relation holds to a surprisingly good approximation despite large advective fluxes of variance and large lateral inhomogeneity in the turbulent mixing.
    Type: Article , PeerReviewed
    Format: text
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  • 5
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    In:  EPIC3in: Marine Turbulence: Theories, Observations and Models, Ed. H. Baumert, J. Simpson, J. Sündermann, Springer Verlag, Berlin, pp, pp. 511 - 529
    Publication Date: 2019-07-16
    Repository Name: EPIC Alfred Wegener Institut
    Type: Inbook , peerRev
    Format: application/pdf
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  • 6
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    In:  EPIC3Guest colloquium at NIOZ, NLOctober 2007., 4
    Publication Date: 2019-07-16
    Repository Name: EPIC Alfred Wegener Institut
    Type: Conference , notRev
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  • 7
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    In:  EPIC3Physics colloquium, NIOZ, NL, Oct 17.
    Publication Date: 2019-07-16
    Repository Name: EPIC Alfred Wegener Institut
    Type: Conference , notRev
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  • 8
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    In:  EPIC3Journal of Fluid Mechanics, 632, pp. 457-474
    Publication Date: 2019-07-16
    Repository Name: EPIC Alfred Wegener Institut
    Type: Article , isiRev
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  • 9
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    In:  EPIC3Ocean Dynamics, 57, pp. 559-578, ISBN: 1616-7341 (Print) 16
    Publication Date: 2019-07-16
    Repository Name: EPIC Alfred Wegener Institut
    Type: Article , isiRev
    Format: application/pdf
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  • 10
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    In:  EPIC3FRISP/WAIS workshop , Losehill Hall, Derbyshire, Englandth-20th Sept. 2008., 18
    Publication Date: 2019-07-16
    Repository Name: EPIC Alfred Wegener Institut
    Type: Conference , notRev
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