TY - JOUR
T1 - Inviscid linear stability analysis of two vertical columns of different densities in a gravitational acceleration field
AU - Prathama, Aditya Heru
AU - Pantano, Carlos
N1 - Publisher Copyright:
© 2017 Cambridge University Press.
PY - 2017/9/10
Y1 - 2017/9/10
N2 - We study the inviscid linear stability of a vertical interface separating two fluids of different densities and subject to a gravitational acceleration field parallel to the interface. In this arrangement, the two free streams are constantly accelerated, which means that the linear stability analysis is not amenable to Fourier or Laplace solution in time. Instead, we derive the equations analytically by the initial-value problem method and express the solution in terms of the well-known parabolic cylinder function. The results, which can be classified as an accelerating Kelvin-Helmholtz configuration, show that even in the presence of surface tension, the interface is unconditionally unstable at all wavemodes. This is a consequence of the ever increasing momentum of the free streams, as gravity accelerates them indefinitely. The instability can be shown to grow as the exponential of a quadratic function of time.
AB - We study the inviscid linear stability of a vertical interface separating two fluids of different densities and subject to a gravitational acceleration field parallel to the interface. In this arrangement, the two free streams are constantly accelerated, which means that the linear stability analysis is not amenable to Fourier or Laplace solution in time. Instead, we derive the equations analytically by the initial-value problem method and express the solution in terms of the well-known parabolic cylinder function. The results, which can be classified as an accelerating Kelvin-Helmholtz configuration, show that even in the presence of surface tension, the interface is unconditionally unstable at all wavemodes. This is a consequence of the ever increasing momentum of the free streams, as gravity accelerates them indefinitely. The instability can be shown to grow as the exponential of a quadratic function of time.
KW - baroclinic flows
KW - instability
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U2 - 10.1017/jfm.2017.511
DO - 10.1017/jfm.2017.511
M3 - Article
AN - SCOPUS:85029501592
SN - 0022-1120
VL - 826
JO - Journal of Fluid Mechanics
JF - Journal of Fluid Mechanics
M1 - R4
ER -