scholarly journals THE BUOYANT TWO-DIMENSIONAL LAMINAR VERTICAL JET

1970 ◽  
Vol 23 (3) ◽  
pp. 413-430 ◽  
Author(s):  
S. B. SAVAGE ◽  
G. K. C. CHAN
Keyword(s):  
1967 ◽  
Vol 29 (2) ◽  
pp. 305-315 ◽  
Author(s):  
R. S. Brand ◽  
F. J. Lahey

The boundary-layer equations for the steady laminar flow of a vertical jet, including a buoyancy term caused by temperature differences, are solved by similarity methods. Two-dimensional and axisymmetric jets are treated. Exact solutions in closed form are found for certain values of the Prandtl number, and the velocity and temperature distribution for other Prandtl numbers are found by numerical integration.


1985 ◽  
Vol 8 (4) ◽  
pp. 449-468
Author(s):  
Graham Wilks ◽  
Roland Hunt ◽  
David Riley
Keyword(s):  

2012 ◽  
Vol 2012 ◽  
pp. 1-14 ◽  
Author(s):  
Marco Rosales-Vera ◽  
Yarko Niño ◽  
Alvaro Valencia

The problem of a hydromagnetic hot two-dimensional laminar jet issuing vertically into an otherwise quiescent fluid of a lower temperature is studied. We propose solutions to the boundary layer equations using the classical Fourier series. The method is essentiall to transform the boundary layer equations to a coupled set of nonlinear first-order ordinary differential equations through the Fourier series. The accuracy of the results has been tested by the comparison of the velocity distributions obtained by the Fourier series with those calculated by finite difference method. The results show that the present method, based on the Fourier series, is an efficient method, suitable to solve boundary layer equations applied to plane jet flows with high accuracy.


1985 ◽  
Vol 8 (4) ◽  
pp. 449-468 ◽  
Author(s):  
Graham Wilks ◽  
Roland Hunt ◽  
David S. Riley
Keyword(s):  

2011 ◽  
Vol 685 ◽  
pp. 191-201 ◽  
Author(s):  
Julien Candelier ◽  
Stéphane Le Dizès ◽  
Christophe Millet

AbstractThe effect of an inclination angle of the shear with respect to the stratification on the linear properties of the shear instability is examined in the work. For this purpose, we consider a two-dimensional plane Bickley jet of width $L$ and maximum velocity ${U}_{0} $ in a stably stratified fluid of constant Brunt–Väisälä frequency $N$ in an inviscid and Boussinesq framework. The plane of the jet is assumed to be inclined with an angle $\theta $ with respect to the vertical direction of stratification. The stability analysis is performed using both numerical and theoretical methods for all the values of $\theta $ and Froude number $F= {U}_{0} / (LN)$. We first obtain that the most unstable mode is always a two-dimensional Kelvin–Helmholtz (KH) sinuous mode. The condition of stability based on the Richardson number $Ri\gt 1/ 4$, which reads here $F\lt 3 \sqrt{3} / 2$, is recovered for $\theta = 0$. But when $\theta \not = 0$, that is, when the directions of shear and stratification are not perfectly aligned, the Bickley jet is found to be unstable for all Froude numbers. We show that two modes are involved in the stability properties. We demonstrate that when $F$ is decreased below $3 \sqrt{3} / 2$, there is a ‘jump’ from one two-dimensional sinuous mode to another. For small Froude numbers, we show that the shear instability of the inclined jet is similar to that of a horizontal jet but with a ‘horizontal’ length scale ${L}_{h} = L/ \sin \theta $. In this regime, the characteristics (oscillation frequency, growth rate, wavenumber) of the most unstable mode are found to be proportional to $\sin \theta $. For large Froude numbers, the shear instability of the inclined jet is similar to that of a vertical jet with the same scales but with a different Froude number, ${F}_{v} = F/ \hspace *{-.1pc}\cos \theta $. It is argued that these results could be valid for any type of shear flow.


1966 ◽  
Vol 24 ◽  
pp. 118-119
Author(s):  
Th. Schmidt-Kaler

I should like to give you a very condensed progress report on some spectrophotometric measurements of objective-prism spectra made in collaboration with H. Leicher at Bonn. The procedure used is almost completely automatic. The measurements are made with the help of a semi-automatic fully digitized registering microphotometer constructed by Hög-Hamburg. The reductions are carried out with the aid of a number of interconnected programmes written for the computer IBM 7090, beginning with the output of the photometer in the form of punched cards and ending with the printing-out of the final two-dimensional classifications.


1966 ◽  
Vol 24 ◽  
pp. 3-5
Author(s):  
W. W. Morgan

1. The definition of “normal” stars in spectral classification changes with time; at the time of the publication of theYerkes Spectral Atlasthe term “normal” was applied to stars whose spectra could be fitted smoothly into a two-dimensional array. Thus, at that time, weak-lined spectra (RR Lyrae and HD 140283) would have been considered peculiar. At the present time we would tend to classify such spectra as “normal”—in a more complicated classification scheme which would have a parameter varying with metallic-line intensity within a specific spectral subdivision.


1966 ◽  
Vol 25 ◽  
pp. 46-48 ◽  
Author(s):  
M. Lecar

“Dynamical mixing”, i.e. relaxation of a stellar phase space distribution through interaction with the mean gravitational field, is numerically investigated for a one-dimensional self-gravitating stellar gas. Qualitative results are presented in the form of a motion picture of the flow of phase points (representing homogeneous slabs of stars) in two-dimensional phase space.


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