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Scaling Aspects of Lyari River Flow Routing [PDF]
In this communication we utilize an improved version for model proposed by Manning for the waste flow via an open channel Lyari. We have computed the status of discharges, storages and depth for all locations of the Lyari waste flow using this proposed ...
Asif Mansoor, Rana Khalid Naeem
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Computers & Fluids, 2002
zbMATH Open Web Interface contents unavailable due to conflicting licenses.
Sadri, R. M., Floryan, J. M.
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zbMATH Open Web Interface contents unavailable due to conflicting licenses.
Sadri, R. M., Floryan, J. M.
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Shallow Water Flows in Channels
Journal of Scientific Computing, 2010zbMATH Open Web Interface contents unavailable due to conflicting licenses.
Gerardo Hernández-Dueñas, Smadar Karni
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SIAM Journal on Scientific and Statistical Computing, 1990
A method is presented for calculating potential flows in infinite channels. Given a collection of N sources in the channel and a zero normal flow boundary condition, the method requires an amount of work proportional to N to evaluate the induced velocity field at each source position.
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A method is presented for calculating potential flows in infinite channels. Given a collection of N sources in the channel and a zero normal flow boundary condition, the method requires an amount of work proportional to N to evaluate the induced velocity field at each source position.
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Sunspot Plumes and Flow Channels
Solar Physics, 2001It is well known that sunspots are dark. This statement is not correct in the sunspot atmosphere between the chromosphere and the corona, where sunspots often are brighter than their surroundings. The brightest feature in the sunspot transition region is called a sunspot plume. Not all sunspots contain a plume. We find that 20 out of 21 sunspots show a
Brynildsen, N. +4 more
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Hydromagnetic flow in a rotating channel
Applied Scientific Research, 1971The steady flow in a parallel plate channel rotating with an angular velocity Ω and subjected to a constant transverse magnetic field is analysed. An exact solution of the governing equations is obtained. The solution in the dimensionless form contains two parameters: the Hartmann number, M2, and K2 which is the reciprocal of the Ekman number.
Nanda, R. S., Mohanty, H. K.
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Axisymmetric Magnetohydrodynamic Channel Flow
Journal of the Aerospace Sciences, 1962Summary x =: axial component r = radial component = condition at wall The axisymmetric subsonic and supersonic flow fields, and the skin friction and heat transfer of an electrically conducting com pressible fluid flowing in a channel of constant circular area through a magnetic field are investigated when the magnetic Remolds number is small.
Hains, F. D., Yoler, Y. A.
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2001
In previous chapters, we derived the differential equations governing the motion of an incompressible Newtonian fluid by requiring mass conservation and enforcing Newton’s second law of motion for infinitesimal fluid parcels. The governing equations are accompanied by initial, boundary, and interfacial conditions, as required.
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In previous chapters, we derived the differential equations governing the motion of an incompressible Newtonian fluid by requiring mass conservation and enforcing Newton’s second law of motion for infinitesimal fluid parcels. The governing equations are accompanied by initial, boundary, and interfacial conditions, as required.
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