Abstract
We will consider here stationary axisymmetric fluid flow over disks rotating with a sufficiently high angular velocity so that effects of gravitational forces on momentum transfer are rather low. In a stationary cylindrical coordinate system arranged in such a way that a disk or a system of disks rotate around its axis of symmetry coinciding with the axis
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© 2009 Springer-Verlag Berlin Heidelberg
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Shevchuk, I.V. (2009). Modelling of Fluid Flow and Heat Transfer in Rotating-Disk Systems. In: Convective Heat and Mass Transfer in Rotating Disk Systems. Lecture Notes in Applied and Computational Mechanics, vol 45. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-00718-7_2
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DOI: https://doi.org/10.1007/978-3-642-00718-7_2
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Publisher Name: Springer, Berlin, Heidelberg
Print ISBN: 978-3-642-00717-0
Online ISBN: 978-3-642-00718-7
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