1989
DOI: 10.1299/jsmeb1988.32.1_52
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Liquid Film Formation on a Rotating Disk (Numerical Analysis at the Initial Stage)

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Cited by 8 publications
(6 citation statements)
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“…ω << µ/ρh 2 (12) where µ is the viscosity of liquid and h is the film thickness. In practice this means that for a fluid of ρ = 1.0 g/cm 3 , µ = 10 g/(m-s), and h around 120 µm, ω must be much less than 6945 rpm.…”
Section: Resultsmentioning
confidence: 99%
See 1 more Smart Citation
“…ω << µ/ρh 2 (12) where µ is the viscosity of liquid and h is the film thickness. In practice this means that for a fluid of ρ = 1.0 g/cm 3 , µ = 10 g/(m-s), and h around 120 µm, ω must be much less than 6945 rpm.…”
Section: Resultsmentioning
confidence: 99%
“…[7][8][9] Many mathematical models were also developed to analyze the time-varying behavior of spin coating flows; however, initial film thickness contours were required. [10][11][12][13][14][15][16][17] In the real spin coating process utilized by the microelectronics industry, the photoresist or polyimide is injected onto a high speed rotating wafer. Only after the film has spread over the entire disk can the initial film thickness contours required by the above investigators be obtained.…”
Section: Reduction Of Photoresist Usage During Spin Coatingmentioning
confidence: 99%
“…They established the basic mechanisms of thread and drop formation by rotating discs. Matsumoto et al 8 analysed the initial stage of the unsteady film formation process by solving the full Navier Stokes equations and showing the initial pattern of film flow on a rotating disc. Bruin 9 analysed the radial, tangential and meridional velocity profiles in a liquid film flowing over a rotating conical disc, and the velocity profiles were obtained through a complex function method with high accuracy.…”
Section: Introductionmentioning
confidence: 99%
“…With an objective of obtaining a numerical solution of the film flow on a rotating disk for a wide range of Reynolds numbers and spin-up protocols, Rehg and Higgins (1988) have solved the self-similar form of the Navier-Stokes equations under planar interface assumption and have characterized the import of inertia and disk acceleration on film thinning rates. Matsumoto et al (1989) have solved the unsteady problem of film flow on a rotating disk numerically for a non-planar interface model. Reisfeld et al (1991) have examined the flow of a thin liquid film on a rotating disk, subject to centripetal and inertial forces, surface tension, gravity and constant mass transfer at the free surface and have obtained the conditions for film instability in several regions of interest using linear stability theory.…”
Section: Introductionmentioning
confidence: 99%