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doi: 10.1098/rspa.2009.0434 published online 13 January 2010Proc. R.…
www.itg.cam.ac.uk/people/grae/92.pdf14 Apr 2010: 6νq0g. )1/3 ( gg′. )2/3(2.24). and St = 2q0(. 6νq0g. )2/3 ( gg′. -
flm483.dvi
www.itg.cam.ac.uk/people/heh/Paper186.pdf5 Jan 2006: The experimentswere generally left to run for 24 hours, but heat loss to the laboratory became asignificant factor after roughly 10 hours. ... dy. dτ= (1 θ). (1 y)(1 Λθ). (3.24). y(τ = 0) = 1, (3.25). -
The Generation of Granitic Magmas by Intrusion of Basalt ...
www.itg.cam.ac.uk/people/heh/Paper83.pdf15 Sep 2006: There is also. [Journal of Petrologf, Vol. 29, P t n 3, pp 599-«24, 1988] Oxford Umvcroty Prcu 19S8. ... FJH,. (24). We determined numerical solutions of (15)—(18) in addition to either (19)—(23) or merely (24).The differences were negligible. -
Gravity currents entering a two-layer fluid
www.itg.cam.ac.uk/people/heh/Paper37.pdf30 May 2006: 24-2. 740 J. Y. Holyer and H. E. Huppert. model for energy dissipation. ... The wavelengths given by (6.3) and (6.4) are 6.1 cm on the lower interface and 24-1 cm on the upper interface. -
The transient behaviour of alloys solidified from below prior to the…
www.itg.cam.ac.uk/people/grae/23.pdf1 Jun 2006: 24 M. G. Worster and R. C. Kerr. with most metals, it has a low entropy of fusion and forms highly branched, rather than prism-like, crystals. -
doi:
www.itg.cam.ac.uk/people/heh/Paper245.pdf24 Apr 2014: The approximate constancy of the late-time first-ordercorrection (E 1.38t1/2) 0.24 is due to the adjustment of the radial flow near thesource towards unidirectional flow over a -
Dense Suspension Flow in a Penny-Shaped Crack, Part I : Theory
www.itg.cam.ac.uk/people/heh/Paper278.pdf26 Mar 2023: 4𝜉3. 𝜕𝜙𝜕𝜉. 𝜂3𝜕𝜙𝜕𝜂. = 1𝛤𝜉. 𝜕(𝜉𝜙𝑣𝑟)𝜕𝜉. 𝜕(𝜙𝑣𝑧)𝜕𝜂. (24). Integrating from 𝑤 to 𝑤 with respect to 𝜂, leaving details to Appendix A for brevity, we obtain. -
A new oscillatory instability in a mushy layer during the…
www.itg.cam.ac.uk/people/grae/27.pdf1 Jun 2006: I. / / ,. /. /. 4 8. 36. (TI1 24. I 32. / / / ’. I. -. -_ -._ - _ -.-__ ---_ -.__. 4.5 0 2 4 6 8 10. %. ... 1 4 8 Unstable. It. / / ,. /. /. 36. (TI1 24. 0 0.2 0.4 0.6 6. FIGURE 5. The critical Rayleigh numbers as they vary with the dimensionless -
Energy balances for axisymmetric gravity currents in homogeneous and…
www.itg.cam.ac.uk/people/heh/Paper213.pdf10 Mar 2009: Conservation of volume. v = 0. (2.24)2. Momentum balance. ρDv. Dt= p (ρ ρb)g ẑ μ2v, (2.25). ... After some algebra and use of(2.24), we obtain. ρD. Dt. [1. -
The effect of confining impermeable boundaries on gravity currents in …
www.itg.cam.ac.uk/people/heh/Paper221.pdf6 May 2010: Sd 75 0.24. V 1 20 200 V a 44 0.20 V 2 60 100 V b 75 0.25V 3 40 150 V 4 40 62.
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