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17 May 2006: 4Laboratoire de Physique Statistique, UMR 8550 CNRS, Ecole Normale Supérieure, 24,rue Lhomond, 75231 Paris cédex 05, France. ... 1. 2. –12. 3. 10. G. I. IG. (ν. /g2 ). 1/3. ̂. H(g/ν2)1/3 Ĥ. ̂ (Ĥ/)10/3Π15/9. Π15/24. Π15/96. Π1–1/6

9 Mar 2004: 0.9993 4.81 0 1.52 – –S3 0 45.8 79.80 0.574 1.375 1.0192 0.9996 19.24 0 1.36 – –S7 0 45.2 ... 19.24 0.0282 1.37 550 0.100R10 0.0500 46.3 79.97 0.579 1.390 1.0107 1.0007 9.80 0.0551 0.99 450

26 Mar 2023: 1r. rrp1r. n2. r2p1 = 0. (4.24). The solution, finite at r = 0, is p1(r, t) = k(t)rn, so that now p(r, θ, t) = p0(r, t)

7 Aug 2008: Uc ={. (3 2M)1/4β, for M 2D 3/24/3 3,(3/24/3 2D M.

30 May 2006: Stability of a large gas bubble rising through liquid 417. 24. ... 1. oo 1.712 1.26 1.42 1.10 1.24. 13.61 1.200 0.79 1.06 1.

11 Apr 2013: 2 2 2. 24/.467. 35.1 Introduction.

18 May 2017: on the y-axis,with τ of (a) 0.085, (b) 0.24, (c) 0.39, (d) 0.55, (e) 0.71, ( f ) 0.87, (g) 1.00 and ... mUmH. 3F10 , (4.23). q= UmH2. sin2/3 θE2/3eq D1F1/30 , (4.24).

1 Jun 2006: 0.01 (for Ra, = lo@), convection continues in the melt until t = 0.24, by which time the system is about 40% solidified.

10 Mar 2011: Hr XNn1. dhndx. dxnd1. XNn1. hn! 3XNn1. h3n. 24. 35, ð61aÞ.

26 Apr 2006: e-mail: grae@esc.cam.ac.uk; heh1@esc.cam.ac.uk. (Received 24 July and in revised form 27 March 1997). ... 24/3λRa1/3 (3.1). between the Nusselt number Nu for thermal convection in the liquid region and theRayleigh number.

5 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).

14 Apr 2010: 6νq0g. )1/3 ( gg′. )2/3(2.24). and St = 2q0(. 6νq0g. )2/3 ( gg′.

15 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.

30 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.

24 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

1 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.

10 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.

1 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

26 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.

6 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.