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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. 372 H. E. Huppert and 144. E. Stern. $1. , //,/,////,//////////////,,,/,////// / ///,/I/ // / / / , // , / , / // , / / / / // / /, /' I -. FIGURE 1. An elevation of the channel, bounded by vertical walls at. ... Moh(x/L) e--ikg. (3.24). While in

19 Apr 2006: MIR.but more common around stars < 100 Myr. MIPS 24 um image of Vega disk. ... MIPS-24 MIPS-70. MIPS-160 JCMT-450CSO-350. HST. Do Stars with Inner Planets (< 5 AU) Also Have Kuiper Disks?

5 May 2006: We areinterested in cases with small C2H because otherwise the distance of propagation issmall, see (3.24), and no real gravity current appears. ... Using the approximations (3.19)–(3.24), we find: (i) for S < 1.

20 Jun 2006: 24. Intriguingly, Filon-type methods (3.11) lend themselves to an alternative interpretation.Comparing (3.11) with (3.1), we observe that. ... Num. Anal.24, 365–391. Iserles, A. & Nørsett, S. P. (2004), ‘On quadrature methods for highly oscillatory

5 Jul 2006: Complementary System Selection (“Random”). • Variability to systems can be obtained by varying for example:– segmentation and clustering [3]– acoustic model decision tree [24]– acoustic model context (tri/quin-phone) [4]– ... Cambridge

21 Sep 2006: 21] for upper bodypose estimation. In [24] it is suggested to partition the parameter spaceof a 3D hand model using a multi-resolution grid. ... range. At detection rates of 0.99 the false positiverate for the centre template is 0.24, wheras it is

1 Jun 2006: Okuz. 24 FLU 251.

27 Apr 2006: 2.18), which can be (2.23) and (2.24) more closely.used in (2.22) to show that Segregation is more sensitive to the value of. ... 4.24)mass reduce to and we use this condition together with (4.21)—.

26 Apr 2006: Leppäranta, pp. 24–104,Univ. of Helsinki Press, Helsinki, 1998. Wettlaufer, J. S., Heat flux at the ice-ocean interface, J. ... E. Huppert, The phase evolution ofyoung sea ice, Geophys. Res. Lett., 24, 1251–1254, 1997a.

30 Mar 2006: Examples includequasistatic compression imaging [26, 29], axial shear wave imaging [32] and acoustic radiationforce imaging in both quasistatic/impulsive [24] and dynamic [2] forms. ... We substitute this into Equation 24, and rearrange to produce a

13 Nov 2006: 26] (see footnote 24, for qK, 00 0) andRef. [24]. This differs from the model of Ref. ... Pfeiffer et al., Phys. Rev. B 71, 155409 (2005).[24] J. Maultzsch, S.

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.

26 Apr 2006: salinity of the ice) is very small; k #1 0 24 [Gross et al., 1987].

26 Apr 2006: H inner H s0D D0. 1. 1 : (24). Importantly, we have a value for the apparent cotangent.

23 Sep 2006: Date: September 24, 2006. Speakers: Dr Pete Moore.

1 Jun 2006: 1 -. f = 16-21 min. 24.5 25.0 25.5 26.0 26.5 27.0 27.5 28.0 28.5 29.0 T. ... 0 - 1 24.5 25.0 25.5 26.0 26.5 27.0 27.5 28.0 28.5 29.0 29.5 30.0 30.5.

20 Feb 2006: 2419.5. 2324.5. 2208.94. 2206.19. 2108.67. 2097.96. 2042.24. 2038.81. 1984.96. 1819.94. 1815.18. ... 1211.24. 1176.47. 1147.32. 1080.84. 1012.11. 963.47. 771.78. 655.02. 509.12. 456.62. 456.58.

12 Apr 2006: 1 5 1 6 1 7 1 8 1 9 20 2 1 2 2 2 3 24 2 5.

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).