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27 Apr 2006: 0 0. c) loo. 50 100 150 200. TIME (yrs). 50 100 150 200. ... 100. 8O. 60. 40. 20. O " '. ". ' ". " ' -. 0 50 100 150 200. TIME (yrs) Fig.

19 Apr 2006: This 200-AU-sized regioncoincides with the slightly tilted inner disk identified optically withthe Hubble Space Telescope5. ... The possible relationship of these components has yetto be explored, but the lower inferred temperatures of the clumpparticles

30 May 2006: J. F u i d Xech. (19761, VOZ. 78, part 4? pp. 821-854 Printed in Great Britain. 82 1. Nonlinear double-diffusive convection By H E R B E R T E. H U P P E R T A N D D A N I E L R. MOORE. Department of Applied Mathematics and Theoretical Physics,

2 Nov 2006: belt width isdr = 0.5r; planetesimal strength is Q?D = 200 J kg. ... kg m3, e = 0.05, e/I = 1,Q?D = 200 J kg.

19 Jul 2006: Gaussianise the data for each speaker:. 20 15 10 5 0 5 10 15 200. ... 0.01. 0.02. 0.03. 0.04. 0.05. 0.06. 0.07. 0.08. 0.09. 0.1. 20 15 10 5 0 5 10 15 200.

7 Sep 2006: 0 100 200 300 400. 50. 100. 150. 200. 250. p1 p2. ... 100 200 300 400 500 600. 100. 200. 300. 400. 500.

22 Nov 2006: 180 190 200 210 220 2300. 50. 100. Frame. aii. Figure 3: Plot of log energy for snippet from AURORA digit string8-6-Zero-1-1-6-2, showing joint ... Asanticipated, the extremes previously observed have disappeared. 180 190 200 210 220 230.

30 May 2006: h. 5 200 - 9. ( b ) 400. 34 4 34 5 34 6 34 1 34 4 34 5 34 6 34 7 S ( % a ) S ( % O ). B I L t<h ... 100 0.0026 0.0061 0.0083 0.0184 150 0.0035 0.0077 0.0092 0.0198 200 0.0041 0.0088 00101 0.0210.

6 Apr 2006: pid: 2191 at: Fri Mar 24 13:51:25 2006 pid: 2247 at: Fri Mar 24 13:53:41 2006 Initial setup complete InitialiseAll 1006 foe UCID:0.1 InitialiseModule 20220170100028 InitialiseModule 20220170100056 InitialiseRod SendPrimList (UCID:0.1 1)

11 Oct 2006: 1992). The typical grid has 200 intervals over [0, xN (t)] and a time step of0.04. ... 2 4 6 8 10 12 14 16 18 200.