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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.

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.

19 Apr 2006: ac-count and 200 dust particles were produced with exactlythe same positions and velocities as the parent popula-tion. ... for the librationparameters to be fitted for each particle, and the meanparameters for each population of 200 dust grains to

1 Jun 2006: 4. 0. Tc W). - 4. 0 200 400 600 800. ... Part 2 347. Equilibrium. t (min). 200 400 600 800. t (min).

1 Jun 2006: I I I. I I I I 0 200 400 600 800. ... about half a year (hi = 200 cm and T / = 1016 "C).

20 Jun 2006: 6. 200. 0.5. 0.4. 0.3. 100. 0.2. 0.1. 800. 6040. 0.1. ... 200. 0 8060. 0.2. 40. 0.3. 100. 0.4. 200. 0.25. 0.2.

27 Apr 2006: 8 c ) and is graphed in Fig. 5. 200 -. 160 h(m). 120. 8 0 -. 4 0 -. 107. o ,6o 26o 36o r(m). ... t f o r d i s c u s s i o n ). 0 200 400 600 Metres I i I. SCALE. Fig. 9.

19 Apr 2006: Accurate telescope pointing wascrucial to these observations and was checked before andafter each map using the nearby blazar 2255282 with rmserror of less than 200. ... Very littleinformation can be deduced about sizes or positions differ-ing by 200,

18 Sep 2006: In t h e case o f olivine, the best available estimate of L is 200 cal g m - 1 (Bottinga a n d Richet 1978), a n d ... 3. 100. o. z 200. I 0 I 0 0 I 0 0 0.