Search

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.

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.

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,

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.

27 Nov 2006: The second algorithm,. 16. 0. 100. 200. 300. 400. 0 5 10 15 20Nkt jet. ... 10. 10 2. 10 3. 10 4. 0 200 400 600 800 1000.