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28 Jul 2006: as to be expected, the figure is much lower for the 200 journals with highest cumulative impact.

21 Sep 2006: Furthermore, since the size of the ROIs may vary from one videoto the other, the final MGO images are resized to the corresponding refined images withstandard size (which is 200 200 ... 3.2 Dimension Reduction by PCA. In order to reduce the number of

30 May 2006: Y f 5 200 -. 6 a. 250 -. 300 -. Salinity ( % o ). I I I I I I I I 34.2 34.3 3 4 4 34.5 34.6 34.7 ... 200. n E. 300. 350. I I 0.1 OC. FIGURE 8.

5 May 2006: Details of our finite-difference numericalcode are presented the Appendix. We used a mesh of 320 horizontal and 200 verticalintervals.

21 Sep 2006: 0 50 100 150 200 250 300 350 4000.25. 0.2. 0.15. ... Fea. ture. Val. ueBatch OSMINC OSM. 50 100 150 200 250 300 350 4000.

6 Dec 2006: 150 C, 200 C, 250 C, and 300 C at various nitgen pressures. ... Above 200 Cconductivity becomes almost independent of N contentits dependence on temperature declines.

19 Apr 2006: up to 200 km in diameter) for impacts with a range ofimpact parameters and with relative velocities comparable to thoseexpected in extrasolar planetesimal discs. ... 6b), all models predict a lifetimethat is shorter than the age of the system (200 Myr)

19 Apr 2006: Compared to the fullextent of the mid-IR–emitting size of the disk (200 AU), therelatively small values of the dust FWHM sizes suggest thatthe mid-IR emission is sharply peaked ... extends out to at least a radius of 100 (200 AU) fromthe star in the

13 Nov 2006: 3(b). The AFM analysis shows a w of 40,200 and 100 nm for a respective original 0.3-, 1- and 5-nmFe thickness (Figs. ... Annealing in pure NH3 (200 sccm, 0.6 mbar pressure) at500 C results in a distinctively different topography for all Fethicknesses.

6 Dec 2006: 5 ] to films deposited. by cathodic arc systems. Doping in ta-C can only bedecreases from 300 cm1 to 200 cm1 for temperaturesbetween room temperature and 200C.