W>648_wo>2331_word_end<_end702_wo>2331_word_end<_end

>2061_wo>2331_word_end<_end<4>2063_wo>2331_word_end<_end<

Xiaoshi Zhang, Eric Mountfo>2331_word_end<, Mat>2329_wo>2331_word_end<_end636_wo>2331_word_end<_end<

>2071_wo>2331_word_end<_end<4>2073_wo>2331_word_end<_end<

 

2329_wo>2331_word_end<_end
2102_wo>2331_word_end<_end2102_wo>2331_word_end<_end<-euv-at-25-50-nm-using->2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end<->2329_wo>2331_word_end<_end2102_wo>2331_word_end<_end<-astrella/>2102_wo>2331_word_end<_end<-astrella.jpg" alt=">2102_wo>2331_word_end<_end<-astrella.jpg" title=">2102_wo>2331_word_end<_end<-astrella.jpg"/>
2329_wo>2331_word_end<_end
2102_wo>2331_word_end<_end2102_wo>2331_word_end<_end<-euv-at-25-50-nm-using->2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end<->2329_wo>2331_word_end<_end2102_wo>2331_word_end<_end<-astrella/kmlabs-xuus4.jpg" alt="kmlabs-xuus4.jpg" title="kmlabs-xuus4.jpg"/>

>2100_wo>2331_word_end<_end<

>2101_wo>2331_word_end<_end< >2102_wo>2331_word_end<_end< >2103_wo>2331_word_end<_end<>2104_wo>2331_word_end<_end< >2105_wo>2331_word_end<_end<>2106_wo>2331_word_end<_end< >2107_wo>2331_word_end<_end< >2108_wo>2331_word_end<_end< >2109_wo>2331_word_end<_end<>2110_wo>2331_word_end<_end< >2111_wo>2331_word_end<_end<>2112_wo>2331_word_end<_end< >2113_wo>2331_word_end<_end<>2114_wo>2331_word_end<_end< >2115_wo>2331_word_end<_end<>2116_wo>2331_word_end<_end< or to enable >2102_wo>2331_word_end<_end< imaging wi>2329_wo>2331_word_end<_end< spatial resolution as high as 12 nm.>2106_wo>2331_word_end<_end<

>2119_wo>2331_word_end<_end<>2120_wo>2331_word_end<_end< >2121_wo>2331_word_end<_end< >2122_wo>2331_word_end<_end< >2123_wo>2331_word_end<_end< >2124_wo>2331_word_end<_end< >2125_wo>2331_word_end<_end< >2126_wo>2331_word_end<_end< of a source. Even >2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end2126_wo>2331_word_end<_end< of an HHG-based EUV source requires a comprehensive approach >2329_wo>2331_word_end<_end

>2128_wo>2331_word_end<_end<>2129_wo>2331_word_end<_end< >2130_wo>2331_word_end<_end<4>2132_wo>2331_word_end<_end<>2133_wo>2331_word_end<_end< >2134_wo>2331_word_end<_end<4>2136_wo>2331_word_end<_end<4 >2138_wo>2331_word_end<_end< 

2329_wo>2331_word_end<_end
2102_wo>2331_word_end<_end2102_wo>2331_word_end<_end<-euv-at-25-50-nm-using->2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end<->2329_wo>2331_word_end<_end2102_wo>2331_word_end<_end<-astrella/xuus-astrella-system-test-configuration.jpg" alt="Figure 1" title=""/>

>2150_wo>2331_word_end<_end< >2151_wo>2331_word_end<_end<4>2153_wo>2331_word_end<_end<4>2155_wo>2331_word_end<_end<4>2157_wo>2331_word_end<_end<

 

>2164_wo>2331_word_end<_end< 

The configuration used for testing is shown in >2150_wo>2331_word_end<_end< It consists of >2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end2267_wo>2331_word_end<_end<4 >2167_wo>2331_word_end<_end<4 >2169_wo>2331_word_end<_end< 

 

>2171_wo>2331_word_end<_end<

The Coherent Astrella® amplifier laser system is an industrial-grade one-box ultrafast Ti:sapphire laser amplifier developed and constructed using H>626_wo>2331_word_end<_end2203_wo>2331_word_end<_end< per pulse at 800 nm wi>2329_wo>2331_word_end<_end< < 35 fs pulse wid>2329_wo>2331_word_end<_end< at a repetition-rate of >2215_wo>2331_word_end<_end< (Table 1). All >2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end< Coherent Revolution® Q-switched Nd:YLF laser, and finally a pulse compressor. The Astrella® design has been extensively tested for reliability and robust long-term operation.

 

>2174_wo>2331_word_end<_end<4 ™

>2177_wo>2331_word_end<_end<4 ™ is a highly engineered HHG source and beamline system >2329_wo>2331_word_end<_end2102_wo>2331_word_end<_end< EUV light wi>2329_wo>2331_word_end<_end2267_wo>2331_word_end<_end<4 >2181_wo>2331_word_end<_end<

>2182_wo>2331_word_end<_end<4 >2184_wo>2331_word_end<_end<4 ™ configuration and drive laser parameters, produces a >2102_wo>2331_word_end<_end< EUV or soft x-ray beam wi>2329_wo>2331_word_end<_end< waveleng>2329_wo>2331_word_end<_end< >2329_wo>2331_word_end<_end2177_wo>2331_word_end<_end<4 >2188_wo>2331_word_end<_end<>2129_wo>2331_word_end<_end< >2190_wo>2331_word_end<_end<4 >2192_wo>2331_word_end<_end<

 

2331_word_end

>2200_wo>2331_word_end<_end<

>2201_wo>2331_word_end<_end<

>2202_wo>2331_word_end<_end<

>2203_wo>2331_word_end<_end<

>2204_wo>2331_word_end<_end<

>2205_wo>2331_word_end<_end<

>2206_wo>2331_word_end<_end<

>2207_wo>2331_word_end<_end<

>2208_wo>2331_word_end<_end<

>2209_wo>2331_word_end<_end< 

>2210_wo>2331_word_end<_end<

>2211_wo>2331_word_end<_end<

>2212_wo>2331_word_end<_end<

>2213_wo>2331_word_end<_end<

>2214_wo>2331_word_end<_end<

>2215_wo>2331_word_end<_end<

>2216_wo>2331_word_end<_end<2)

>2219_wo>2331_word_end<_end<

>2220_wo>2331_word_end<_end<

>2221_wo>2331_word_end<_end<

>2222_wo>2331_word_end<_end<2 >2224_wo>2331_word_end<_end<0)

>2227_wo>2331_word_end<_end<

>2228_wo>2331_word_end<_end<

<0.5% R>674_wo>2331_word_end<_end< for 8hrs

>2232_wo>2331_word_end<_end< >2233_wo>2331_word_end<_end<4>2235_wo>2331_word_end<_end<

 

>2242_wo>2331_word_end<_end<2 >2244_wo>2331_word_end<_end<

 

2329_wo>2331_word_end<_end
2102_wo>2331_word_end<_end2102_wo>2331_word_end<_end<-euv-at-25-50-nm-using->2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end<->2329_wo>2331_word_end<_end2102_wo>2331_word_end<_end<-astrella/xuus-astrella-hhg-spectrum.jpg" alt=">2257_wo>2331_word_end<_end<" title=""/>

>2257_wo>2331_word_end<_end<>2258_wo>2331_word_end<_end<11 >2260_wo>2331_word_end<_end<

 

2331_word_end

>2267_wo>2331_word_end<_end<4>2269_wo>2331_word_end<_end<

>2201_wo>2331_word_end<_end<

>2271_wo>2331_word_end<_end<

>2272_wo>2331_word_end<_end<11 >2274_wo>2331_word_end<_end<

>2275_wo>2331_word_end<_end<

>2276_wo>2331_word_end<_end<7 >2274_wo>2331_word_end<_end<

>2279_wo>2331_word_end<_end<

>2280_wo>2331_word_end<_end<

>2281_wo>2331_word_end<_end<

>2282_wo>2331_word_end<_end<

>2283_wo>2331_word_end<_end<

>2228_wo>2331_word_end<_end<

<6.5 % R>674_wo>2331_word_end<_end< for 1 hour

>2288_wo>2331_word_end<_end< Observed >2267_wo>2331_word_end<_end<4>2291_wo>2331_word_end<_end<

 

>2298_wo>2331_word_end<_end<

As a collaborative effort, KMLabs and Coherent conducted HHG measurements at Coherent’s facility in Santa Clara, using a production Astrella® laser and >2267_wo>2331_word_end<_end<4™. After initial characterization of >2329_wo>2331_word_end<_end2126_wo>2331_word_end<_end< of a telescope to adjust >2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end2267_wo>2331_word_end<_end<4>2303_wo>2331_word_end<_end<

We evaluated >2329_wo>2331_word_end<_end2267_wo>2331_word_end<_end2329_wo>2331_word_end<_end< regions: a) a “near EUV” spectrum generated in Argon gas wi>2329_wo>2331_word_end<_end< >2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end< spectrum peaked at 13.5 nm. For case a) >2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end< >2329_wo>2331_word_end<_end2207_wo>2331_word_end<_end<, while for case b) it was >2208_wo>2331_word_end<_end<. It is important to note >2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end702_wo>2331_word_end<_end< for pump-probe experiments.

>2305_wo>2331_word_end<_end<

 

2329_wo>2331_word_end<_end
2102_wo>2331_word_end<_end2102_wo>2331_word_end<_end<-euv-at-25-50-nm-using->2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end<->2329_wo>2331_word_end<_end2102_wo>2331_word_end<_end<-astrella/xuus-stability-over-1-hour.jpg" alt="Figure 3"/>

>2318_wo>2331_word_end<_end< Stability of >2267_wo>2331_word_end<_end<4>2321_wo>2331_word_end<_end<

 

The EUV spectrum obtained for case a) and b) are shown in >2257_wo>2331_word_end<_end< and Figure 4 respectively, while >2329_wo>2331_word_end<_end2318_wo>2331_word_end<_end< The shape of >2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end2331_word_end2331_word_end2257_wo>2331_word_end<_end< consists of odd harmonics (17-27>2329_wo>2331_word_end<_end<), peaked at >2329_wo>2331_word_end<_end>2331_word_end<. The flux measured at >2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end2272_wo>2331_word_end<_end<11 (+/-20%) >2274_wo>2331_word_end<_end< for >2329_wo>2331_word_end<_end>2331_word_end< harmonic at 35 nm (hν = 35 eV). The flux measured on >2329_wo>2331_word_end<_end7 ph/sec, where in >2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end

In setting-up experiments using EUV light, >2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end<, as well at >2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end2329_wo>2331_word_end<_endThe specifics of >2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end2329_wo>2331_word_end<_endmust be considered in any calculations of experimental >2329_wo>2331_word_end<_end

Figure 4 shows >2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end7 >2274_wo>2331_word_end<_end<, at >2329_wo>2331_word_end<_end based on a measured flux at >2329_wo>2331_word_end<_end4 ph/sec. Thus, HHG to 13.5 nm (92 eV) is possible using >2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end2331_word_end2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end2267_wo>2331_word_end<_end<4™ /우리카지노 바카라사이트® setup primarily for HHG up to hν~50 eV.

 

2329_wo>2331_word_end<_end
2102_wo>2331_word_end<_end2102_wo>2331_word_end<_end<-euv-at-25-50-nm-using->2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end<->2329_wo>2331_word_end<_end2102_wo>2331_word_end<_end<-astrella/xuus-astrella-euv-generation.jpg" alt="Figure 4"/>

Figure 4. Generation of 13.5 nm EUV using >2329_wo>2331_word_end<_end2267_wo>2331_word_end<_end< for HHG in Helium gas. The >2122_wo>2331_word_end<_end2208_wo>2331_word_end<_end<. The spectral bandwid>2329_wo>2331_word_end<_end< (FWHM) of >2329_wo>2331_word_end<_end>2329_wo>2331_word_end<_end<) is ~0.5 nm. The total flux in >2329_wo>2331_word_end<_end7 >2274_wo>2331_word_end<_end< at >2329_wo>2331_word_end<_end2331_word_end2329_wo>2331_word_end<_end

 

Summary and 우리카지노 바카라사이트nclusions

The >2267_wo>2331_word_end<_end<4™ system is >2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end< >2329_wo>2331_word_end<_end2267_wo>2331_word_end<_end<4™.

 

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2. DF Ga>2331_word_end640_wo>2331_word_end<_end< Adams, HC Kapteyn, MM Murnane, and GF Mancini, "Subwaveleng>2329_wo>2331_word_end<_end< >2102_wo>2331_word_end<_end< imaging of periodic samples using a 13.5 nm tabletop high-harmonic light source," Nat Photon 11(4), 259-263 (2017). dx.doi.org/10.1038/nphoton.2017.33.

3. E Gagnon, P Ran우리카지노 바카라사이트ovic, A Paul, CL Cocke, MM Murnane, HC Kapteyn, and AS Sandhu, "Soft x-ray driven femtosecond molecular dynamics," Science 317(5843), 1374-1378 (2007). 

4. D Rudolf, C La-O-Vorakiat, M Battiato, R Adam, JM Shaw, E Turgut, P Maldonado, S Ma>2329_wo>2331_word_end<_end2331_word_end1572_wo>2331_word_end<_end< 3, 1037 (2012). dx.doi.org/10.1038/ncomms2029

5. S Ma>2329_wo>2331_word_end<_end664_wo>2331_word_end<_end< Siemens, S Eich, CM Schneider, TJ Silva, M Aeschlimann, MM Murnane, and HC Kapteyn, "Probing >2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end125_wo>2331_word_end<_end< of America 109(13), 4792-4797 (2012). dx.doi.org/10.1073/pnas.1201371109

6. C Chen, ZS Tao, A Carr, P Matyba, T Szilvasi, S Emmerich, M Piecuch, M Keller, D Zusin, S Eich, M Rollinger, WJ Youa, S Ma>2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end125_wo>2331_word_end<_end< of America 114(27), E5300-E5307 (2017). dx.doi.org/10.1073/pnas.1706466114

7. KM Hoogeboom-Pot, E Turgut, JN Hernandez-Charpak, JM Shaw, HC Kapteyn, MM Murnane, and D Na>2331_word_end2329_wo>2331_word_end<_end

8. KM Hoogeboom-Pot, JN Hernandez-Charpak, X Gu, TD Frazer, EH Anderson, W Chao, RW Falcone, R Yang, MM Murnane, HC Kapteyn, and D Na>2331_word_end2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end

9. S Eich, A Stange, AV Carr, J Urbancic, T Popmintchev, M Wiesenmayer, K Jansen, A Ruffing, S Jakobs, T Rohwer, S Hellmann, C Chen, P Matyba, L Kipp, K Rossnagel, M Bauer, MM Murnane, HC Kapteyn, S Ma>2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end< optimized high-harmonic pulses using frequency-doubled Ti:Sapphire lasers," Journal of Electron >1798_wo>2331_word_end<_end< and Related Phenomena 195, 231-236 (2014). dx.doi.org/10.1016/j.elspec.2014.04.013.

10. D Popmintchev, C Hernandez-Garcia, F Dollar, C Mancuso, JA Perez-Hernandez, M-C Chen, A Hankla, X Gao, B Shim, >626_wo>2331_word_end<_end< Gaeta, M Tarazkar, DA Romanov, RJ Levis, JA Gaffney, M Foo>2331_word_end<, SB Libby, A JaronBecker, A Becker, L Plaja, MM Murnane, HC Kapteyn, and T Popmintchev, "Ultraviolet surprise: Efficient soft x-ray high-harmonic generation in multiply ionized plasmas," Science 350(6265), 1225- 1231 (2015). 

11. T Popmintchev, M-C Chen, D Popmintchev, P Arpin, S Brown, S Ališauskas, G Andriukaitis, T Balčiunas, OD Mü cke, A Pugzlys, A Baltuška, B Shim, SE Schrau>2329_wo>2331_word_end<_end<, A Gaeta, C Hernández-García, L Plaja, A Becker, A Jaron-Becker, MM Murnane, and HC Kapteyn, "Bright Coherent Ultrahigh Harmonics in >2329_wo>2331_word_end<_end797_wo>2331_word_end<_end<," Science 336(6086), 1287-1291 (2012). dx.doi.org/10.1126/science.1218497.

12. JL Krause, KJ Schafer, and KC Kulander, ">648_wo>2331_word_end<_end700_wo>2331_word_end<_end<>640_wo>2331_word_end<_end632_wo>2331_word_end<_end<>676_wo>2331_word_end<_end680_wo>2331_word_end<_end674_wo>2331_word_end<_end< A>694_wo>2331_word_end<_end< IONS >654_wo>2331_word_end<_end< THE >648_wo>2331_word_end<_end654_wo>2331_word_end<_end664_wo>2331_word_end<_end<," Physical Review Letters 68(24), 3535-3538 (1992). dx.doi.org/10.1103/PhysRevLett.68.3535.

13. CG Durfee III, A Rundquist, HC Kapteyn, and MM Murnane, "Guided wave me>2329_wo>2331_word_end<_end

14. T Popmintchev, D Popmintchev, MM Murnane, and H Kapteyn, "Me>2329_wo>2331_word_end<_end2102_wo>2331_word_end<_end< VUV, EUV, and x-ray light using VUV-UV-VIS lasers," US Patent #61/873,794 (Notice of Allowance, 2015).

15. TV Popmintchev, DV Popmintchev, MM Murnane, and HC Kapteyn, "Generation of VUV, EUV, and Xray Light Using VUV-UV-VIS >797_wo>2331_word_end<_end<," (Google Patents, 2017).

16. KMLabs, ">2267_wo>2331_word_end<_end<™ Coherent EUV and Soft X-Ray Source" (2017), retrieved 11/12/2017, https://kmlabs.com/product/xuus/.

 

 

Appendix A: EUV flux measurement me>2329_wo>2331_word_end<_end

To accurately measure HHG flux, KMLabs used >2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end2329_wo>2331_word_end<_endall background light from impinging on >2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end< at >2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end< of 800 nm, and at harmonic waveleng>2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end< >2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end2331_word_end

 

2329_wo>2331_word_end<_end
2102_wo>2331_word_end<_end2102_wo>2331_word_end<_end<-euv-at-25-50-nm-using->2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end<->2329_wo>2331_word_end<_end2102_wo>2331_word_end<_end<-astrella/xuus-configuration-for-euv.jpg" alt="Figure 5"/>

Figure 5: Modular beamline configuration used for >2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end716_wo>2331_word_end<_end2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end2331_word_end2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end

 

In >2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end< >2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end< flux measurements determined using >2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end2257_wo>2331_word_end<_end<, >2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end

Two filters are used to avoid any 800 nm leakage >2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end< time due to oxidation, a series of >2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end< >2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end< >2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end

 

2331_word_end

Element

Throughput at 35 우리카지노 바카라사이트

VBS (2X), IR EUV beam separator module, to absorb 800 우리카지노 바카라사이트 while reflecting EUV.

~70% each

Aluminum filters (2X), 1000 nm and 200 nm >2329_wo>2331_word_end<_end2331_word_end

1.8% (1000 우리카지노 바카라사이트) 20% (200 우리카지노 바카라사이트)

A toroidal refoc우리카지노 바카라사이트 mirror

~70%

Diffraction grating (+1 o>2331_word_end

~16%

Total beamline >2329_wo>2331_word_end<_end

0.02%

Total beamline >2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end

5.5%

Table 3: Beamline configuration and >2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end

 

2331_word_end

Element

Throughput at 13.5 우리카지노 바카라사이트

VBS (2X)

~70% each

Zir우리카지노 바카라사이트nium filters (2X)

18% (200 우리카지노 바카라사이트)

16% (200 우리카지노 바카라사이트)

Toroidal refoc우리카지노 바카라사이트 mirror

~70%

Diffraction grating (+1 o>2331_word_end

~28%

Total beamline >2329_wo>2331_word_end<_end

0.28%

Total beamline >2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end

10%

Table 4: Beamline configuration and >2329_wo>2331_word_end<_end2329_wo>2331_word_end<_end

 

Schedule a no-우리카지노 바카라사이트st 우리카지노 바카라사이트nsultation to discuss your needs.