'9 ma' presentation slideshows

Pre- Type II SN Nucleosynthesis (s-process)

Pre- Type II SN Nucleosynthesis (s-process). 21 solar mass star. ratio to solar abundance. Rauscher et al. (2002). Type II SN Nucleosynthesis (r-process). 25 solar mass star. Rauscher et al. (2002). Galactic Composition evolution. Chiappini (2004). Nearby Supernova. Knie et al. (2004).

588 views • 50 slides

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429 views • 29 slides

1 National Taiwan University, Taipei, Taiwan

40 Ar/ 39 Ar and Fission Track constraints on Miocene Tectonics in the Buruanga Peninsula, Panay Island, Central Philippines. Monika Walia 1 , T. F. Yang 1 , T. K. Liu 1 , C. H. Lo 1 , L. S. Teng 1 , W. M. Yuan 2 , Ling Chung 1 , G. P. Yumul 3 , C. B. Dimalanta 4.

404 views • 25 slides

Correlation between Hot Spot Activities and Geomagnetic Paleointensity:

319 views • 18 slides

Simplified Transistor - Transistor Logic (TTL)

Simplified Transistor - Transistor Logic (TTL). Transistor - Transistor Logic (TTL) Simplified form of inverter Two instead of four transistors Two instead of four resistors For low v i input, output v o is high Q 1 is on ( saturation ).

365 views • 16 slides

Modeling Cyclotron Resonances in ECLOUD

Jim Crittenden Cornell Laboratory for Accelerator-Based Sciences and Education CTA09 CesrTA Electron Cloud R&D Program for Linear Collider Damping Rings 25 June 2009. CTA09 Cornell University, 25-26 June 2009. Modeling Cyclotron Resonances in ECLOUD.

145 views • 14 slides

Ryan et al. (1995) Leeman et al. (2004)

Fluid-Mobile Element Constraints on Processes Within Subduction Zones: Applications of Boron Geochemistry to Arc Volcanic Rocks. Curves show mixing between mantle (M) and fluids with high B/Nb but different B isotopic compositions as specified. SSW. d 11 B = +16. Tonga, Izu. d 11 B = +8.

279 views • 7 slides

Scaling of impurity (Ne & Ar) transport in beam heated NSTX H-mode discharges

Scaling of impurity (Ne & Ar) transport in beam heated NSTX H-mode discharges. L. F. Delgado-Aparicio, D. Stutman, K. Tritz, and M. Finkenthal The Johns Hopkins University, The Plasma Spectroscopy Group R. E. Bell, R. Kaita, S. Kaye, B. P. LeBlanc, S. Paul, L. Roquemore and D. Smith

139 views • 6 slides