PPT-NSTX-U 5 Year Plan for Transport and Turbulence

Yang Ren Walter Guttenfelder Gregory W Hammett for the NSTXU Research Team NSTXU PAC33 Meeting PPPL B318 February 1921 2013 NSTXU Supported by Culham Sci Ctr York U Chubu U. Captain Rocky Stone. . Chief Technical Pilot - Surveillance. FPAW - Oct. 24, 2013. Overview. Turbulence information, what do we do with it?. Turbulence information needs. Pilot and dispatcher training. Jim Kneller. NC State University. NOW 2010. The neutrinos we will detect from the next SN in our Galaxy will tell us much about the explosion . and. the neutrino.. The flavour content of the signal changes as it propagates from the proto-neutron star to our detectors here on Earth.. http://turb.seas.ucla.edu/~jkim/sciam/turbulence.html Turbulence ? Why do the skin of sharks have groves ? Related Links But what exactly is turbulence? A few everyday examples may be illuminati University of California at Davis. N.C. Luhmann, Jr.,. R. Barchfeld, C.W. Domier, C.M. Muscatello, M. Sohrabi. NSTX-U Collaborator Research Plan Meetings. April . 25, . 2014. NSTX-U. Supported by . Rebecca . Bertsch. Advisor: Dr. . Sharath. . Girimaji. March 29, 2010. Supported . by: NASA MURI and Hypersonic Center. Outline . Introduction. RDT Linear Analysis of Compressible Turbulence. Method. A. Najmi – University of Maryland. B. . Eliasson. – University of . StrathClyde. X. Shao, G. . Milikh. , S. Sharma, K. Papadopoulos – University of Maryland. Introduction. Observation of DAILs (Descending Artificial Ionized Layers) (Pedersen et al 2009, 2011). local winds. Scales of Atmospheric Motion vs. Lifespan. We’ve already started to investigate some of the synoptic-scale features…. Topics for today’s discussion. Basically here’s our roadmap for the rest of the course.. Nova Photonics, Inc.. Fred M. Levinton,. Howard . Yuh. NSTX-U Collaborator Research Plan Meetings. PPPL . – LSB B318. April / May . 2014. NSTX-U. Supported by . Culham Sci Ctr. York U. Chubu U. Fukui U. CSDMS Annual Meeting 2016: Capturing Climate Change (May 17-19, 2016). Zhen Cheng. 1. (Charlie. ), . Tian-Jian. . Hsu. 1. . (Tom. ), . Julien. Chauchat. 2. ,. . Thibaud. Revil-. Baudard. 3. 1. University of Delaware, Newark, DE, 19716, USA. local winds. Scales of Atmospheric Motion vs. Lifespan. We’ve already started to investigate some of the synoptic-scale features…. Topics for today’s discussion. Basically here’s our roadmap for the rest of the course.. Bas van de . Wiel. , . Ivo. van . Hooijdonk. & Judith . Donda. in collaboration with:. Fred . Bosveld. , Peter Baas, . Arnold . Moene. , Harm . Jonker. , . Jielun. Sun, Herman Clercx, . e.a. .. Overview of NSTX-U Research Program Progress and Plans. NSTX-U PAC 37. PPPL B318. January 26-28, . 2016. Events s. ince . PAC-35. Charge Questions. Mission and Capabilities of NSTX-U. Research Goals and Milestones. 3- Buoyant . Production/Consumption . Production. Term . III is large and positive near the ground, corresponding to a large generation rate of turbulence whenever the . underlying . surface is warmer than the air. this term represents the effects of thermals in the ML. It's with sunny days . . tokamaks. Michael . Barnes. University . of . Oxford. Culham. Centre for Fusion Energy. F. I. Parra, E. G. . Highcock. , A. A. . Schekochihin. , . S. C. Cowley, and C. M. Roach. Objective. Connor et al. (2004).