Divertor & SOL Characterisation with Visible Imaging

Slides:



Advertisements
Similar presentations
Institute for Plasma Physics Rijnhuizen Heat load asymmetries in MAST G. De Temmerman a,b, A. Kirk a, E, Nardon a, P. Tamain a, A. Thornton a a Present.
Advertisements

Progress with PWI activities at UKAEA Fusion GF Counsell, A Kirk, E Delchambre, S Lisgo, M Forrest, M Price, J Dowling, F Lott, B Dudson, A Foster,
Introduction to Plasma-Surface Interactions Lecture 6 Divertors.
ASIPP Characteristics of edge localized modes in the superconducting tokamak EAST M. Jiang Institute of Plasma Physics Chinese Academy of Sciences The.
Institute of Interfacial Process Engineering and Plasma Technology Gas-puff imaging of blob filaments at ASDEX Upgrade TTF Workshop.
1 Edge Electrode Biasing Experiments on NSTX S. Zweben, C. Bush, R. Maqueda, L. Roquemore, R. Marasla M. Bell, J. Boedo, R. Kaita, Y. Ratises, B. Stratton.
ELM Filament Propogation Measurements on MAST A. Kirk a, N. B. Ayed b, B. Dudson c, R. Scannel d (a) UKAEA Culham, (b) University of York, (c) University.
A. Kirk, 20th IAEA Fusion Energy Conference, Vilamoura, Portugal, 2004 The structure of ELMS and the distribution of transient power loads in MAST Presented.
General Properties Absolute visual magnitude M V = 4.83 Central temperature = 15 million 0 K X = 0.73, Y = 0.25, Z = 0.02 Initial abundances: Age: ~ 4.52.
V. A. Soukhanovskii (LLNL) Acknowledgements: J. Abramson, R. E. Bell, A. L. Roquemore, R. Kaita, H. W. Kugel, G. Tchilinguirian, P. Sichta, G. Zimmer (PPPL),
Laser Anemometry P M V Subbarao Professor Mechanical Engineering Department Creation of A Picture of Complex Turbulent Flows…..
Auroral dynamics EISCAT Svalbard Radar: field-aligned beam  complicated spatial structure (
The Sun Astronomy 311 Professor Lee Carkner Lecture 23.
Further Study of Ion Pickup. Turbulent Alfven waves and magnetic field lines Turbulent waves represent enhanced random fluctuations. Fluctuations vitiate.
Physics 202: Introduction to Astronomy – Lecture 13 Carsten Denker Physics Department Center for Solar–Terrestrial Research.
HMI – Synoptic Data Sets HMI Team Meeting Jan. 26, 2005 Stanford, CA.
Chapter 7 The Sun. Solar Prominence – photo by SOHO spacecraft from the Astronomy Picture of the Day site link.
The MOSS Camera on H-1NF Clive Michael John Howard PRL,RSPhysSE,ANU Outline: MOSS (Modulated Optical Solid-State Spectrometer) Camera imaging Results and.
Trilateral Euregio Cluster Simultaneous observation of CD and C 2 in the near UV region in the JET divertor spectral window for the observation of CD and.
A. HerrmannITPA - Toronto /19 Filaments in the SOL and their impact to the first wall EURATOM - IPP Association, Garching, Germany A. Herrmann,
17.4 Sound and Hearing Sound waves are longitudinal waves that travel through a medium. Many behaviors of sound can be explained by using a few properties:
The Sun and the Heliosphere: some basic concepts…
Model prediction of impurity retention in ergodic layer and comparison with edge carbon emission in LHD (Impurity retention in the ergodic layer of LHD)
XP-746: ELM characterization in NSTX R. J. Maqueda Nova Photonics Inc. and the NSTX Research Team ’07 Results Review July 23-24, 2007 PPPL.
Edge Localized Modes propagation and fluctuations in the JET SOL region presented by Bruno Gonçalves EURATOM/IST, Portugal.
18-April-2006XRT Team1 Initial Science Observations Solar-B XRT Ed DeLuca for the XRT Team.
Fast Imaging of Visible Phenomena in NSTX R. J. Maqueda Nova Photonics C. E. Bush ORNL L. Roquemore, K. Williams, S. J. Zweben PPPL 47 th Annual APS-DPP.
V. A. Soukhanovskii NSTX Team XP Review 31 January 2006 Princeton, NJ Supported by Office of Science Divertor heat flux reduction and detachment in lower.
Edge Turbulence Imaging During L-H Transitions in NSTX S.J. Zweben, R.J. Maqueda, T. Munsat, D. P. Stotler, T.M. Biewer, C.E. Bush, B. LeBlanc, R. Maingi,
Display of Motion & Doppler Ultrasound
Flow and Shear behavior in the Edge and Scrape- off Layer in NSTX L-Mode Plasmas Y. Sechrest and T. Munsat University of Colorado at Boulder S. J. Zweben.
Helically Twisted Shocks in the M87 Jet Philip Hardee 1, Andrei Lobanov 2 & Jean Eilek 3 1 The University of Alabama, Tuscaloosa, AL, USA 2 Max-Planck.
D. Carralero et al.17 th ISHW, Princeton, /15 Radial and Parallel Transport Fast Camera Observation on LHD SOL Region D. Carralero 1, M. Shoji 2,
1 Results and analysis of Gas Puff Imaging experiments in NSTX: turbulence, L-H transitions, ELMs and other phenomena R.J. Maqueda Nova Photonics S.J.
Large-Amplitude Electric Fields Associated with Bursty Bulk Flow Braking in the Earth’s Plasma Sheet R. E. Ergun et al., JGR (2014) Speaker: Zhao Duo.
1 Blobs in the divertor region R. J. Maqueda (Nova Photonics) Although some understanding is emerging on the generation and evolution of blobs from the.
N. Fedorczak O-26 PSI 2010 San Diego 1 Nicolas Fedorczak Poloidal mapping of turbulent transport in SOL plasmas. G. Bonhomme,
SOHO-20 “Transient events on the Sun and In the Heliosphere” – August 28, 2008, Ghent SOHO-20 “Transient events on the Sun and In the Heliosphere” – August.
بسمه تعالی Fast Imaging of turbulent plasmas in the GyM device D.Iraji, D.Ricci, G.Granucci, S.Garavaglia, A.Cremona IFP-CNR-Milan 7 th Workshop on Fusion.
CCFE is the fusion research arm of the United Kingdom Atomic Energy Authority Presentation on prioritisation of DIVSOL proposals for M9 Andrew Kirk.
R. A. Pitts et al. 1 (12) IAEA, Chengdu Oct ELM transport in the JET scrape-off layer R. A. Pitts, P. Andrew, G. Arnoux, T.Eich, W. Fundamenski,
A. Vaivads, M. André, S. Buchert, N. Cornilleau-Wehrlin, A. Eriksson, A. Fazakerley, Y. Khotyaintsev, B. Lavraud, C. Mouikis, T. Phan, B. N. Rogers, J.-E.
Coronal loops: new insights from EIS observations G. Del Zanna 1,2, S. Bradshaw 3, 1 MSSL, University College London, UK 2 DAMTP, University of Cambridge,
Edge Two Fluids and Gyrokinetic Continuum Simulations Xueqiao Xu Presented at ITER Fusion Simulation Workshop May 16, 2006, Peking University.
Parallel Correlation of SOL Turbulence S.J. Zweben, F. Scotti, J.W. Ahn, T. Gray, M. Jaworski, S. Kubota, R. Maqueda, N. Mandell, D. Smith, V. Soukhanovskii.
ELM propagation in Low- and High-field-side SOLs on JT-60U Nobuyuki Asakura 1) N.Ohno 2), H.Kawashima 1), H.Miyoshi 3), G.Matsunaga 1), N.Oyama 1), S.Takamura.
Edge Turbulence in High Density Ohmic Plasmas on NSTX K.M. Williams, S.J. Zweben, J. Boedo, R. Maingi, C.E. Bush NSTX XP Presentation Draft 5/25/06.
ELM propagation and fluctuations characteristics in H- and L-mode SOL plasmas on JT-60U Nobuyuki Asakura 1) N.Ohno 2), H.Kawashima 1), H.Miyoshi 3), G.Matsunaga.
Fast response of the divertor plasma and PWI at ELMs in JT-60U 1. Temporal evolutions of electron temperature, density and carbon flux at ELMs (outer divertor)
Radiation divertor experiments in the HL-2A tokamak L.W. Yan, W.Y. Hong, M.X. Wang, J. Cheng, J. Qian, Y.D. Pan, Y. Zhou, W. Li, K.J. Zhao, Z. Cao, Q.W.
Review: Recent Observations on Wave Heating S. Kamio Kwasan and Hida Observatories Kyoto University.
Warm up The wavelength of water waves in a shallow dish is 7.5 cm. The water moves up and down at a rate of 5.6 oscillations per second. a.What is the.
Fast 2-D Tangential Imaging of Edge Turbulence: Neon Mantle (draft XP) R. J. Maqueda, S. J. Zweben, J. Strachan C. Bush, D. Stutman, V. Soukhanovskii Goal:
Landsat Satellite Data. 1 LSOS (1-ha) 9 Intensive Study Areas (1km x 1km) 3 Meso-cell Study Areas (25km x 25km) 1 Small Regional Study Area (1.5 o x 2.5.
High Spatial Resolution Observations of Pores and the Formation of a Rudimentary Penumbra G. Yang, Y.Xu, H.Wangm and C.Denker 2003, ApJ, 597, 1190.
Member of the Helmholtz Association Meike Clever | Institute of Energy Research – Plasma Physics | Association EURATOM – FZJ Graduiertenkolleg 1203 Dynamics.
IP Moving wave sources Moving wave sources.
10 mm is the same as... 1 cm. 20 mm is the same as... 2 cm.
A spherical balloon is being inflated such that its volume increases at a constant rate of 10 cm3 per second. When the radius of the balloon is 5 cm, what.
Sun: General Properties
Stochastic Acceleration in Turbulence:
Features of Divertor Plasmas in W7-AS
LH Generated Hot Spots on the JET Divertor
Secondary divertor heat and particle flux
Visible Doppler Spectrometer for Edge Toroidal Rotation
Stereoscopic Pellet Imaging
The control of exfoliated dust sizes to less than ~1mm is indispensable for steady state discharge operation Fig.3: Traces of exfoliation of carbon-rich.
ITER consequences of JET 13C migration experiments Jim Strachan, PPPL Jan. 7, 2008 Modeled JET 13C migration for last 2 years- EPS 07 and NF paper in prep.
Predicting Scrape-Off Layer profiles and filamentary transport for reactor relevant devices   A statistical framework was developed to interpret and predict.
Martian Sands Scott Rowland TGIF Groundhog day, 2019
Presentation transcript:

Divertor & SOL Characterisation with Visible Imaging Filamentary transport imaged in the MAST divertor using a fast framing camera Filaments observed in the SOL and private flux region Extent of fluctuating regions different in L-mode and H-mode Flow of C2+ ions measured using Doppler coherence imaging Spatial resolution <1cm, flow resolution ~1km/s C2+ ions ~2x faster in outer divertor leg after L-H transition Carbon ions accelerate to deuterium sound speed near target High-speed imaging Coherence imaging of C2+ flows CIII Line Intensity CIII Parallel Flow EX/P4-37