Asymmetries in density profiles?

Slides:



Advertisements
Similar presentations
How to check close-to-the-line arrows F E D E R A T I O N I T N E R N A T I O N A L E D E T I R A L ' A R C a b TOP VIEW FRONT VIEW a b c d e c d e.
Advertisements

Beginning to use the language of position. Four children stand in a row. Children discuss who is at the front/first in the row? Who is behind? Who is.
Enabling Technology on Alcator C-Mod Jim Irby MIT-PSFC.
ASIPP Characteristics of edge localized modes in the superconducting tokamak EAST M. Jiang Institute of Plasma Physics Chinese Academy of Sciences The.
NSTX Reflectometer Measurements of RF Waves in the Scrape-off Layer in Front of the HHFW Antenna Array J. B. Wilgen, G. R. Hanson, P. M. Ryan, D. W. Swain.
TORE SUPRA Association EURATOM-CEA Département de Recherches sur la Fusion Contrôlée CEA - CADARACHE Saint-Paul-lez-Durance FRANCE Nonlinear LH Wave.
ELECTRON CYCLOTRON SYSTEM FOR KSTAR US-Korea Workshop Opportunities for Expanded Fusion Science and Technology Collaborations with the KSTAR Project Presented.
LH SOL generated fast particles meeting, Prague, Dec 2004 J. Mailloux JET Programme 2005 Selected issues that could affect LH experiments.
New Experimental Results Obtained using Microwave Reflectometry in HL-2A Tokamak W.W. Xiao1), X.T. Ding1), X.L. Zou2), Z.T. Liu1), Y.D. Gao1), J.Q. Dong1),
WARNING…WARNING… WARNING…WARNING THIS POWER POINT PRESENTATION MAY IMPROVE STUDENT ACHIEVEMENT VIEW AT YOUR OWN RISK!!!! Mean, Mode, Median, Range Mr.
What is your strategy for counting money?
IOS-5.2 Maintaining ICRH Coupling in expected ITER regime Spokes person: M. Goniche M.-L. Mayoral (JET), R. Pinsker (DIII-D), L. Colas (TS), V. Bobkov.
Reference patterns: 3 yagi stack. Bottom 3-yagi stack: 20m: ft 6-el OWA yagis on 48 ft boom.
1 JBW-NSTX 9/10/02 Reflectometer Measurements of the Plasma Edge in front of the HHFW antennas John Wilgen, David Swain, Greg Hanson, Phil Ryan Oak Ridge.
Initial Exploration of HHFW Current Drive on NSTX J. Hosea, M. Bell, S. Bernabei, S. Kaye, B. LeBlanc, J. Menard, M. Ono C.K. Phillips, A. Rosenberg, J.R.
10th ITPA conference, Avila, 7-10 Jan Effects of High Energy Ions Accelerated in front of ICRF Antennas in LHD S. Masuzaki on behalf of the LHD Experimental.
Heating and Current Drive Systems for ARIES-AT T.K. Mau University of California, San Diego ARIES Project Meeting September 18-20, 2000 Princeton Plasma.
Microwave Engineering, 3rd Edition by David M. Pozar Copyright © 2004 John Wiley & Sons Figure 13.1 (p. 634) Photograph of various millimeter wave antennas.
Review Calculate the perimeter.. Review Calculate the perimeter. P = 21(2) + 38(2) P = 118m.
Fyzika tokamaků1: Úvod, opakování1 Tokamak Physics Jan Mlynář 8. Heating and current drive Neutral beam heating and current drive,... to be continued.
D. A. Rasmussen, NCSX Research Forum 2006 Page 1 ECH and Fast Wave Electron Heating Systems for NCSX Tim Bigelow, Dave Rasmussen, Phil Ryan, Mike Cole.
Vacuum Vessel Recent Progress. Horizontal or Vertical Rib? Over-Stressed Spots We get over-stressed spots on the horizontal ribs (Very high stress spots)
1 KIT – Universität des Landes Baden-Württemberg und nationales Forschungszentrum in der Helmholtz-Gemeinschaft Institute for Pulsed Power.
ASIPP Long pulse and high power LHCD plasmas on HT-7 Xu Qiang.
Mean: The AVERAGE values of a set of numbers. The mean is found by ADDING all of the values, then DIVIDING by the number of values in the set of data.
Plasma Facing PFA Antenna Group POLITECNICO DI TORINO 19 Topical Conference on Radio Frequency Power in Plasmas June 1-3, Newport 1 Mitigation of.
MAST V.Shevchenko et al, ISTW 2006, October 2006, Chengdu, China EBW Experiments on MAST V. Shevchenko 1, G. Cunningham 1, A. Gurchenko 2, E. Gusakov.
Finding the Density for layers.  Check out this picture from your book. Which layer has the highest density?  Which layer has the lowest density? 
NSTX HIGH HARMONIC FAST WAVE CALCULATIONS
D. Tskhakaya, LH SOL Generated Fast Particles Meeting IPP.CR, Prague December 16-17, 2004 Quasi-PIC modelling of electron acceleration in front of the.
Work with TSC Yong Guo. Introduction Non-inductive current for NSTX TSC model for EAST Simulation for EAST experiment Voltage second consumption for different.
1 Columbia U Comp-X General Atomics INEL Johns Hopkins U LANL LLNL Lodestar MIT Nova Photonics NYU ORNL PPPL PSI SNL UC Davis UC Irvine UCLA UCSD U Maryland.
HHFW heating experiments in NSTX S. Bernabei, J. Hosea, B. LeBlanc, C. K. Phillips, P. Ryan, D. Swain, J. R. Wilson and the whole NSTX crew. ORNL.
Mean, Median, and Mode Lesson 7-1. Mean The mean of a set of data is the average. Add up all of the data. Divide the sum by the number of data items you.
FINDING THE MEDIAN BY JOEY & BILLY WHAT IS THE MEDIAN? The median is simply the middle number For example: 7,8,9,10,11,12,13, In this situation the median.
5.4 Stored Energy Crashes  Diamagnetic loop shows the plasma energy crashes at low plasma density  ECE signals are in phase with the energy crashes 
XP 514: Thermal Electron Bernstein Wave Conversion to O-Mode at GHz G. Taylor, P. Efthimion, J. Wilgen, J. Caughman Goals for this experiment: –Measure.
1 NSTX Electron Bernstein Wave Emission Measurements Gary Taylor NSTX Results Review September 20-21, 2004.
T. Biewer, Sep. 21 st, 2004 NSTX Results Review of 11 Dependence of Edge Flow on Magnetic Configuration in NSTX T.M. Biewer, R.E. Bell, D. Gates,
Why Study Electromagnetics? Contributors: Allen Taflove Cynthia Furse.
Contextual Marketing Campaigns are placed in topically appropriate situations. For students in the process of researching college, finding financial aid,
What is your strategy for counting money?
Are teacher salaries equitable throughout the state?
Date of download: 10/16/2017 Copyright © ASME. All rights reserved.
Pin-fed back to back pyramidal horn antenna
Low-profile corrugated feeder horn antenna (Bull's Eye)
قراءة القوائم المالية وفـاء شـريف علي. محلل مالي
ICRF Task Force Summary
מדינת ישראל הוועדה לאנרגיה אטומית
Using Cathode Ray Oscilloscopes (CRO’s)
GHz reflectometer to be operated in X-mode
High Bootstrap Fraction Plasmas with ITBs
A cusp field or and end block can greatly increase the density
Lower Ip Long Pulse H+ITB Advanced Scenarios
J.R. Wilson, R.J. Goldston, J.C. Hosea ReNew Theme III Workshop
Commissioning of high power LH operation J. R. Wilson, S. Bernabei, J
Purpose of the ex-p: localization of LH current
FRONT No Solutions Infinite Solutions 1 solution (x, y)
Determining the transport of fast electrons in LHCD regimes
Lower Ip Long Pulse L-mode and H-mode Advanced Scenarios
There is a crab in the bottom left of the aquarium
C. Kessel, PPPL Standard breakdown is done at 5.4 T
Proposal #2: AT scenarios, Rerun 600 and 450 kA discharges with PLH = 1 MW C. Kessel,  PPPL Previous discharges with varying rampups at 600 and 450.
LO – I can use positional language.
Mean.
Near-Field Physics of Lower-Hybrid Wave Coupling to Long-Pulse, High Temperature Plasmas in Tore Supra A dynamic Stark effect measurement performed near.
18 Responses to “How many pets do you have?”
Building pattern  Complete the following tables and write the rule 
Team Members: Paige, Ben, Ellie, and Givonni
L2036H1 grid6 First cut x x x x x x x x x x x x x x x x x x x x x x x
Presentation transcript:

Asymmetries in density profiles? 6 locations: top, middle and bottom of LH launcher (C port, 2009) and top, middle, and bottom of ICRF antenna (J port, 2010) Microwave switches to control which horn to launch waves from (2010) Asymmetries in density profiles?

C D E J C

Plan is to test out a variety of situations and different horn locations for density profile data in front of C,D,E, J ports. Ohmic, LH, ICRF shots, L-mode, H-mode Scan line averaged density, outer gap, ICRF, LH power, different species (H and He) Switch between horn locations within a shot to compare data Test out ICRF, LH coupling, asymmetries Throughout campaign