'Toroidal field' presentation slideshows

Piero Martin Consorzio RFX- Associazione Euratom-ENEA sulla fusione, Padova, Italy

Reversed Field Pinch: equilibrium, stability and transport. Piero Martin Consorzio RFX- Associazione Euratom-ENEA sulla fusione, Padova, Italy Department of Physics, University of Padova. Notes for the lecture at the European Ph.D. Course (Garching, 29 September 2008). Note for users.

1.04k views • 83 slides

Experimental RFP results

Experimental RFP results. Emilio Martines Consorzio RFX, Padova, Italy email: emilio.martines@igi.cnr.it. A bit of history Magnetic configuration Discharge formation Dynamo PPCD-OPCD Oscillating Field Current Drive (OFCD) Transport mechanisms Scaling laws. Density limit

705 views • 58 slides

Global MHD Instabilities of the Solar Tachocline

Global MHD Instabilities of the Solar Tachocline. Currently Active Collaborators (alphabetical): Paul Cally (Monash University & HAO) Mausumi Dikpati (HAO) Peter Gilman (HAO) Mark Miesch (HAO) Aimee Norton (HAO) Matthias Rempel (HAO) Past Contributors (alphabetical):

720 views • 56 slides

Experimental RFP results

Experimental RFP results. Emilio Martines Consorzio RFX, Padova, Italy email: emilio.martines@igi.cnr.it. A bit of history Magnetic configuration Discharge formation Dynamo PPCD-OPCD Oscillating Field Current Drive (OFCD) Transport mechanisms Scaling laws. The shell problem

678 views • 56 slides

ENERGY SOURCES

675 views • 44 slides

Dynamos in Astrophysics

Dynamos in Astrophysics. See Chapter 13 of Kulsrud for more details. Some Fundamental Questions. Where do magnetic fields come from? How can seed fields be amplified? How can fields avoid decaying?

1.44k views • 37 slides

Sustained Compact Toroids in MRX

Sustained Compact Toroids in MRX. A First Look At Our Recently Completed Ohmic Campaign. S.P. Gerhardt, M. Yamada, H. Ji M. Inomoto 1 , E. Belova, R. Maqueda 2 Y. Ren, B. McGeehan, & C. Jacobsen. 1: Osaka University 2:Nova Photonics.

486 views • 31 slides

Scientific astrology: planetary effects on solar activity

473 views • 30 slides

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402 views • 28 slides

365 views • 24 slides

Roberto Crupi INFN Lecce & Physics Department, University of Salento - Italy on behalf of the

Muon reconstruction and selection at the last trigger level of the ATLAS experiment. Roberto Crupi INFN Lecce & Physics Department, University of Salento - Italy on behalf of the ATLAS Collaboration. 11 th ICATPP Conference on Astroparticle, Particle, Space Physics, Detectors and

441 views • 24 slides

Fifty Years Of Solar Events

Fifty Years Of Solar Events. NOAO 50 th Anniversary Symposium. The Sun is never still. Conditions change on time scales from 10 -6 to 10 17 seconds, spanning 23 orders of magnitude On the long end, secular evolution of the internal solar structure

412 views • 24 slides

Clumps With Self Contained Magnetic Field And Their Interaction With Shocks

Clumps With Self Contained Magnetic Field And Their Interaction With Shocks. Shule Li, Adam Frank, Eric Blackman University of Rochester, Department of Physics and Astronomy. Rochester, New York 14627 HEDLA 2012, Tallahassee, FL.

287 views • 17 slides

Stellar Activity

Stellar Activity. Chromospheric activity is defined as: The variability of a chromosphere and/or corona Spots (plage and dark spots) Flares Associated with convection, magnetic fields, rotation. The Solar Magnetic Field.

370 views • 16 slides

Progress on UCLA MTOR Film Flow Experiments for ALIST (Nov. 2002- April 2003)

Progress on UCLA MTOR Film Flow Experiments for ALIST (Nov. 2002- April 2003). Presented by Alice Ying M. Abdou, N. Morley, T. Sketchley, J. Burris, M. Narula April 7, 2003 APEX Meeting Grand Canyon, AZ.

281 views • 16 slides

Daily operation report Mar .15-16, 200 3

Daily operation report Mar .15-16, 200 3. G roup II. This file is now available @ Computer: Yangyu (D06), Directory: Headington. Outline. 1, 24-hour Review 2, Plasmas & Systems 3, New Information. This file is now available @ Computer: Yangyu (D06), Directory: Headington.

286 views • 15 slides

Examples of using Langevin equation to solve FP equation

Examples of using Langevin equation to solve FP equation. ASCOT Racetrack for tokamak particles. Ab initio particle loading Fusion alphas (thermonuclear, beam-target, beam-beam) NBI-generated ions Realistic orbit tracing Guiding center (4th order RK, w/ 5th order error check, fast)

236 views • 13 slides

XP 540: Transport of Fast Ions by Fishbones and TAEs

XP 540: Transport of Fast Ions by Fishbones and TAEs. Motivation: Exploit new diagnostic capabilities to achieve a quantitative understanding of fast-ion transport. Experimental Goal: Strong fishbone & TAE instabilities Fast-ion profiles Fluctuation profiles. Why fishbones?.

213 views • 8 slides

Fast ion transport by interaction of multiple modes

Fast ion transport by interaction of multiple modes. E D Fredrickson, N N Gorelenkov, G Fu. Phase space interactions of multiple modes may enhance fast ion losses. Phase-space island overlap of multiple modes leads to big fast ion losses.

158 views • 7 slides

Appplication of Toroidal Field

209 views • 6 slides