Since 18 of December 2019 conferences.iaea.org uses Nucleus credentials. Visit our help pages for information on how to Register and Sign-in using Nucleus.
Oct 13 – 18, 2014
Hotel Park Inn Pribaltiyskaya
Europe/Moscow timezone

Progress toward Commissioning and Plasma Operation in NSTX-U

Oct 17, 2014, 2:00 PM
4h 45m
Green 8-9 (Hotel Park Inn Pribaltiyskaya)

Green 8-9

Hotel Park Inn Pribaltiyskaya

Saint Petersburg, Russian Federation
Poster Poster 8

Speaker

Dr Steven Sabbagh (Columbia University)

Description

The National Spherical Torus Experiment - Upgrade (NSTX-U) is the most powerful spherical torus facility being constructed at PPPL, Princeton USA. The NSTX-U project has entered the last phase of construction, and preparation for plasma operations is now underway. The major mission of NSTX-U is to develop the physics basis for an ST-based Fusion Nuclear Science Facility (FNSF). The ST-based FNSF has the promise of achieving the high neutron fluence needed for reactor component testing with relatively modest tritium consumption. At the same time, the unique operating regimes of NSTX-U can contribute to several important issues in the physics of burning plasmas to optimize the performance of ITER. The NSTX-U program further aims to determine the attractiveness of the compact ST for addressing key research needs on the path toward a fusion demonstration power plant (DEMO). Enabled by key technology innovations, the upgrade will nearly double the toroidal magnetic field BT, plasma current Ip, and NBI heating power compared to NSTX, and increase the TF flat top pulse length from 1 s to 6.5 s. The new center stack will provide BT = 1 Tesla (T) at a major radius of R0 = 0.93 m compared to 0.55 T at R0 = 0.85 m in NSTX, and will enable a plasma current Ip of up to 2 mega-Amp (MA) for 5 sec compared to the 1 MA for 1 sec in NSTX. The anticipated plasma performance enhancement is a quadrupling of the plasma stored energy and at least doubling of the plasma confinement time, which would result in an order of magnitude increase in the fusion performance parameter nτT. With BetaT ~ 25% at BT = 1T, the absolute average plasma pressure in NSTX-U could become comparable to that of present-day tokamaks. A much more tangential 2nd NBI system, with 2-3 times higher current drive efficiency compared to the 1st NBI system, is installed. NSTX-U is designed to attain the 100% non-inductive operation needed for a compact FNSF design. With higher fields and heating powers, the NSTX-U plasma collisionality will be reduced by a factor of 3-6 to help explore the trend in transport towards the low collisionality FNSF regime. If the favorable trends observed on NSTX holds at low collisionality, high fusion neutron fluences could be achievable in very compact ST devices. NSTX-U first plasma is planned for November 2014, at which time the transition to plasma operation will occur.
Country or International Organisation USA
Paper Number FIP/P8-30

Primary author

Dr Masayuki Ono (PPPL/Princeton University)

Co-authors

Dr Ahmed Diallo (PPPL) Mr Alfred von Halle (PPPL/Princeton University) Dr Ali Zolfaghari (PPPL/Princeton University) Dr Benoit LeBlanc (PPPL/Princeton University) Dr Brently Stratten (PPPL/Princeton University) Mr Charles Neumeyer (PPPL/Princeton University) Mr Chrzanowski James (PPPL/Princeton University) Dr David Gates (PPPL) Mr Dudek Lawrence (PPPL/Princeton University) Mr Erik Perry (PPPL/Princeton University) Dr Gary Taylor (PPPL/Princeton University) Mr George Labik (PPPL/Princeton University) Mr Hans Schneider (PPPL/Princeton University) Dr Joel Hosea (PPPL/Princeton University) Mr John Lawon (PPPL/Princeton University) Dr Jonathan Menard (Princeton Plasma Physics Laboratory) Mr Keith Erickson (PPPL/Princeton University) Ms Kelsey Tresemer (PPPL/Princeton University) Mr Lane Roquemore (PPPL/Princeton University) Mr Mark Cropper (PPPL/Princeton University) Mr Mark Smith (PPPL/Princeton University) Mr Mike Williams (PPPL/Princeton University) Mr Newat Atnafu (PPPL/Princeton University) Mr Peter Titus (PPPL/Princeton University) Mr Philip Heitzenroeder (PPPL/Princeton University) Dr Rajesh Maingi (Oak Ridge National Laboratory) Mr Raki Ramakrishnan (PPPL/Princeton University) Mr Robert Ellis (PPPL/Princeton University) Dr Robert Kaita (PPPL Princeton University) Dr Roger Raman (University of Washington) Mr Ronald Hatcher (PPPL/Princeton University) Dr Stanley Kaye (Princeton Plasma Physics Laboratory, Princeton University, Princeton NJ, 08543 USA) Dr Stefan Gerhardt (Princeton Plasma Physics Laboratory) Mr Stephan Jurczynski (PPPL/Princeton University) Mr Steve Raftopoulos (PPPL/Princeton University) Dr Steven Sabbagh (Columbia University) Mr Strykowsky Ronald (PPPL/Princeton University) Mr Timothy Stevenson (PPPL/Princeton University) Dr Vsevolod Soukhanovskii (Lawrence Livermore National Laboratory) Mr William Blanchard (PPPL/Princeton University)

Presentation materials