1 / 4

NSTX

NSTX. Supported by. Developing the Core Physics Scenarios For Next Step STs. Stefan Gerhardt Friday AM Talk at 2011 APS DPP. Columbia U CompX General Atomics FIU INL Johns Hopkins U LANL LLNL Lodestar MIT Nova Photonics New York U ORNL PPPL Princeton U Purdue U SNL

katen
Download Presentation

NSTX

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript


  1. NSTX Supported by Developing the Core Physics Scenarios For Next Step STs Stefan Gerhardt Friday AM Talk at 2011 APS DPP Columbia U CompX General Atomics FIU INL Johns Hopkins U LANL LLNL Lodestar MIT Nova Photonics New York U ORNL PPPL Princeton U Purdue U SNL Think Tank, Inc. UC Davis UC Irvine UCLA UCSD U Colorado U Illinois U Maryland U Rochester U Washington U Wisconsin Culham Sci Ctr U St. Andrews York U Chubu U Fukui U Hiroshima U Hyogo U Kyoto U Kyushu U Kyushu Tokai U NIFS Niigata U U Tokyo JAEA Hebrew U Ioffe Inst RRC Kurchatov Inst TRINITI NFRI KAIST POSTECH ASIPP ENEA, Frascati CEA, Cadarache IPP, Jülich IPP, Garching ASCR, Czech Rep

  2. Outline of Talk (20 slides) • Intro (4 slides) • Describe why STs are (potentially) useful. (1 slide) • The NSTX facility. (1 slide) • Emphasize upgrades in the past 3-4 years that contribute to “advanced” plasmas (routine RMW control, Lithium, improved control). • What is the present “best” performance in NSTX. (2 slides) • Database analysis of operating space, example discharges. • Describe results in three interacting areas (10 slides): • Transport (2 slides) • Lowest order scanlings….effect of Li? • Current drive (4 slides) • Cases that are approximately classical without *AE activity. • Phenomenological modeling of current redistribution with TAE Avalanches. • Achieved non-inductive fractions in NSTX • Stability (4 slides) • Importance of elevated qmin>1 to avoid core kink/tearing • Strong shaping, broad profiles. • RWM control • NSTX-Upgrade Simulations (4 slides) • Describe the methods (1 slide) • Example profiles for 100% non-inductive cases w/ Pinj=12.6 MW, BT=1.0T, including thermal profile and confinement scaling sensitivity. (1 slide) • Compare a broad range of upgrade scenarios to existing NSTX parameters (2 slides) • Separate 100% non-inducive and high-current partial inductive. • Emphasize what is similar (bN, H), and what is better (lower collisionality, elevated qmin) • 2 Themes: • How facility improvements help with scenarios • How physics results support the modeling.

  3. How Recent Facility Improvements Interact to Improve Performance Eliminate ELMs Broaden the Conductivity Profile Reduced PCS Latency Increase k Elevate qmin Avoid core n=1 modes Lower li Lithium Conditioning of PFCs Increase Bootstrap Current Increase Non-Inductive Fraction Improved Electron Confinement n=1 Control RWM & DEFC Increase NBCD Reduce bN Limit Maintain Rotation Increase Projected Fusion Gain Maintain or Increase bN Eliminate Rapidly Growing RWMs

  4. What is needed. • Most of the data is well analyzed. • Could use: • Finish upgrade modeling (SPG work). • Conclusion on the Li vs. no-Li confinement trends. Does collisionality explain everything? Pedestal vs. Core? • NSTX-U modeling assumes that ion transport remains neoclassical. Do we expect this to be true? GTS calculations started? • Elongation scaling of the no-wall limit in NSTX/NSTX-U relevant plasmas. • Conditions for TAE Avalanche onset in H-mode plasmas. • Is it necessary to say anything about disruptions…their frequency or predictability?

More Related