Title: Major NSTX Program Topics of Interest, Feb 2004
1Major NSTX Program Topics of Interest, Feb 2004
- NSTX PAC-15th Meeting, Jan 12 14, 2004
- FY04-06 Research Milestones
- FY04 Research Coordination Among DIII-D, C-Mod,
and NSTX (on-going discussion)
2NSTX PAC-15th Meeting
- Three charges
- Due to funding reality, effectiveness of
- Updated plan for 04-08
- 04 run plan
- 05-06 research facility plan (for FWP)
- in addressing the goals of the 5-Year Plan
3NSTX PAC-15th Meeting Results
- PAC was impressed gave many positive comments
- Congratulations on TF repair
- More better analysis, integration scenario
development - Aggressive RWM upgrade and research plans
- Progress toward ?i resolution
- FY04 run planning, and run-week contingency
- Tests of high k, multiple approaches for startup
- Partition into startup (100-150kA), rampup (to
500kA), sustainment (to 1MA) - Exemplary effort in international collaboration
- General approval of facility plan
4NSTX PAC-15th Meeting Results
- Several areas require attention
- Timely availability of MSE CIF data (? begin
quarterly review and update) - Global confinement study, for projection to
future devices - Systematic linear and nonlinear m-turbulence
calculations as part of research, for ion and
electron diffusivities - HHFW modeling benchmarking with experimental
measurements - Schedule for lithium vs. cryo decisions, critical
for future scenarios - Schedule and criteria for EBW frequency MAST
collaboration, 06 decision - Investigation of CTF scenarios
- Coordination of US ST programs
- MW EBW source development schedule and funding
- ? Work on these as part of preparation of FWP
5FY05-06 Research Milestones, Arrived at on Feb
10, 2004, to Address Overarching Fusion
Scientific Issues
FY04
FY06
FY05
Exp. Run-Weeks
18
12
14
1) Transport Turbulence What causes electron
ion transport? (04-2) Measure (05-1) Measure
hi-k low-k turbulence turbulence
2) MHD How are plasma pressure bootstrap
current limited? (05-2) Study plasmas
near with-wall limit
3) Wave-Plasma How do energetic particles RF
power sustain plasmas? (04-3) Measure ?J
(05-3) Demonstrate (06-1) Assess EBW from RF,
NBI ?p JNI 100 for tskin HCD
requirements (04-4) Characterize EBW
emission, est. HCD
4) Start-up How to convert externally directed
energies to plasma magnetic flux? (04-5) Test
current (06-2) Solenoid-free initiation ramp-u
p to high bp
5) Boundary How do plasmas interact with
materials? (06-3) Characterize edge of
H-mode plasmas
6) Integration of ST plasma science into
attractive regimes (04-1) Assess hi tE
(05-4) Assess combined (06-4) Demonstrate hi
bT H-mode for gtgt tE RF NBI effectiveness JNI
100 for gtgt tskin