ࡱ> @ V2jbjbqq ^H#Pl$PD$/LD R : =$8u%1&`hKjKjKjKjKjKjK,M OK&#=$&&K* D ***&   hK*@P@&hK*|*M2 BTDD D<)6(C"DD$/L/LJCP*PDD*Princeton Plasma Physics Laboratory NSTX Experimental ProposalTitle:  FORMTEXT Differentiation between ELM types on NSTX FORMTEXT OP-XP-450Revision: Effective Date: 06/17/04 (Ref. OP-AD-97) Expiration Date: (2 yrs. unless otherwise stipulated)PROPOSAL APPROVALSAuthor: R. Maingi, K. Tritz, E. Fredrickson, C. BushDateATI ET Group Leader: R. MaingiDateRLM - Run Coordinator: S. KayeDateResponsible Division: Experimental Research OperationsChit Review Board (designated by Run Coordinator) MINOR MODIFICATIONS (Approved by Experimental Research Operations) NSTX EXPERIMENTAL PROPOSAL  REF Text27 \h  \* MERGEFORMAT Differentiation between ELM types on NSTX  REF Text28 \h  \* MERGEFORMAT OP-XP-450 1. Overview of planned experiment This experiment has two goals: (1) to collect data on different ELM types with edge diagnostics, and (2) test elements of certain hypotheses regarding type V ELMs. In part I, shots will be repeated while switching the USXR and divertor fast visible camera for 4 different filter combinations, changing the timing of gas puff imaging, and changing the dwell depth of the edge reciprocating probe. In part II, the linkage between type V ELMs and the center stack gas puff will be investigated, as well as the possible link to SOL filaments observed in DIII-D[1]. The latter requires running the divertor Langmuir probes at 0 Volts. 2. Theoretical/ empirical justification Several different ELM regimes have been identified on NSTX, corresponding to identified types from conventional aspect ratio tokamaks. Historically these ELMs have been identified by their size/frequency dependence on heating power, proximity to the power threshold, and the presence or absence of magnetic pre-cursors. At low heating power just above the L-H power threshold, Type III ELMs are typically observed (both at conventional aspect ratio and in NSTX/MAST); these ELMs decrease in frequency with heating power, until the discharge becomes ELM-free. They usually have an intermediate frequency pre-cursor oscillation between 40-100 kHz, and result in a 1-5% drop in plasma stored energy. Type III ELMs are thought to be related to resistive MHD. At sufficient heating power, type I ELMs are observed, which increase in frequency with heating power and cause a 3-10% drop in stored energy. Type I ELMs are thought to be related to ideal MHD. Recently in NSTX, a new ELM type has been identified (ref. 2 see also fig. 1), which occurs over a broad heating power range and can co-exist at least with Type I ELMs. These ELMS have been termed Type V, and they do not require any significant change in shape as required for type II or grassy ELMs. Type V ELMs individually cause no drop in stored energy, but they do apparently increase the edge particle transport. These ELMs have a counter-Ip rotating mode with n=1. They are observed as distinct events in the USXR diagnostic, divertor Da, etc. The experiment has two parts. Part 1 is devoted to repeating representative discharges with type I, III, and V ELMs, while switching filters on diagnostics. The different filter combinations on the USXR (Ti3, Be5, and Be100) will allow a better estimation of the ELM depth and the impact on the core plasma. In addition, the different filters on the divertor fast camera (no filter, Da, CIII) will provide insight into the ELM/MARFE dynamics near the X-point. Also, the GPI timing will be adjusted on these repeat shots to try to catch ELMs at the highest acquisition rates. Finally the fast-probe plunge depth (if available) will be varied to estimate the ELM depth in the SOL. Part II of the experiment is geared to investigating the correlation between type V ELMs and the center stack midplane gas puffer, as well as similarities with DIII-D observations which show current filaments in a narrow region near the strike points. The latter point will be investigated by running the divertor Langmuir probes at fixed voltage (0 volts) and looking for signs of filaments near the time of the ELMs. The former point will be addressed as follows. Several successful discharges with fueling from the center stack shoulder injector and also the early H-mode scenarios have shown an absence of type V ELM activity. Therefore the following questions will be addressed: (1) Is there a fueling rate threshold on the CS midplane injector for type V ELMs? (2) Is the ELM helical perturbation spatially tied to the gas puff location? 3. Experimental run plan Part I: Reproduce discharges with different ELM types and switch diagnostic configurations Restore#112503 (Ip=800 kA, Bt=4.5 kG, PNBI=6 MW) which had type V and several type I ELMs and cycle through diagnostic changes in repeat shots (5 shots) Repeat #112159 (Ip=800 kA, Bt=4.5 kG, PNBI=2 MW, with PF1B) which had type III ELMs and cycle through diagnostic changes in repeat shots (5 shots) Part II: Look at correlation between type V ELMs and center stack midplane puffer, as well as SOL filaments Restore #112506 (Ip=800 kA, Bt=4.5 kG, PNBI=3 MW) which had type V only, and drop fueling rate to look for threshold for type V ELMs. (2-5 shots) Decision point: If minimum fueling rate needed for L-H transition is above the threshold for type V ELMs, then consider (a) using the early H-mode discharges which did not require center stack fueling (#112550), and then add the fueling in small bits until type V ELMs observed, or (b) use the successful shoulder fueling scenarios (#112771) and add center stack in small amount to try to trigger type V ELMs. (2-5 shots, if step 3 unsuccessful) Change q95 from step III in LSN (higher Ip ~ 1 MA, maybe Bt ~ 0.4 T) to see if origin of USXR perturbation moves away from the lower divertor region. (3 shots) Compare ELMs in DN with LSN from step #1, i.e. re-run #112525 (DN), and cycle through filters if desire. (5 shots) 4. Required machine, NBI, RF, CHI and diagnostic capabilities This XP requires an operational NBI system, as well as the capability of generating lower-single null and double-null diverted discharges with the plasma control system. No RF or CHI will be used during this experiment. We require HeGDC between shots of nominally 12-14 minutes. 5. Planned analysis Fast EFITs will be required for the faster ELMs to estimate ELM impact on stored energy, and an inversion of the USXR data will be attempted with the different filter combinations. 6. Planned publication of results The results will be presented at the IAEA meeting and in APS talks. References: [1] H. Takahashi, et. al., Nucl. Fusion at press (2004). [2] R. Maingi, et. al., ELMS and the H-mode pedestal in NSTX, submitted to J. Nucl. Mater. PHYSICS OPERATIONS REQUEST  REF Text27 \h  \* MERGEFORMAT Differentiation between ELM types on NSTX  REF Text28 \h  \* MERGEFORMAT OP-XP-450 Machine conditions (specify ranges as appropriate) ITF (kA):  FORMTEXT 52 Flattop start/stop (s):  FORMTEXT _____/_____ IP (MA):  FORMTEXT 0.8-1.0 Flattop start/stop (s):  FORMTEXT 0.15/0.5 Configuration:  FORMTEXT Lower Single Null/Double null Outer gap (m):  FORMTEXT 5-10cm, Inner gap (m):  FORMTEXT 8-10cm Elongation k:  FORMTEXT 2, Triangularity d:  FORMTEXT 0.5-0.7 Z position (m):  FORMTEXT 0.00 Gas Species:  FORMTEXT D, Injector:  FORMTEXT Inner wall Midplane NBI - Species:  FORMTEXT D, Sources:  FORMTEXT A/B/C, Voltage (kV):  FORMTEXT 90, Duration (s):  FORMTEXT <0.3 sec ICRF Power (MW):  FORMTEXT ____, Phasing:  FORMTEXT      , Duration (s):  FORMTEXT _____ CHI:  FORMTEXT Off Either: List previous shot numbers for setup:  FORMTEXT 112503, 112164 (LSN) Or: Sketch the desired time profiles, including inner and outer gaps, k, d, heating, fuelling, etc. as appropriate. Accurately label the sketch with times and values. DIAGNOSTIC CHECKLIST  REF Text27 \h  \* MERGEFORMAT Differentiation between ELM types on NSTX  REF Text28 \h  \* MERGEFORMAT OP-XP-450 DiagnosticNeedDesireInstructionsBolometer tangential array(Bolometer array - divertor (CHERS(Divertor fast camera(EBW radiometerEdge pressure gauges(Edge rotation spectroscopy(Fast lost ion probes(Filterscopes(FIReTIP(Gas puff imaging(Ha camera - 1D(Infrared cameras(Interferometer - 1 mmLangmuir probe array(Magnetics - Diamagnetism(Magnetics - Flux loops(Magnetics - Locked modes(Magnetics - Pickup coils(Magnetics - Rogowski coils(Magnetics - RWM sensorsMirnov coils high frequency(MSE(Neutral particle analyzer(Neutron measurements(Plasma TV(Reciprocating probe(Reflectometer core(Reflectometer - SOL(SPRED(Thomson scattering(Ultrasoft X-ray arrays(Visible bremsstrahlung det.(Visible spectrometer (VIPS)(X-ray crystal spectrometer - HX-ray crystal spectrometer - VX-ray GEM cameraX-ray pinhole camera(  REF Text28 \h  \* MERGEFORMAT OP-XP-450  PAGE 6 /  NUMPAGES 6 Fig. 1  Illustration of ELM regimes and impact on stored energy in NSTX: (a) Type I in high d, DN; (b) Type III in high d, LSN with PF1B; (c) Type V in high d, LSN without PF1b; and (d) Type V and  giant in high d, LSN without PF1b (d) (b) (c) (a) WMHD [kJ] Da [au] $>?@GHRST}~NRSTuyz{   op¾ɻɻɻmHjbU jU>* 5>*CJCJ6CJ6CJCJ5CJj5CJU 5CJmHj5CJUj5CJUCJ5CJ$5CJ=$?@j[D$P$If]^P`a$$$If`a$3$$IfP4&%4 Pah$Dx$If^`Da$1$$IfP4&%4 Pah$P$If`a$$P$If`a$$?@NSTuz{   PQRSTo tu _½  `    _    !I!J!!!!    7|Pk$PP$If`a$W$$IfP4FN &6 N     4 Pah$P$If]^P`a$$VP$If]^V`a$NSTuz{QQD$$IfP40& 4 Pah$Pd$If]^P`a$$d$If`a$:$$IfP4&%   4 Pah   vi[xx$If^ $xx$Ifa$1$$IfP4&%4 Pah$d$If`a$D$$IfP40& 4 Pah  PQRST{H:$^a$ $&3$$IfP4 &%4 Pah xx$If:$$IfP4&%   4 Pah $PP$Ifa$3$$IfP4& &%4 PahTo tu _rsdh & Fdh$^a$!$a$ $0^`0a$  '(tu  *+58  !+,69^_! 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