The primary activities at Alcator C-Mod during the second quarter of FY01 were:
assessment and rectification of the J-port antenna problems, improvement of the DNB
and diagnostics, and data analysis of results from the previous run campaign. Plasma
operation resumed on May 23.
Science
Results
Core
Confinement and Transport
with a central field below 4.5 T), and can also develop spontaneously in some Ohmic
H-mode discharges. The formation of the ITB appears in conjunction with a decrease
in the central (impurity) toroidal rotation velocity. The ITB foot is located near
r/a = 0.5, regardless of how the barrier was produced. The ITBs persist for 15 energy
confinement times (tE), but exhibit a continuous increase of the central electron density, up to values near 1x1021/m3 (in the absence of an internal particle source), followed by
collapse of the barrier. This ITB is also evident in the electron and ion temperature profiles, and a drop of the core thermal conductivity, c eff , is confirmed by modeling.
Application of additional on-axis ICRF heating arrests the density and impurity peaking;
this occurs along with an increase (co-current) in the core rotation velocity, and steady
state double barrier plasmas have been maintained for 8 tE or longer, with a current
density bootstrap fraction of 0.13 near the ITB foot. The trigger for the ITB formation is unknown.
Shown in Fig.1 are the time histories of several parameters of interest for a 4.5 T plasma,
which had an EDA H-mode edge pedestal and a core ITB generated by off-axis ICRF
waves. 2 MW of ICRF power at 80 MHz were delivered for the time interval between
0.7 and 1.5 s, as seen by the green curve in the 4th panel of the figure. This deuterium
majority discharge had a hydrogen fraction of 4%. The plasma entered H-mode at 0.76 s,
as evidenced by the drop in the Da signal, and the subsequent rises in the plasma stored
energy, electron density, ion temperature and central toroidal rotation velocity. The EDA
H-mode was well established when around 0.85 s the rotation velocity began to drop in
conjunction with the formation of the ITB, as seen in the continuous rise of the core
electron density.
Fig. 1
The ITB formation may be visualized by examination of the evolution of the electron density profiles:
www.psfc.mit.edu/people/marmar/denmovie2.mpg
By adding a modest amount of on-axis heating power to an ITB discharge, the increase
of the electron density can be stopped and the barrier can be maintained in steady state.
This effect is demonstrated in Fig.1; at 1.25 s additional heating power at 70 MHz was
injected, reaching 600 kW by 1.35 s, as shown in red in the 4th panel. (The total ICRF power is shown in blue.) Not surprisingly, there was an increase in the plasma stored energy and the central ion temperature after this time. Of particular interest is the return
of the co-current toroidal rotation during this interval, along with a halt to the electron density increase. Besides the arrest of the electron density peaking and the increase in the core ion temperature, there are other beneficial effects from the additional on-axis heating, as is demonstrated in Fig.2. Between 1.35 and 1.5 s, the ambient level of central soft x-ray emission was held constant. Note that throughout the ITB phase of this
discharge, sawtooth oscillations were present, and that the sawtooth inversion radius was near R = 0.73 m, well inside of the ITB foot location. Similarly, the additional on-axis heating stemmed the increase of the total radiated power, holding it at a tolerable level of about 50% of the total input power. Likewise, Zeff was maintained at a constant value
of 1.8 during this time. In Fig.2 is also shown the ratio of the central electron density to the value at R=0.83 m, well outside of the ITB foot, reiterating the arrest of the density peaking.
Fig. 2
EDA/QC
Mode
The EDA looks like a promising regime - with good energy confinement, no accumulation of impurities and no giant elms. To extrapolate EDA, we need to understand the physics. The observed QC mode is apparently responsible forEDA; they are always seen together. Probes show a strong particle flux from correlated n and E fluctuations. Deff calculated from density profiles and the measured particle source is roughly proportional to the mode amplitude as measured by PCI. The mode is localized to the outer portion of the density pedestal, apparently quite narrow in radial extent - maybe no more than 1-2 mm.
A large amplitude coherent mode is found in non-linear gyro-fluid simulations [Rogers and Drake, U MD], which shows that turbulence is not inevitable. Linear gyro-kinetic stability calculations using the GS2 code find an unstable mode - tentatively identified as resistive ballooning [Dorland, UT]. Jim Hastie has been working with J. Ramos and F. Porcelli on an analytic theory of RB stability.Initial results agree with parametric
dependences seen in experiments.Xu and Nevins [LLNL] using the BOUT code to simulate the edge (including separatrix) find a coherent mode - identified as a resistive
X-point mode with some similar features to QC mode.They predict a higher frequency mode at 4-6 MHz and reversal of propagation for reversed BT.
Edge/Divertor
Physics
can be much longer (> 5 meters) allowing plasma to ‘fill-in’ the limiter shadow both by transport and by ionization. The importance of these effects will be investigated with further analysis using the KN1D code. As a more direct test of this hypothesis, measurements of the neutral pressure in the shadow of the limiter near the horizontal scanning probe will be performed during the next run campaign using new in-vessel Penning gauges.
Fig. 3
Another important result from the KN1D simulations bears on the role of charge
exchange heat transport in these discharges: charge exchange is clearly a negligible
player relative to the total heat flux crossing the last closed flux surface. In most cases, neutrals contribute to an inward-going heat flux ‘pinch’ across the separatrix. A comparison with the magnitude of cross-field plasma heat convection in the near and far SOL (see Fig. 3) also show that neutrals play only a minor role in the total heat transported across the scrape-off layer. For reference, an estimate of the cross-field heat flux from plasma convection is shown in the top panel ofFig. 3 for a variety of plasma densities. The corresponding heat flux due to atomic hydrogen (computed by KN1D) is shown in the bottom panel. The heat flux from atomic neutrals does not significantly impact the power losses in the SOL. In fact, at high densities, the atomic fluxes contribute and inward-going heat flux ‘pinch’ over much of the SOL.
Recent success in commissioning a 4-strap (J-port) antenna has allowed the maximum injected power to reach 2.5 MW from this antenna.From analysis of the antenna performance, a RF-plasma edge interaction at power levels > 2.5 MW resulted in injections and hot spots on the antenna top and side protection tiles (sometimes on the Faraday screen).These hot spots appeared to be connected on a field line with the longest connection length, typically a corner tile and a side tile.The corresponding side
tile hot spot would change in accordance with the edge plasma q. Furthermore, arc damage was concentrated in areas on the antenna strip line where the E-field was parallel to the ambient B-field.From the typical operation, several arc events were identified with an energy content consistent with the observed melt damage.The empirical electric field was 15-17 kV/cm.This is consistent with an empirical observation made at JET
where 1.5 kV/mm for E parallel to B and > 2.5 kV/mm for E perpendicular to B.
Some images may be seen at:
www.psfc.mit.edu/cmod/operations/EngImages/
RF/ICRF/P0001408.JPG
www.psfc.mit.edu/cmod/operations/EngImages/INVESSEL/2001/
Close_Up_Survey/P0001531.JPG
www.psfc.mit.edu/cmod/operations/EngImages/INVESSEL/2001/
Close_Up_Survey/P0001558.JPG
The antenna has been further modified to reduce the RF-plasma edge interaction.The protection tiles have been moved to the same radius as the other antennas.A BN septum has been installed to interrupt field lines, and all metal surfaces nearest the plasma except for the Faraday screen have been removed or covered . The strip lines have been rotated to make E perpendicular to the ambient B-field and increased the strip line spacing to reduce maximum electric fields. An additional arc detection system based upon the relative phase between antenna strap voltage has been implemented.New magnetic probes to measure the current in the antenna straps have been installed.In addition, new voltage probes and directional couplers have been added.A local pressure measurement and optical monitoring system has been implemented for the strip line region behind the antenna back plane. See:
http://www.psfc.mit.edu/people/irby/
jport_antenna_stripline3a.jpg
Impurity injection laser:
A laser was installed for laser ablation of impurities for transient transport experiments.
The BES optics were repaired and recalibrated during the recent C-Mod opening.One in-vessel mirror, which had become detached, was secured. Redesign of the optical system to provide better damage resistance and to improve the fluctuation resolution was begun.
Beam duct monitors:
Diagnostics were installed in the DNB duct to monitor any reionization effects.These included pressure gauges and H-alpha monitors.These have been used and are working satisfactorily.
Progress on beam conditioning:
The best beam pulses were taken during February.During these pulses, the full energy component was as high as 23% and the water component was negligible.After repairs to the beam cryo system, a brief up-to-air for reconnection to C-Mod, and installation of the
beam duct monitors, the beam is being conditioned with the expectation that it will return to those levels.
CXRS calculations:
A calculation of photon emission cross sections from partial charge exchange was developed so that we can compare the emission cross sections for various sets of state selective charge exchange cross sections (partial cross sections).This will also be useful to investigate the effect of beam excitation as it transits the neutral gas in the beam duct.
The ambient emission due to plasma excitation of the charge exchange transitions was calculated for comparison with the above calculation.
MSE:
Repairs of an invessel mirror restored the MSE/BES view locations to proper alignment.Although initial beam into gas shots did not yield sufficient signal for the necessary MSE calibration, further attempts will be made after the beam drift duct has been properly
conditioned.Initial beam into plasma data was obtained, showing modestly improvements in signal to noise ratios compared to the end of the last run campaign.As the beam conditioning continues, a return to the high full energy component fraction achieved in February will yield better signals for MSE.
Earl Marmar went to a JET collaboration discussion at OFES in Germantown on Feb 26.
Earl Marmar, Ron Parker, and Miklos Porkolab attended the DoE Budget and Planning Meeting March 13 to 15 in Gaithersburg.Earl and Ron gave talks on C-Mod and the LH MIE Project.
Amanda Hubbard gave atalk at California State University of Sacramento on Thursday, 3/15, as part of the APS/DPP Distinguished Lecturers in Plasma Physics series,entitled ‘Understanding and Improving Energy Transport in Fusion Plasmas.’
Jim Irby visited PPPL Mar. 27 for discussions with Douglas Loesser, Randy Wilson, Stefano Bernabei, and Gerd Schilling on the Lower Hybrid Launcher.He also met with Raffi Nazikian and attended a PPPL/MIT proposal review of the reflectometry collaboration.
Miklos Porkolab and Paul Bonoli attended the Annual Sherwood Fusion Theory Conference in Santa Fe, NM, on April 2-4.
Bob Childs was in Brooklyn, NY on Apr. 6 supervising copper plating of the ICRF antenna stripline components.
On April 6, Amanda Hubbard gave the Plasma Physics Colloquium at Columbia University,NYC, entitled ‘Edge transport barrier and fluctuations in Alcator C-Mod’.
John Rice was at the Univ. of Wisconsin on Monday, Apr. 9, and gave a seminar on the latest C-Mod results.
Rejean Boivin was at GA Apr.17 and gave a talk on neutrals.
Miklos Porkolab attended the Tom Stix Memorial Service in Princeton on April 23.
Jim Terry reported at the weekly Physics Meeting on his observations at the April meeting of the APS, which took place April 28 - May 2 in Washington D.C. This event is a general meeting of the APS. Jim presented an Alcator C-Mod overview poster entitled‘Experiments in Plasma Physics and Fusion Science on the Alcator C-Mod Tokamak’.It was one of six other fusion posters at the meeting. There was one invited talk from the fusion community on self-organized criticality in plasma transport. The participation at this meeting was an ‘outreach’ by the fusion community to the rest of the physics community.
Ron Parker, Miklos Porkolab, Joe Snipes, and Spencer Pitcher attended the Burning Plasma Workshop II at General Atomics on May 1-3.Options for a future burning plasma experiment - Ignitor, FIRE, and ITER-FEAT, were discussed.
Martin Greenwald travelled to Washington DC May 7 to attend a meeting of the ESnet Steering Committee where he presented a talk on Office of Science programs and their network requirements to a group of DOE program managers.
Miklos Porkolab and Spencer Pitcher attended the FESAC meeting in Germantown,
MD, on May 15,16. During the Public Comment session Miklos gave a brief presentation on the status of graduate students at the PSFC. He emphasized the healthy status of graduate student enrollment at MIT, and the strong job market for recent Ph.D's graduating in plasma and fusion sciences. Spencer discussed his ‘open letter to
FESAC’ advocating a burning plasma tokamak experiment, during the public
comment session.
Jim Terry, Brian LaBombard, John Rice, Martin Greenwald, Catherine Fiore,
Jerry Hughes, and Valerie Censabella attended the 14th Transport Task Force
(TTF) meeting in Fairbanks, Alaska, May 16-19. LaBombard, Greenwald and Terry
also participated in a Meeting on Plasma Turbulence and Transport in Edge/SOL
regions, also held in Fairbanks on May 14-15, prior to the TTF meeting.
Martin Greenwald travelled to Lausanne Switzerland to participate in the international database meeting held April 2-5.He took the opportunity to meet with Jo Lister, Basil Duval, Richard Pitts and Yves Martin to discuss plans for joint TCV - C-Mod
experiments.
Amanda Hubbard attended the International Workshop on Physics of Internal Transport Barriers, Edge Pedestal, and Steady State Operation in Tokamaks, in Garching, Germany the week of Apr. 28.She gave talks on C-mod pedestal andITB results, and also
made plans for a comparison experiment with ASDEX-Upgrade on Type II elms and EDA modes.
Eric Nelson-Melby traveled to the CRPP-EPFL in Lausanne, Switzerland on May 7
and gave a seminar on C-Mod RF PCI results entitled "Phase Contrast Imaging
of Ion Bernstein Waves in Alcator C-Mod."
Please comment on the progress in installation and initial operation on Alcator C-Mod of the University of Texas Diagnostic Neutral Beam (DNB), giving due consideration to the financial, material and human resources that have been available.
Please comment regarding the difficulties that have been encountered in initial DNB operation, and give every suggestion you can for improving DNB performance.
Please provide your best assessment of the potential ultimate performance of the DNB and the resulting prospects for the desired plasma diagnostic measurements, including current density profile (MSE), ion temperature and rotation profiles (CXRS) and internal fluctuations (BES).
Earl Marmar has assigned responsibility for coordinating DNB and related diagnostic activity to Bob Granetz, implementing a suggestion made by the C-Mod Program Advisory Committee that a senior staff member take on this challenge.
Installation of improved duct diagnositics and addition of shutters to the charge exchange optics have been implemented. The remainder of the recommendations will be addressed during the coming campaign.
Attending the review were:
ORNL:Phil Ryan, Rick Goulding
PPPL:Gerd Schilling, Bob Ellis
GA:Bob Pinsker
MIT:Steve Wukitch, Rejean Boivin, Jim Irby, Peter Titus, Bruce Lipschultz,
Brian Labombard
UTexas:Perry Phillips
There was general agreement on the antenna modifications.There was also strong agreement that phase measurements with fast time response are essential.These measurements have been implemented. Since the modifications require supporting the antenna at the top and bottom from the center of the antenna, a concern was raised about thermally induced stresses. FEA analysis of the antenna performed following the review indicates that these stresses are in fact small.
Several unanswered questions regarding the double transport barrier plasmas
will be addressed: Is this ITB an energy barrier as well? Can the ITB be sustained in steady state? Why is the ITB foot location near r/a = 0.5, regardless of ICRF
resonance location, or whether it is formed in Ohmic plasmas or by pellet injection? Why is there an abrupt threshold (in lowering BT) for the ITB formation by ICRF heating? Does the ITB appear only with the ICRF resonance on the high field side, or is there a power threshold? How is impurity transport affected by the ITB?