Diagnostics Working Group (WG6) Summary Report

National Spherical Torus Experiment

FY98 Research Forum

Princeton Plasma Physics Laboratory

December 3-5, 1997

 

Diagnostic Working Group

Co-chairmen

David Johnson

Princeton Plasma Physics Laboratory

Robin Snider

General Atomics

Attending Members

Jeff Beckstead

InterScience Inc.

Ron Bell

Princeton Plasma Physics Laboratory

Manfred Bitter

Princeton Plasma Physics Laboratory

Norton Bretz

Princeton Plasma Physics Laboratory

Ed Cecil

Colorado School of Mines

Tom Crowley

Rensselaer Polytechnic Institute

Michael Finkenthal

Johns Hopkins University

Bob Kaita

Princeton Plasma Physics Laboratory

Ben LeBlanc

Princeton Plasma Physics Laboratory

Fred Levinton

Fusion Physics and Technology

Ricky Maqueda

Los Alamos National Laboratory

Ernesto Mazzucato

Princeton Plasma Physics Laboratory

Sid Medley

Princeton Plasma Physics Laboratory

Rick Moyer

General Atomics

Hyeon Park

Princeton Plasma Physics Laboratory

Alan Ramsey

Princeton Plasma Physics Laboratory

Charles Skinner

Princeton Plasma Physics Laboratory

Joe Snipes

Massachusetts Institute of Technology

V. Soukhanovski

Johns Hopkins University

Dan Stutman

Johns Hopkins University

 

Introduction

As was the case at the first Research Forum, this second Forum benefited from ample discussion of diagnostic challenges and measurement needs. Each of the Physics Working Groups was charged to give special attention to this area, and to integrate into its research plan a consideration of the availability of the required measurement tools.

In a change from the organization of the first Forum, the second Forum featured a dedicated "Diagnostics Working Group" (WG6), charged with balancing the needs of the overall program and reviewing the plan for the phased implementation of the diagnostic set. A list of those who attended the WG6 discussions appears above.

There were diagnostic presentations by Bob Kaita on the Baseline Diagnostic Set and by David Johnson on the Upgrade Diagnostic Plans at the Joint Plenary Session the first day of the Forum. These presentations summarized the considerable evolution of diagnostic planning for NSTX that has taken place in the last year, due to discussion at the first Forum and subsequent Program Advisory Committee recommendations.

The morning of the second day, the Physics Working Groups (WG1-WG5) met in parallel sessions. These WG’s were asked to consider measurement needs in the morning session and to prepare a summary of measurement needs for another joint session in the early afternoon of the second day. Each WG6 member chose which morning session to attend, to participate in the individual WG discussion of measurement needs. Then after the joint early afternoon session, WG6 met for the first time as a group.

Co-chairman Robin Snider led the group in a discussion of a series of questions aimed at providing feedback to the project on the strategy for implementation of diagnostics. This discussion also considered the measurement needs highlighted in the previous session by the other WG’s. Following this general discussion, specific diagnostic presentations were made on various topics.

On the morning of the third day, Co-chairman David Johnson then summarized the WG6 discussion and listed a number of action items.

This Report will highlight changes in the diagnostics planning since the FY97 Forum, including several diagnostic issues that were prominent in the various discussions at the FY98 Forum. It should be noted that each of the other working groups will have its own comments on measurement needs and even on specific diagnostic priorities in its summary report. While this report will anticipate some of these issues and provide some response, a full integration of these comments will take time.

Summary of Plenary Session Presentations on Diagnostics

Bob Kaita presented plans for the baseline set of diagnostics shown in red in Figure 1, which has changed significantly since the last Forum. A year ago, a single pulse ruby Thomson scattering system and a conventional motional stark effect diagnostic were both in the baseline set. Due largely to discussions at the FY97 Forum last February and concurrence from the NSTX PAC, and OFES, these diagnostics were removed from the baseline set and given special consideration. There were strong recommendations and subsequent support to design and install a multipulse Nd:YAG laser Thomson system. It was also decided to install an existing X-ray PHA to provide early central Te measurements and heavy impurity data. The decision to stress multipulse Thomson scattering was largely due to the fact that the very low toroidal field on NSTX (0.3T at R0) prevents the use of conventional electron cyclotron emission techniques for measuring Te(r,t). The toroidal field is also too low for conventional MSE techniques to perform polarimetry of the motional stark components of the beam-excited D-alpha emission, the technique developed in recent years to derive J(r,t) in tokamaks. For this reason MSE was also removed from the baseline set and J(r,t) diagnostic development was given special consideration as discussed below. Another addition to the baseline set since the last Forum was a neutral particle analyzer, added to give capability for core Ti measurements before charge exchange recombination spectroscopy (CHERS) measurements are available, and to provide fast ion measurements in neutral beam and RF heated plasmas. It is planned to use an existing PPPL analyzer system.

Bob described the availability of port space for the diagnostics and showed the current allocation plan, pointing out that midplane port space for diagnostics is adequate for the baseline set and some upgrades, but that careful planning and future reallocation will be needed to accommodate future upgrades.

Bob then listed the baseline diagnostic techniques and planned capabilities, with particular emphasis on the magnetic diagnostics. He presented the layouts of the flux loops, the segmented loops and the locked mode coils, used for plasma control and equilibrium, as well as the Mirnov coils used for MHD stability measurements.

Bob summarized the philosophy of the baseline diagnostics as those essential for machine operation and for characterization of fundamental discharge parameters. They must be straightforward techniques requiring little or no R&D. Furthermore, to minimize costs, existing equipment is to be reused whenever possible.

David Johnson presented proposals for supplementing the baseline set with other needed diagnostics. A proposed implementation plan for this so-called ‘upgrade set’ is also shown on Fig. 1. As mentioned above, the highest priority diagnostic upgrades are currently the multipulse Thomson scattering system, which is a PPPL project, and a J(R) diagnostic, which is proposed to be a collaborative task.

The design goals for the multipulse Thomson scattering system were described by Dave, along with a schedule aimed at providing partial availability for the FY99 initial NSTX run. A design concept with a backscattering geometry was shown along with proposed placement of the laser and detector hardware.

At the FY97 Research Forum, it was recommended that a dedicated Study Group should meet to discuss ideas for development of an effective J(R) diagnostic. Dave summarized this meeting, held at PPPL in July, which involved about 25 community experts. A number of techniques were considered, and encouragement for continued investigation was given in the areas of Faraday rotation FIR polarimetry, flux surface mapping with soft x-ray imaging, enhanced MSE techniques, heavy ion beam probe, and Fizeau interferometry. The technique with the most promise for yielding results comparable to existing MSE results on tokamaks was MSE polarimetry, enhanced with modifications to reduce line broadening effects, to reduce the passband of the spectral filters, and to increase the photon flux. The Study Group Summary gave a strong endorsement to support these areas of development.

Dave pointed out that similar Study Group meetings are planned in the areas of ‘Fluctuation Diagnostics’ and ‘Divertor Diagnostics.’

The first day’s Plenary Session ended with WG Leaders briefly discussing plans for the parallel sessions scheduled for the second day. Dave Johnson offered the following questions to serve as guidance for the WG6 discussion:

WG6 Discussion of Diagnostic Implementation Strategy

The afternoon of the second day, after WG6 members had participated in WG1-5 morning sessions and listened to WG1-5 Leaders summarize measurement needs, Robin Snider led a discussion guided loosely by the questions listed above. Nearly all of the WG6 members listed above attended this session.

WG6 agreed with several other group’s recommendations that if a reciprocating probe can be installed at low cost, it should be moved to a start-up diagnostic for edge characterization, particularly during RF experiments. There was a discussion of the need for central Ti measurements before the heating beam is available, brought up by WG5. The WG6 conclusion was that the project should study cost/benefit tradeoffs of 1) x-ray crystal spectrometer installation, 2) VIPS modification and 3) NPA capability to provide for such measurements for the initial run. There was considerable discussion of the baseline plans for two x-ray arrays. With care in design, the two x-ray arrays can be configurable to address different needs as research evolves. For example, for low Te to high Te plasma evolution during CHI research, the two arrays can be configured as an USXR array and a SXR array for broad energy coverage for both phases of the discharge. For some information on Te(r,t) for RF deposition studies and other research requiring fast Te information both arrays can be configured as SXR arrays at different toroidal locations, providing toroidal mode number information as well.

Although it was not discussed in the WG6 parallel session, another issue which came up in the plenary session the third day was concern about fringe counting reliability of the baseline 170 Ghz microwave interferometer. Listed in the implementation plan shown in Fig. 1 is a tangential interferometer/polarimeter, which would likely be an FIR system with several midplane chords. It was suggested that the project consider accelerating the implementation of multichord tangential interferometry with a single chord operational for the initial run.

WG6 felt that the right balance exists in the current plan in the phasing of diagnostics after the baseline set, with proper emphasis on core profile diagnostics. Multipulse Thomson scattering should be highest priority, with a J(R) diagnostic a not too distant second.

Triggered by a strong recommendation from WG4 that core fluctuation measurements are a high priority for NSTX and that FIR scattering the best technique, there was considerable discussion of the appropriate priority for implementing such a diagnostic. The consensus of WG6 was that fluctuation diagnostics, including FIR scattering, are at a lower priority than core profile diagnostics, and are not essential "near day one". However, it was recognized that more attention should be given early to this area. (See next question)

To aid in the planning for diagnostics, there is a need for definition of requirements for measurements. It was suggested that a table of measurement needs be created, similar to that used in ITER diagnostic planning, with column headings such as plasma parameter, plasma region, spatial resolution, temporal resolution, and measurement precision. As an example, there were several discussions of enhanced capability in the plasma edge region for profile diagnostics. There is a need to define expectations for edge pedestals to properly specify edge spatial resolution needs in profile diagnostics. (such as MPTS, CHERS,...)

Several WG6 members, who had participated in the July, 1997 J(R) Diagnostic Study Group Meeting, felt that the meeting was a success in defining the challenges and identifying candidate techniques, but that the project (along with OFES) needs to follow-up more aggressively on the resulting recommendations, and more actively nurture hopeful approaches.

Members felt that "Fluctuation Diagnostics" is an appropriate choice for a second Study Group meeting. Many felt that the meeting, tentatively scheduled for the summer of 1998, should be held sooner. FIR scattering, laser-enhanced BES, reflectometry and heavy ion beam probe techniques should be among those considered.

NSTX collaborators as well as PPPL physicists interested in installing diagnostics would benefit from a concise description of the instrumentation and control interface. Following a design review in March, the project is asked to provide this information, would be very useful in writing grant proposals

There was a discussion of urging that the project do it’s best in anticipating future diagnostic needs in the assignment of port allocations. There was also a request to make port information available on web.

Finally, there was a discussion about being pro-active to encourage diagnostic ideas. The project needs to be vigilant enough to spot a good diagnostic idea even though that idea may not have a dedicated, vocal champion. It must also be flexible enough to nurture these ideas.

List of Action Items Identified by WG6

 

Individual Diagnostic Presentations in All Working Group Parallel Sessions

Presenter

Institute

Topic

WG

 

 

 

 

E. Cecil

CSM

Fast Ion Loss Probes

2

S. Medley

PPPL

Fast Ion Physics & Neutral Particle Analysis

2

A. Ramsey

PPPL

Passive Spectroscopy

4

J. Boedo

UCSD

Fast Scanning Probe Arrays

?

F. Levinton

FP&T

MSE Enhancements

1,3

H. Park

PPPL

Tangential Interferometer/ Polarimeter

6

T. Crowley

RPI

Heavy Ion Beam Probe

6

R. Bell

PPPL

CHERS and Poloidal Rotation

4

B. LeBlanc

PPPL

Multipulse Thomson Scattering

6

R. Maqueda

LANL

Fast Camera and IR Camera

1

M. Bitter

PPPL

X-Ray Crystal Spectroscopy

6

C. Skinner

PPPL

LIF Edge Fluctuations

6

D. Stutman

JHU

MLM Soft X-ray Array

6

 

 

 

Figure 1