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What’s the most difficult question you’ve been asked as a maintenance instructor?
Blye Widmar
"Where are the prints?!"
This was the final question in an onslaught of verbal feedback, comments, and critiques I received from my students back in 2019. I had two years of instructor experience and was teaching a class that had been meticulously rehearsed in preparation for an accreditation visit. I knew the training material well and transferred that knowledge effectively enough for all the students to pass the class. As we wrapped up, I asked the students how they felt about my first big system-level class, and they did not hold back.
“Why was the exam from memory when we don’t work from memory in the plant?” “Why didn’t we refer to the vendor documents?” “Why didn’t we practice more on the mock-up?” And so on.
J. L. Terry, B. LaBombard, B. Lipschultz, M. J. Greenwald, J. E. Rice, S. J. Zweben
Fusion Science and Technology | Volume 51 | Number 3 | April 2007 | Pages 342-356
Technical Paper | Alcator C-Mod Tokamak | doi.org/10.13182/FST07-A1426
Articles are hosted by Taylor and Francis Online.
Research on the scrape-off layer (SOL) plasma of the Alcator C-Mod Tokamak is reviewed. The research has focused on understanding the transport of energy and particles both parallel and perpendicular to the magnetic field. Large differences between the inboard, high-field side SOL and the outboard, low-field side are found. On the outboard side large levels of anomalous cross-field transport of heat and particles exist, with important and far-reaching consequences on recycling, power handling, plasma flows, and possibly core-plasma density limits and rotation. The phenomenon of main chamber recycling is discussed. Parallel and perpendicular transport, together with the heat and particle sources, determine the plasma profiles in the SOL, and these profiles show qualitative differences between near- and far-SOL regions. Particle transport in the near SOL exhibits a strong scaling with collisionality, while transport in the far SOL is clearly convective, with little obvious dependence on collisionality. The anomalously large magnitudes of perpendicular transport are the result of turbulence. Turbulent structures, "blobs," are largely responsible, and their characteristics have been examined. The turbulent structures are approximately aligned with the field and have k << kperp. Their characteristic size perpendicular to the field is ~1 cm, and their characteristic lifetime is ~1 to 50 s. The turbulent structures move both radially outward and poloidally at speeds up to ~1 km/s. Evidence that this turbulent transport may play an important role in the core-plasma density limit is presented. Much lower levels of turbulence and no blobs are observed in the high-field-side SOL. For single-null magnetic configurations, plasma in the inboard SOL appears to be almost entirely a result of plasma flow along field lines from the low-field side. Strong parallel flows with sensitivity to magnetic topology are found, along with strong evidence for momentum coupling between these SOL flows and core toroidal rotation.