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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.
B. Zurro, A. Baciero, D. Rapisarda, V. Tribaldos, TJ-II Team
Fusion Science and Technology | Volume 50 | Number 3 | October 2006 | Pages 419-427
Technical Paper | Stellarators | doi.org/10.13182/FST06-A1264
Articles are hosted by Taylor and Francis Online.
The poloidal rotation of C V ions has been deduced, in the TJ-II stellarator, from spectral line shifts measured using a high-spectral-resolution spectrometer and a nine-fiber-channel system. Analysis of the data obtained has shown that a change of sign of the poloidal rotation direction occurs that depends abruptly on plasma density but is independent of the heating method. Whereas in low-density plasmas the poloidal direction corresponds to a positive radial electric field, at higher densities negative radial electric fields are deduced from the measured poloidal rotation. These measurements are in qualitative agreement with neoclassical theory calculations that predict a change in the sign of the radial electric field mainly because of a change in the ratio of the electron-to-ion temperature.