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Optically thin perpendicular electron-cyclotron emission from hot electrons in TMX-U

Journal Article · · Rev. Sci. Instrum.; (United States)
DOI:https://doi.org/10.1063/1.1139204· OSTI ID:5642282
Perpendicular electron-cyclotron emission (PECE) from relativistic (T-italic/sub H-italic/--100--400 keV) hot electrons within the thermal-barrier region of Tandem Mirror Experiment-Upgrade (TMX-U) is detected at 35, 60, 94, and 98 GHz. For the operating regime of TMX-U, these signals are optically thin (tau<<1) and thus proportional to the radial hot-electron line density. A relativistic code is used to calculate the theoretical temperature dependence of the perpendicular emission coefficient, j-italic/sub perpendicular/(..omega.., T-italic/sub H-italic/), for each of the detected frequencies. This dependence has been verified experimentally by x-ray measurements of the hot electron temperature, T-italic/sub H-italic/. The observed qualitative agreement demonstrates that optically thin PECE signals can be used to determine the temporal evolution of T-italic/sub H-italic/. An inability to absolutely calibrate the present PECE waveguide system has prevented quantitative agreement.
Research Organization:
Lawrence Livermore National Laboratory, University of California, P. O. Box 5508, Livermore, California 94550
DOE Contract Number:
W-7405-ENG-48
OSTI ID:
5642282
Journal Information:
Rev. Sci. Instrum.; (United States), Journal Name: Rev. Sci. Instrum.; (United States) Vol. 57:8; ISSN RSINA
Country of Publication:
United States
Language:
English