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

Conference ·
OSTI ID:6092186
Perpendicular electron-cyclotron emission (PECE) from relativistic (T/sub H/ approx. 100 to 400 keV) hot electrons within the thermal-barrier region of 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 perpendicular(..omega..,T/sub H/), for each of the detected frequencies. This dependence has been verified experimentally by x-ray measurements of the hot electron temperature, T/sub H/. The observed qualitative agreement demonstrates that optically thin PECE signals can be used to determine the temporal evolution of T/sub H/. An inability to absolutely calibrate the present PECE waveguide system has prevented quantitative agreement.
Research Organization:
Lawrence Livermore National Lab., CA (USA); Maryland Univ., Baltimore (USA)
DOE Contract Number:
W-7405-ENG-48
OSTI ID:
6092186
Report Number(s):
UCRL-93882; CONF-860324-11; ON: DE86008027
Country of Publication:
United States
Language:
English