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Quantifying noise sources in the KSTAR 2014 Thomson Scattering system from the measured variation on electron temperature

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Published 16 March 2016 © 2016 IOP Publishing Ltd and Sissa Medialab srl
, , 17th International Symposium on Laser-Aided Plasma Diagnostics (LAPD17) Citation T.-S. Oh et al 2016 JINST 11 C03036 DOI 10.1088/1748-0221/11/03/C03036

1748-0221/11/03/C03036

Abstract

With the Thomson scattering (TS) system in KSTAR, temporal evolution of electron temperature (Te) is estimated using a weighted look-up table method with fast sampling (1.25 or 2.5 GS/s) digitizers during the 2014 KSTAR campaign. Background noise level is used as a weighting parameter without considering the photon noise due to the absence of information on absolute photon counts detected by the TS system. Estimated electron temperature during a relatively quiescent discharge are scattered, i.e., 15% variation on Te with respect to its mean value. We find that this 15% variation on Te cannot be explained solely by the background noise level which leads us to include photon noise effects in our analysis. Using synthetic data, we have estimated the required photon noise level consistent with the observation and determined the dominant noise source in KSTAR TS system.

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10.1088/1748-0221/11/03/C03036