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- G.M. Wang, B. Bacha, A. Blednykh, E.B. Blum, W.X. Cheng, J. Choi, L.R. Dalesio, M.A. Davidsaver, J.H. De Long, R.P. Fliller, G. George, W. Guo, K. Ha, H.-C. Hseuh, Y. Hu, W. Louie, M.A. Maggipinto, J. Mead, D. Padrazo, T.V. Shaftan, G. Shen, K. Shroff, O. Singh, Y. Tian, K. Vetter, F.J. Willeke, H. Xu, L. Yang, X. Yang
BNL, Upton, Long Island, New York, USA
- P.B. Cheblakov, A.A. Derbenev, A.I. Erokhin, S.M. Gurov, R.A. Kadyrov, S.E. Karnaev, E.A. Simonov, S.V. Sinyatkin, V.V. Smaluk
BINP SB RAS, Novosibirsk, Russia
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NSLS-II is a state-of-the-art third-generation light source under construction at BNL. As many facilities worldwide, NSLS II uses the EPICS control system to monitor and control all accelerator hardware. CSS is used for simple tasks such as monitoring, display, setting of PVs and browsing the historical data. For more complex accelerator physics applications, a collection of scripts are mainly written in Python. The controls group developed the services, such as channel finder, machine snapshot, data archiving, twiss server, unit conversion etc. This paper will present the tools that we have been using for commissioning.
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