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- J.A. Safranek, S. Allison, P. Bellomo, W.J. Corbett, M. Cornacchia, E. Guerra, R.O. Hettel, D. Keeley, N. Kurita, D.J. Martin, P.A. McIntosh, H. Morales, G.J. Portmann, F.S. Rafael, H. Rarback, J.J. Sebek, T. Straumann, A. Terebilo, J. Wachter, C. Wermelskirchen, M. Widmeyer, R. Yotam
SLAC/SSRL, Menlo Park, California
- M.J. Boland, Y.E. Tan
ASP, Melbourne
- J.M. Byrd, D. Robin, T. Scarvie, C. Steier
LBNL/ALS, Berkeley, California
- M. Böge
PSI, Villigen
- H.-P. Chang, C.-C. Kuo, H.-J. Tsai
NSRRC, Hsinchu
- W. Decking
DESY, Hamburg
- M.G. Fedurin, P. Jines
LSU/CAMD, Baton Rouge, Louisiana
- K. Harkay, V. Sajaev
ANL/APS, Argonne, Illinois
- S. Krinsky, B. Podobedov
BNL/NSLS, Upton, Long Island, New York
- L.S. Nadolski
SOLEIL, Gif-sur-Yvette
- A. Ropert
ESRF, Grenoble
- M. Yoon
POSTECH, Pohang, Kyungbuk
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Starting in April, 2003, the SPEAR2 storage ring was removed and replaced with a new 500 mA, 3 GeV light source, SPEAR3. The SPEAR2 storage ring had been in use for high energy physics, then synchrotron radiation since 1972. Commissioning of SPEAR3 started on December 8, 2003 and synchrotron radiation will be delivered to the first users on March 8, 2004. SPEAR3 commissioning will be reviewed, including discussion of diagnostics, orbit control, optics correction and high current studies.
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