Attendees :M. Blaskiewicz, D. Davino, A. Fedotov, H. Hahn, Y. Y. Lee, N. Malisky, I. Papaphilippou, S. Tepikian, N. Tsoupas, D. Raparia,G. Parzen
Wie stress the need to finish the Holi lattice as soon as possible.
and measurement of 27CDM30 corrector magnet which were acceptable.
shown that the with increase in number of particles the asymmetry between straight section almost gone. fig 1, fig2 fig 3
He also shown the result for numerical saturation 3d space charge modeling.