Notes - Synclite Instrumentation/beam physics meeting Wed. Sept 8, 2004 ( I'll start a BD document for this note and future ones from the Inst/beam physics meetings>) Next week - Tune measurements Action Items: 1. A careful calculation of the diffraction contribution is needed. Sasha will do this with Timur Shaftan's code once Sasha gets the code. (Note, SL3 code makes no diffraction correction to sigma**2) 2. Analyze if the body light is better than the edge light for stable operation. 3. Check for the factor of 2 observed by Sasha when he compared to flying wires. (After the meeting Randy and Stephen found that the returned sigma is sqrt(2) larger than the actual sigma. This accounts for the factor of two and also means that Sasha's offset is a factor of 2 too big.) 4. Sasha will repeat his analysis for protons on store 3744 which has a wide range of proton emittances bunch to bunch. 5. It would be very useful if someone(Randy?) would summarize and document the optical calculations made to explain the two peak behavior. This is, I think, equivalent to the suggestion that a simple model be made. Some details: 1. Randy showed some pictures of the spots after the pbar mirror was moved in. He described the two peak phenomenon. He stated that the actual distributions are a convolution of light from the two( maybe three) edges, the body of the full dipole, and possibly reflections. This sparked considerable discussion. There seemed to be some consensus that the two peak behavior is what would be expected. The two peaks are light from the end of the 1/2 dipole and the beginning of the full dipole. 2. Sasha pointed out that the distance scales measured when the orbits are moved now agree with expectation and are the same for p and pbar. 3. Sasha pointed out that the two mirror positions are consistent with light from the edges and light from the body. Body light comes from a small region in the middle of the full dipole. 4. Randy had plots showing the ratio of the pbar intensity as measured by SL and by the SBD for 3 bunches as a function of time, intensity and SL sigma. The ratio depends on the bunch. There is about a 4% change in the ratio for the 12 hours of this store, so things are not crazy. Since sigma and intensity both change smoothly with time in the store, it's hard to get the actual dependence from these plots. 5. Sasha compared the H and V emittances as measured by synclite with those measured by flying wires at the beginning and end of the store for pbars for the 36 bunches. He subtracted from the sigmas an amount such as to make the intercept 0 when plotting synclite versus flying wires emittances. The slopes in all 4 cases are a factor of 2 two large, explained after the meeting by the extra square root of two in the SL3 code. The offsets are the same for H and V, but different for the beginning and end of the store. It was speculated that subtracting from sigma squared would make these the same. The same square root of two also makes these offsets too big. 6. There was a long discussion of the offset, which is probably due to diffraction. A quick estimate by Valeri gave a reasonable value but larger than that quoted by Alan Hahn - remember the square root of 2 error! Sasha said he was corresponding with Timur Shaftan of BNL who has a code to calculate the optics, including diffraction of systems like ours. Timur is doing it for synchrotron light source applications. Once Sasha gets the code he'll do the estimate.