Minutes of the CALCOM analysis meeting April 25, 1997. Agenda: B. Niczyporuk DC time calibration (cont) K. Egiyan Effective speed of light in EC scintillators V. Giourdjian Status of cosmic ray analysis on LAEC Summary: (1) Kim Egiyan presented his conclusions on the effective speed of light measurements using runs triggered on electrons. The method was briefly described in the minutes of the last CALCOM meeting (see web page). After applying time walk corrections he obtains a value of 16.0 +/- 0.4 cm/nsec. When he extracts the combined time resolution for a single EC stack and the related TOF bar the resulting resolution is worse (dT ~ 1.1 ns) than the combined resolution of two EC stacks (~0.85 ns). This shows a much larger than expected contribution from the TOF counter indicating a need for improvements in the TOF calibration. (2) Volker Burkert reminded everybody of the importance of the TOF calibration. This task requires increased attention immediately so that we may fully employ the TOF information for particle id during the upcoming commissioning runs in June - August. Maurik Holtrop from UNH has recently joined this effort. (3) Vartan Giourdjian reported on the status of the cosmic ray data taking and analysis of the large angle em. calorimeters (LAEC). Data a currently taken alternating with the forward EC. The goal is to perform the PMT gain matching with min. ion. signals in the center of the scintillator stacks. The hope is to do this with similar accuracy as it was done in the lab in Italy (O(1-2% rms). Vartan showed that in the retracted position the LAEC is currently in, the trigger arrives late and cuts into the fastest signal from the stacks (nearest to the PMTs) so that not the full stack length can be covered. Next meeting: Due to the CLAS collaboration meeting there will be no CALCOM analysis meeting this week. On Saturday May 3, several brief reports from the CALCOM analysis effort will be presented to the collaboration. The next CALCOM analysis meeting will be on Friday May 9. Volker Burkert -------------------------------------------------------------------------- Individual report: B. Niczyporuk: ============= The data, Run# 781.b01 (85072 triggers, Itorus = 1929A and Iminit = 6000A) has been processed with the SDA. The 13919 tracks (Q=-1) were reconstructed for Theta < 60 degrees. The SDA takes only < 4 ms > to process one trigger. The 11235 electrons were identified by matching the DC tracks with the corresponding hits in SC and EC. The losses of 19% are mainly due to the geometry of EC. The corresponding MC prediction is about 14%. The hits in DC and SC of the identified electons were used to derive the calibration constants (time offsets:) for drift chambers, it is: Cdelay = DL1 - (Dcable)dc + (Dcable)sc [ns] where DL1 - Level1 trigger delay to stop DC tdc (common stop) (Dcable)dc - signal wire cable delay to start DC tdc (Dcable)sc - DC signal wire cable delay to stop SC tdc After corrections: for time of flight (ToF), time of propagation along SC slab, time of propagation along signal wire, and adding the raw tdc for SC hit with the raw tdc for DC hits on the reconstructed tracks (to get rid trigger jitter), the Cdelay has been determined with resolution of < 10 ns. Thus, having the DC filled with the slow gas (velocity about 15 microns/ns), the calibration constant resolution will contribute about 0.02 cm to the distance of closest approach (Dca). For Region 1 the constant "Cdelay" has two values: 1200 ns and 1130 ns. The smaller value of the "Cdelay" corresponds to the following wires: <25 (la 1), <24 (la 2), <24 (la 3), <23 (la 4), <29 (la 7), <28 (la 8), <28 (la 9), <27 (la 10), <27 (la 11), <26 (la 12). Having the calibration constants "Cdelay" the drift times "Td" in a cell has been obtained. From "Td" distributions the functions: Dca = f(Td) for each Superlayer have been derived. It has been found that for Superlayer 3 the shape of Dca = f(Td) funcion does not depend on the strength of magnetic field (slow gas). The Figures (postscript files) are available on request.