|
Investigation of the leaky chambers
RPC Prompt Analysis
Data vs MC comparison workshops
Summer Global Runs (2014)
RPC DPG Website and EOS
|
RPC Currents and noise Task ForceRelease Planning and deadlines for Software DevelopmentRPC Upgrade SimulationsRPC Crusade (2008-2012) from Camilo
Change to Multi Threaded CMSSW
RPC Synchronization (Trigger Responsability, not DPG) |
Plot | Legend |
---|---|
Error: (1) can't find cms_upg_o_g_b_ni_grid_160229_small.png at /Main.OldRpcDpgtwiki | CMS Quadrant Figure: DT orange, CSC green, RPC blue, steel darkest grey - for startup scenario (included in MUO-11-001). Figure made by Tim Cox, pdf version available here, figures for post LS1 and Phase-2 upgrades available at the CSC DPG Figures Twiki page. --- Tim.Cox@cernSPAMNOTNOSPAMPLEASE.ch |
Plots | Legends |
---|---|
Error: (1) can't find 2010EffDist.png at /Main.OldRpcDpgtwiki | RPC Barrel Efficiency Distribution Each RPC chamber is divided in 2 or 3 partitions called Rolls. Efficiency Distribution is given per roll. Anna.Colaleo@cernSPAMNOTNOSPAMPLEASE.ch |
Error: (1) can't find 2010RPCSynch.png at /Main.OldRpcDpgtwiki | RPC synchronisation The RPC trigger logic electronics receives data via optical fibers from 1232 Link Boards. Each Link Board transmits hits from up to 96 chamber strips. The plot shows how well chambers hits are synchronized w.r.t. the Level-1 Global Trigger decision (BX=0). Only chamber hits matched to good muon candidates are considered in order to reduce effects of cosmic background, signal afterpulses, etc. The central bin contains 99.8% of all hits. rybinska@cernSPAMNOTNOSPAMPLEASE.ch |
Error: (1) can't find 2010RPCSynch2.png at /Main.OldRpcDpgtwiki | RPC synchronisation The plot shows how many Link Boards of the RPC trigger system are well synchronized w.r.t. the Level-1 Global Trigger decision. For each Link Board the average hits arrival time and its spread are calculated from all input strips and from the time windows of 7 consecutive LHC bunch crossings. 28 out of 1232 Link Boards (2%) have hits time spread above 0.15 BX. Further improvement of the synchronization is possible after collecting more collisions data. rybinska@cernSPAMNOTNOSPAMPLEASE.ch |
Error: (1) can't find 2010RPCSynch3.png at /Main.OldRpcDpgtwiki | RPC synchronisation The RPC trigger delay w.r.t. the Level-1 Global Trigger. The RPC triggers are matched (η, Φ) to a muon trajectory propagated to the reference muon station. The upper limit on RPC pre-triggering probability is about 4·10-5 for the analyzed data sample containing 67k good muon candidates. In this data sample muon triggers were disabled in the Level-1 Global Trigger to avoid possible biases due to early muon triggers. rybinska@cernSPAMNOTNOSPAMPLEASE.ch |
Plots | Legends |
---|---|
Error: (1) can't find BarrelScan2009.png at /Main.OldRpcDpgtwiki | Efficiency and Background Example of one barrel chamber HV scan for noise and efficiency at two different thresholds. |
Error: (1) can't find Eff2009.png at /Main.OldRpcDpgtwiki | Efficiency distribution Efficiency distributions at 9.3 kV for two different thresholds. |
Error: (1) can't find Muography2009.png at /Main.OldRpcDpgtwiki | Muography Efficiency distributions at 9.3 kV for two different thresholds. |
Plots | Legends |
---|---|
Error: (1) can't find RPCTriggerEff2009.png at /Main.OldRpcDpgtwiki | RPC Trigger Efficiency with respect to the DT trigger |
Error: (1) can't find RPCTriggerEffPt2009.png at /Main.OldRpcDpgtwiki | Efficiency vs Pt by taking out the cracks Green plot: obtained taking into account only the central region of the wheels: 200 < ΙZΙ < 300 and 450 < ΙZΙ < 550 and ΙZΙ < 100, And the center of sectors 2 - 6: 25 < Ι Ø Ι < 45 and 55 < Ι ØΙ < 75 and 85 < ΙØΙ <105 and 115 < ΙØ Ι< 135 and 145 < ΙØΙ < 165 |
Error: (1) can't find RPCTriggerEffResiduals2009.png at /Main.OldRpcDpgtwiki | Residuals Difference between the muons reconstructed by the muon system and muons measured by the RPC trigger algorithm (for cosmic rays patterns and LHC collisions patterns) |
Plots | Legends |
---|---|
Error: (1) can't find Noise2008.png at /Main.OldRpcDpgtwiki | Distribution of the number of rolls as a function of the roll average noise at 9.2 kV. Channels exceeding 100 Hz/cm2 are masked and do not contribute to the average noise. |
Plots | Legends |
---|---|
Error: (1) can't find ClusterSize2008.png at /Main.OldRpcDpgtwiki | Cluster size distributions at 9.2 kV for tracks with an angle between ± 20 degrees with respect to the normal to the RPC surface in the plane perpendicular to the strip direction. Left plot: normalized distribution of the cluster size for the RB1in layer. Right plot: relative population of reconstructed clusters with size equal to 1, 2, 3 and more than 3 strips, for each RPC layer. Different layers correspond to different strip pitch as indicated in the x axis label. |
Error: (1) can't find EffDist2008.png at /Main.OldRpcDpgtwiki | Efficiency distribution for the barrel rolls, at 9.2 kV. The tail at lower efficiency values is due to now fixed swapped cables, chambers working in single gap mode and chambers with synchronization problems. |
Error: (1) can't find Current2008.png at /Main.OldRpcDpgtwiki | Distribution of the current drawn by the RPCs at 9.2 kV. Left plot: average over one full day of data taking at the end of the CRAFT period, Right plot: average current s a function of time. Each point is the average current over 4 hours and over all barrel stations. |
Error: (1) can't find Efficiency2008.png at /Main.OldRpcDpgtwiki | Efficiency of an RB1in roll as a function of the x and y coordinates (as defined In the figure) of the extrapolated track impact point. The lower efficiency spots are due to the dead regions induced by spacers on a 10 x 10 cm2 grid. An efficiency reduction is also visible for the y coordinate at about 55 cm, where only a single gap is present. |
Error: (1) can't find Residuals2008.png at /Main.OldRpcDpgtwiki | Residuals distributions at 9.2 kV for tracks with an angle between ± 20 degrees with respect to the normal to the RPC surface in the plane perpendicular to the strip direction. Left plot: normalized distribution of the residuals for the RB1in layer. Right plot: RMS of the distribution of the residuals, for different RPC layers (corresponding to different strip pitches) and for different cluster sizes. |
Error: (1) can't find timing2008.png at /Main.OldRpcDpgtwiki | Typical time distribution (in bunch crossing units of 25 ns) of the data coming from individual RPCs with respect to the CMS global trigger time. The dashed line shows the background caused by the 10 over 1020 Link Boards connect to the most noisy channels. |
Error: (1) can't find AverageClusterSize.png at /Main.OldRpcDpgtwiki | Average cluster size as a function of the absolute value of the tangent of angle alpha defined as the angle between the track direction and the normal to the RPC surface in the plane perpendicular to the strip direction. RB1in at 9.2 kV. |
RE4 upscope documentation and drawings:Known HW problems:RPC Pull Requests to CMSSW:RPC WBMNoise Tool web pageRPC SimulationRE4 in CMSSWRPC Muon Reconstruction studies
RPC Monitor Stream and HLT AlCa contactAccessing dataMisc. CMSSW notes / howto |
RPC root Tree
Old RPC Twiki Page
|