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News and Related Issues. Ted & Kirsten May 27, 2005 TDWG News since last meeting (April 29th) Organization Issues: how to improve communication Future Plans: near term and long term. Many news since April 29th. Operation related Trigger performance related
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News and Related Issues Ted & Kirsten May 27, 2005 TDWG News since last meeting (April 29th) Organization Issues: how to improve communication Future Plans: near term and long term
Many news since April 29th • Operation related • Trigger performance related • Detector and machine related • Trigger software related • Trigger Table changes and tests
News: Operation Related • Fixes to problems related to prescale changes • Rate Limited trigger problem: protection in L2 decision node code (by Daniel W) • ScalerMon DPS algorithm prescaling to 1 prematurely: protection against this and more diagnostic info (by Bill B) • No prescale change in some high lumi runs, caused by unused L2 trigger bits not properly initialized (confuses ScalerMon): protection in Pulsar crate CPU code (by Konstantin A) • L2ctrl node stuck when start a new run, requires reset • due to memory leak in L2ctrl code, fixed (by Daniel W) So far, haven’t seen any problem after all the fixes above …
News: Trigger Performance related • SVT Fast Abort problem fixed in firmware (by Anna Maria) • SVT fast abort re-enabled on May18 • At high luminosity (~120E30), with high-lumi table, the online average L2 latency is about 40 us at the beginning of the run (Pulsar L2 without fast abort) • With fast abort enabled, L2 latency is 37 us (~3 us saving) • With Alpha driving, SVT fast abort doesn’t help. The online average L2 latency is about 48 us at the beginning of the run • Overall, we have about 10 us L2 performance gain at high luminosity. The higher the luminosity, the more performance gain (Pulsar over Alpha) • Allows us to increase L1A rate when new EVB opens up downstream • EVB Upgrade Review on May 19th: operational in July is possible • at luminosity around 125-127E30, L2 rate saturates at ~395 Hz • deadtime is about 10%, mostly due to waitBusy (~1% due to L2) Let’s see how new EVB will perform…and where is the next brick wall
News: Detector and Machine related • Central hadron and plug online LER calibrations update on May 20 • CHA, WHA, PEM and PHA, effective for runs > 198389 • Some CAL related trigger rates have gone up a lot • L1_SUMET90 from 850Hz to 1.7KHz at 50E30; • L1_MET15 from 500Hz to 1KHz at 50E30; • L1_JET10 from 1Khz to 1.3 Khz For details, see main shift e-log entries in the past few days For a summary, see my e-log entry on May 25th, eve shift • Machine performance: new record at 136E30 on May 12 deadtime was 10-20% at very beginning of the run all due to Busy, then had EVB problem. L2A saturated at 400Hz. Short run 197985.
News: Trigger Software • Daniel W (with help from Tom W) have ported all of the post-freeze changes to the Pulsar • Daniel has checked every bit in every event he could find from the Alpha test run 196104 (physics_test_3_02, v7 run), made sure every bit matches between Alpha and Pulsar • He also uncovered a bug in the BMU bit map, fixed it before it is used in real table • Tom took care of the ElectronTau (by Peter W) in database, new version of TriggerDB. For details, see trigger table testing e-log (previous page) • Alpha crate has been converted into a Pulsar crate, for software development of Pulsar Phase II with CERN FILAR PCI cards. • For better performance, and prepare for Stereo XFT upgrade
News: Trigger Tables/tests • JET_CALIB_TEST[4,645,656] test runs taken • Run 197658 and 197659 taken on May 9th, processed on May 11th • Data to calibrate the Calorimeter, details see Trigger Table Testing e-log • See talk at the end of this meeting • PHYSICS_HIGHLUM_3_03[3,655,570]ready • Prescales to J/Psi to mumu, higher XFT threshold on inclusive muon triggers • Aim to keep us alive at luminosity above 135E30 • Yet to see the performance with the recent CAL LERs update • Details is now in Trigger Table e-log • PHYSICS_TEST_3_02[9,656,571] run taken finally • Run 198597 finally taken this morning, request for offline process • Mostly check the L2 code which was ported to Pulsar • With a few fixes such as Z to bbbar • Details see Trigger Table Testing e-log Most of the work done by Kirsten and Veronica
Organization Issues • Had a meeting with spokes and physics group conveners last Friday • To discuss participation of “trigger representatives” from each group • TDWG == trigger dataset working GROUP • This has to be a GROUP effort ! • Need to encourage young people to get deeply involved • One of the best ways to learn how to be a HEP experimentalist • New ideas could still make a big difference in this mature experiment • Without “G”, TDW == Two Do the Work • We have major challenges ahead of us in the coming year • Our system is flexible enough that we know we can handle it • What we need is energetic young people with fresh ideas …
Plans: near and long term • Near Term Plan: stay alive • Come up with trigger table good up to 150 E30 while fully efficient at lower luminosity • When Kirsten comes back, will move all the changes to the high lumi into default table • Then focus on getting all the triggers under testing into physics table • June 10th Meeting: meet new Trigger Reps! show your plan and results, sign off high-lumi to default • Should keep high-lumi table a pure subset of default table; • Come up with standardize tool to handle DPS offline (manpower promised by spokes) • Expand L2 bits from 128 to 192 • Long Term Plan: GrandUnification of the Trigger Table • Many advantages to this … • Possible mostly due to DPS and lumi enable • Feasibility study on going • Will present plan this summer • Prepare to take full advantage of new EVB & SVT upgrade this year • And find out where is the new brick wall… see the rest of talks