FPD Meeting Agenda - PowerPoint PPT Presentation

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FPD Meeting Agenda

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9/25 to 10/7 Detector repairs cable tests ... Tom Fitzpatrick (FPD/DFE Interface/DFE Timing) Brian Cox, Dave Mercer, Scott Kolya (LM) ... – PowerPoint PPT presentation

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Title: FPD Meeting Agenda


1
FPD Meeting Agenda
  • 1) Introduction, Shutdown, Trigger 20 Andrew
  • 2) Grounding Issues 15
    Duncan
  • 3) Software Update 10
    Gilvan
  • 4) DQ statusplans
    5 Marcia
  • 5) Data analysis/mc update 10
    Duncan
  • 6) data samples update 10
    Mike
  • 7) automatic insertion?
  • AOB

2
2004 Issues
  • Data taking with integrated Phase II
  • Obtaining new elastic data sample
  • LMTrigger Commissioning/FPD triggers in global
    list
  • Automatic pot insertion
  • Halo/background reduction and modelling
  • Detector studies, alignment, resolution, cross
    talk, efficiency
  • Tracking alignment, acceptance, database,
    efficiency, lattice uncertainty, MC
  • Data handling and quality
  • L2L3 Trigger
  • Physics
    Goals
  • Published results on dN/dT and Z
  • Preliminary results on several physics topics
    including double pom

3
Primary Shutdown Work
  • Repair P2I and A2O (light leak?)
  • Investigate A1O first step in problems
  • A1 muxspare mux tests (A1OA1D motors coupled)
  • Camera repairs
  • Investigate any cabling/mapping problems
  • Replace veto counters and veto PMT'ssurvey
  • Survey before and after separator changes
  • Trigger Commissioning
  • Automatic Pot Insertion
  • Ground searchesrepairs

4
Shutdown Schedule
  • up to 9/20 Grounding Issues
  • 9/24 A20,P2I,P1D removed
  • 9/25 veto scintillator arrives, to be machined by
    Phyillis
  • 9/25 to 10/7 Detector repairscable tests
  • 10/5-10/19 Helio does Mux work, motor adjustment,
    castle maintenance
  • supervises separator work
  • 10/7-10/8 FPD survey
  • 10/11 Seperator work begins
  • 10/25 PMTs arrive need to be tested
  • 11/11 Veto counters reinstalled
  • Trigger/LM Commissioning throughout
  • Automatic Pot Insertion throughout

5
Shutdown Issues/Duncan
  • Supervise cable tests
  • Cable tester tool needed, also accessing TPP
    signals
  • Backplane stabilization
  • Cu link repairs/ optical DFE/TM tests
  • 3 operational DFEs
  • AFE cable replugging
  • Sequencer tests
  • Keep eye on veto counters
  • Grounding issues
  • Trigger

6
Shutdown Issues
  • Andrew
  • Veto counter partssupervision
  • VME scalars/Elgar
  • Trigger progress
  • PMT testing facility
  • UTA control boxes
  • Mike
  • Detector removal, repairs, reinstallation
  • P2I to A1O
  • A2 HV
  • Light leak training
  • LMBs???

7
FPD DAQ and Trigger
8
Trigger Team
  • Andrew Brandt (Trigger Logic/List/Oversight)
  • Duncan Brown (Trigger Implementation)
  • Mario Vaz (FPD DFE equations/TM firmware)
  • Wagner Carvalho (DFE equations/test vectors)
  • Ricardo Ramirez (FPD/DFE Interface)
  • Tom Fitzpatrick (FPD/DFE Interface/DFE Timing)
  • Brian Cox, Dave Mercer, Scott Kolya (LM)
  • Carlos Avila, Luis Mendoza (Stand-alone trigger)

9
2004 Trigger Strategy
  • Input information
  • Currently no global run trigger capability
  • Vertex board is delayed (may now be finished
    during shutdown)
  • DFE boards and TM work and ready to be
    commissioned
  • Main background not from pileup (multiple
    interactions) but from halo spray
  • Strategy
  • Instead of calculating bin of ? and t, use fiber
    hit patterns to demand 2 or 3 out
  • of 3 planes of each detector are hit.
    Replaces trigger scintillator, simpler algo
  • Use multiplicity cut to reject halo spray, code
    several multiplicity levels
  • NOTE fiber ADC threshold must be high enough to
    avoid noise, low enough
  • to retain efficiency and allow vetoing
    of halo
  • One advantage is pot positions not needed at
    trigger level
  • Issues
  • Setting ADC threshold, need special run (and
    analysis)
  • Dealing with noisy channels, variable means,
    could initially set threshold high,
  • later load in mean pattern, known hot
    channels
  • Measure efficiency with jet triggers, scint
    triggers from special runs
  • Exposure groups, triggers in global run or
    separate global run

10
Exposure Groups etc.
  • For normalization purposes each trigger is
    assigned an exposure group
  • and live time is measured for that
    groupdifferent beam conditions require
  • different groups
  • Only 8 exposure groups (6 used), we have more
    combos so must
  • operate outside exposure groupsnew value
    NOLUM
  • Another issue is dynamic downloading, which
    allows multiple global runs
  • This would allow us to take elastic or other
    monitoring data in separate
  • global run, so as to avoid general reco
    streaming and other issues with this
  • Once FPD DFE/TM is ready we are mostly restricted
    to dedicated special
  • runs until these other issues are resolved

11
Interim Plan
  • Proceed with DFE/TM debugging during shutdown
  • Elizabeth indicates NOLUM work will start in 2
    monthstake
  • 2-4 weeks to complete
  • Since current FPD commissioning is special run
    intensive and
  • new elastic triggers with adjacent
    spectrometer veto have rates
  • around 1 Hz, we propose adding an elastic
    trigger to global list in
  • V13.x.
  • If we do this carefully it will only take one
    exposure group and allow
  • us to obtain good elastic sample at lums
    lt40E30

12
Trigger Progress
  • DFE/TM chain tested by Duncan with help from
    Jamieson and Jeff Temple, works with debugging
    Johnson counter firmware. Two of three DFE boards
    work, 3rd needs attention from Jamieson. Two
    DFE-to-TM Cables also need to be repaired during
    shutdown. Will eventually be replaced by optical
    links (should happen during shutdown).
  • Two versions of DFE firmware developed by Mario.
  • Version 3 1 spectrometer only (U5 chip),
    passes fine segment (2/3 and 3/3) and wide
    segment
  • info to TM. This version was simulated,
    implemented, and tested successfully at combined
    test
  • stand but failed at platform
  • Version 4 3 spectrometers on one DFE,
    includes some extra bits to simplify TM
  • algorithms. This version failed some
    timing tests upon implementation and needs
    further
  • development
  • V3 failures traced to delays between different
    inputs to DFE, Tom is working on solution similar
    to TM, which waits for all inputs before
    processing, in parallel Mario working on V4
    firmware.
  • 4. Ricardo is working on arbiter, which is
    necessary for V4 firmware it adds outputs from 3
    spectrometers to form 96 bit DFE word sent to TM.
    He has produced a 3-chip testbench to
  • simulate full DFE
  • 5. Jeff produced first version of TM firmware
    to operate with V3, Mario has version to operate
    with V4 (not yet implemented.)

13
V3 Trigger Manager (debugging)
  • The logic sets the output triggers named
    fpd255..0.
  • Triggers fpd255..101 are set to ground
  • Trigger fpd0 is set to VCC
  • Triggers fpd96..1 are set to the input signals
    A95..0
  • fpd100..97 are set according to conditions on
    va1, and va2,
  • which are defined as inputs A30..28 and
    A26..24, according to the
  • mapping we got from Ricardo.
  • The triggers are (va1uvx in detector 1)
  • fpd97 -- Tight trigger va1va21
  • fpd98 -- Loose trigger va1gt0, va2gt0
  • fpd99 -- Medium trigger 0ltva1lt5, 0ltva2lt5
  • fpd100 -- Dead trigger va1va20

14
V4 TM Algorithm
DFE will pass word for each spectrometer
indicating coincidence of two detectors tight
track exactly 1 hit with 3/3 fine segments in
each detector medium gt0 with 2/3 lt20 wide
segement loose gt 0 with 2/3 lt20 wide
segement At TM we would form terms DIFFany
spectrometer track DIFFQany quadrupole
spectrometer track (could be false if gt1 or 2 on
A or P side) DIFFDdipole track ELASAU-PD or
AD-PU or AI-PO or AO-PI DPOMAU-(PU or PI or PO)
or AD-(PD or PI or PO) or AI-(PU or PI or PD) or
AO-(PU or PD or PO)DI -(PU or PD
or PO or PI) OVERAU-DI or AD-DI or AO-DI or
AI-DI (over-constrained track for alignment)
15
FPD Trigger List
Tentative L1 FPD trigger list (V14?) 1)
elastic (diag opposite spectrometers) GAPSN 2)
soft diffraction (single spectrometers)GAPS or
GAPN 3) overconstrained track (pbar in quadrupole
dipole spectrometers)GAPN 4) double pom (up-up,
dn-dn etc.)GAPSN if needed 5) CJT(2,3) FPD
Track (DIFFQ or DIFFD) GAPS or GAPN if needed 6)
CEM(1,3)? FPD track GAP? 7) TTK(1,?) FPD track
GAP? 8) MU(1,x) FPD track GAP? Monitors may
be necessary, will need to study with
special runs. Also rates are unknown. If 4
(dpom) it is not low enough to run unprescaled we
would need to repeat 5-8 with two FPD
tracks. Possibly 1-3any monitors are best done
in a separate global run since they will not need
general farm reconstruction.
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