Summary 2/25/22
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PARTICIPANTS: Brad Sawatzky, Carlos Munoz-Camacho, Carlos Yero, David Hamilton, Hamlet Mkrtchyan, Vladimir Berdnikov, Tanja Horn, Steve Wood, Paul King, Julie Roche, Rachel Montgomery
ANALYZER DISCUSSION
- A simple Analyzer exists - getting fADC scaler data out shoul be straightforward for initial checkout
- Decoding and getting Analyzer set up requires more work:
- Brad can take care of the Analyzer setup and data written to disk
- Software lead neded for the rest
- Analyzer support for VTP payload
- payload modifications should be straightforward
- fADC --> VTP --> summing and triggers decisions
- Task of the Fast Electronics Group - status: "done"
- needs to get this going in the test setup
- Event unblocking feature
- lots of ideas, but not yet concrete
- needs to be done by Hall C - B. Michaels had initially offered help - Brad will check in with him
- SBS is not using event blocking
- not needed when starting the NPS assembly
- The team
- Coordination: Brad Sawatzky
- Software lead: David Hamilton
- Contributors: Steve Wood, Paul King, ...
DAQ/ELECTRONICS TESTS IN SUMMER 2022
- DAQ will be running and HV will be available
- stack crystals - a few options
- stack 1-2 rows, hook up, and check functionality on scope (diagui)
- stack everything (as was done for DVCS/Hall A) since usually the electronics are bad not the crystal
- Trigger tests
- preload data into fADC to test how VTP is doing
- use LEDs to simulate clusters and check if VTP is doing what it should be doing
- cosmics to sanity check VTP
- For cluster trigger tests a board will be provided by FEG
- NPS readout: ~75% of full readout will be available (256 channels == 1 crate remains in HMS and is not available)
- this only impacts signals
- can still test all channels - just need to move cables from block to block
NPS DETECTOR CHECKOUT
- Discussion of the list prepared by Julie
- DAQ requirements for these tests is low
- one question is the stacking strategy: stack everything and plut into DAQ vs. checking individually with scope
- in DVCS/Hall A everything was stacked - smaller calorimeter, but should be ok for NPS too
- Check gain variation with cosmics
- better with LED as it is faster
- can also check how LY varies with temperature as sanity check
- Time estimate: a few months of debugging assuming all tools are available
- Consider developing remote control features and displays
- for HV remote control need to make sure TOSP in place and hard interlock for the box
OVERVIEW DIAGNOSTIC TOOLS AND HISTOGRAMS FROM COMCAL
- Note: ComCAL has 12 x 12 channels
- Diagnostic controls:
- turn on/off LED, change frequency, change amplitude
- HV GUI: turn on/off channels one-by-one
- Histograms:
- (ONLINE) rate vs. fADC channel (block)
- (ONLINE) fADC count vs. paddle
- (OFFLINE) cosmic event in matrix
- (ONLINE) 2D heat map (density/occupancy plot) for scalers row vs. column
- (ONLINE) EPICS to archive to monitor temperature
- (ONLINE) HV adjustment - response from PMT, fit and plot
- Note that scalers from fADC can run without decoding - other items will depend on decoding
- Detector debugging - how to separate PMT from amplifier malfunction
- in general, the approach (if a dead channel is observed) is the same - access to PMT and board and swap entire assembly
- Cooling strategy on Day 0 and in the hall
- need to watch for condensation - should not get into box
- in ComCal assembly the AC failed for a period of time and resulted in humid conditions
- if there is condensation one strategy could be absorbers, but these might saturate quickly
- in the hall humidity will be controlled
- Action items:
- develop histograms and scaler/scaler displays (David H. and team)
DATA TAKING DURING EXPERIMENTS
- waveform data from 5x5 grouping set around VTP determined cluster --> see page 4 in Brad's talk from 2022 Collaboration Meeting
- HMS trigger is generated in NIM (as is done)
- NPS trigger: VTP generates trigger based on internal logic and sends out NIM signal that will be combined with HMS (as in any third arm)
- HMS also event blocked
- ET
- scaler events
NEXT MEETING: FRIDAY MARCH 10 AT 2PM ET(TBC) AND EVERY TWO WEEKS AFTERWARDS