The HPS Run Wiki

[edit]

• Shift Documentation
• Short Term Schedule
• Long Term Schedule
• Monitoring
• Phone Numbers
• Remote Shifts

Phone Numbers Shift Schedule Shift-Taker's Checklist Hot Checkout Beam Time Accounting Run Spreadsheet 2021 2019,2016, 2015 2019 HPS production triggers descriptions COO, ESAD, RSAD Things to read before shift. Expert shift - refresher video demo Remote worker shift - requirements and responsibilities HPS 2021 Run discription and beam parameter requirements

Procedures Procedure for establishing physics quality beam Commissioning Plans: Trigger ECal SVT Hodoscope Tunnel/Hall Access Power Failure

Manuals Harp Scans Beam Trip Runs SVT ECal (Annex) DAQ Beamline and Beamline Drawings Turning Chicane ON/OFF Chicane Settings Manual Turning Chicane ON/OFF Slow Controls

JLab Logbooks MCC DTM Hall-A Hall-B Hall-C Hall-D

HPS (E12-11-006) 2021 run, August - October'
Beam energy 3.74 GeV
Important: Document all your work in the logbook!
Bluejeans for Run Meetings on DAY and DAY at 3 pm

RC: Stepan Stepanyan

• (757) 575-7540
• 9 575 7540 from Counting Room

PDL: Valery Kubarovsky

• (757) 876-1789
• 9 876-1789 from Counting Room

Important instructions

* Turn OFF beam before target move!

* No access to the alcove if the chicane magnet beacon is ON.

Chicane magnets must be OFF if the hall is in Controlled access and access to the alcove is needed or when the hall is in Restricted access. If Chicane magnets are OFF, they can be energized only when the hall is in Power or Beam Permit, [1].

* TURN OFF the chicane magnet if beam is not available due to a thunderstorm. Loss off power would seriously damage detectors.

* Fill out BTA hourly. Click "Load from EPICS" to fill the left side, then make sure numbers are correct. If needed edit the entry.

NO ABUs or BANU if beam tune is in progress, make it all BNA with ER 100%. At the end of the shift save BTA to the logbook!

* Please close any GUI that is not being used, e.g. close harp scanner after harp scan is done, close chicane, after chicane is ON, etc.

* For orbit lock positions on 2H00(X=0.7,Y=1.1) and on 2H02(X=1.8,Y=0.1). Use the 2.82 mm SVT collimator

am profile check once a day, at 9 am, using 2H02 and SVT wire harps Run Plan September 1 - September 3, 2021 When the machine will be ready use procedurse[2] to establish a physics beam for HPS, see step-by-step instructions on the right. The chicane should be ON when sending the beam to Faraday cup (energize it while tagger magnet is degaussed) - Ask Cameron if he is ready before allowing the beam to the hall . To define the correct trajectory for the beam to FC positions on 2C24A BMP are [3] x=0.699, y=0.719, positions on the harp should be as in [4]. T With MCC Check the correctness of the 2H02 BPM readings (direction notations in X and Y) using the 2H02 harp. On the harp increasing number for the mean values of the peaks in X and Y mean beam moves to th eleft and down, respectively. Ask MCC to set the orbit locks using 2H00 and 2H02 BPMs, tell them x,y positions on these BPMs, see above After getting the beam to FC with parameters close to or better than [5], align beam relative to SVT - call SVT expert if alignment changes the beam positions, make sure to record new positions on 2H00 and 2H02 and ask MCC to change the orbit locks to the new numbers Turn ON calorimeter and the hodoscope, run DAQ (even if no SVT, only ECal and hodoscope) with 8 um W target and 100 nA. Record trigger rates (dump the trigger GUI into the logbook). With any problems with DAQ call the expert cell phone SVT commissioning (Cameron) Run baseline measurements to set the threshold Time-in SVT, requires moving to 3 mm from beam position Set up the Trigger (if needed contact Valery on PDL phone) and DAQ, and take data After checking data, occupancies in SVT using DQM, move SVT to 1.5 mm and take more data Every Shift: Follow the run plan as outlined by RC With any issue contact On-Call Experts or RC Monitor carefully the SVT bias current (see below for details) If any concern about beam stability, ask MCC if orbit locks are on (they should be ON). Keep shift summary up to date in HBLOG. Record all that happens. Document any beam condition change and send scaler GUIs to HBLOG Fill out BTA hourly. Click "Load from EPICS" to automatically fill the left side then make sure numbers are correct. If needed edit the entry. Note: in the "Sift information" tab choose experiment E12-11-006. . At the end of the shift send BTA to teh logbook. Fill and submit the shift checklist in the logbook Every Run: After "Go": Check SVT Occupancy Update the Run Spreadsheet Log screenshots of: main scaler_hps display ECAL FADC rate gui Trigger rate gui SVT and HODOSCOPE and ECAL Monitoring pdfs Please watch Hybrid sync GUI for correct status (currently three red lights) and the L0-3 and L4-6 occupancy plots for any empty plots beyond the expected three. SVT Bias Currents: Shifters must pay attention to the L0 bias currents. This is on both the SVT motor GUI and the main bias GUI. The bias currents will slowly creep up over the course of a run. When the bias current is between 15-20 uA for either L0 sensor, do the following: Stop the run. Take the beam away, turn off SVT bias voltages, and wait 10 min. Turn the bias voltages back on. Check that the L0 bias currents have gone back down to ~4 uA Bring back the beam and start a new run. Do not let the bias current exceed 20 uA. It takes about 4-5 hours for the bias currents to creep up to those values. Call SVT expert if unsure. Harp Scan Procedure: During harp scans, SVT must be retracted (motors/SVT Positioners). HVs on SVT, ECal and Hodoscope should be OFF. Halo counter FSDs (Downstream, HPS Up and HPS Down) are masked, Beam current 100 nA, Orbit locks running. Perform the HARP scan, log the results. If the beam looks different, you should call beam-line on-call that will advise on the next steps. If the beam looks different, perform SVT wire scan, the target needs to be retracted as well for this one. Important Notes: When re-establishing beam to Hall B after a >1h long downtime follow "General Guidelines" on the right and the Beamline Procedures and Manual on the shift documentation page. Do not hesitate to call the beamline expert. Do not run more than 60 minutes above 30 nA without the beam blocker in front of Faraday cup. Put beam blocker in for long running at high currents. For SVT Operations: From the time beam first comes into the hall until it is being delivered to the Faraday cup with orbit locks on for a known good trajectory, the SVT should be completely off. This is especially important during tuning to the tagger dump, when mis-steering of the beam can result in very high hard neutron backgrounds. Once stable beam is being delivered to the Faraday cup with orbit locks on for a known good trajectory, and the SVT collimator is in position, the FEBs and hybrids can be powered and operated, but the HV bias for the sensors must remain off. In order to turn on the HV, the FSD system must be functioning so a beam excursion that hits the collimator will quickly trip off the beam.

General Instructions Establishing Physics Quality Beam for HPS: Make sure SVT is retracted and detectors, SVT, Hodoscope and ECAL are OFF. If the beam was off for 4 hours or more or in case of troublesome beam tuning, send a beam to the tagger dump: Check that beam type is set to "Photon" (HPS_EPICS->Beam->BTA). Position "Blank" on the beam for the Hall-B collimator Ask MCC to turn ON the tagger magnet and then deliver <10 nA beam to the tagger dump. Check the beam position on the tagger viewer, it should be approximately in the center of the screen Follow instructions under "Procedures" on the documentation tab for "Beamline"[6]. To tune the beam on tagger dump and perform harp scans beam current should be <10 nA. Check profile using 2C21 and tagger (2C24) harp scans and compare the positions and widths with previous scans ([7],[8]) Positions on both harps should be within 1mm Width on 2C21 should be <~0.2+/-0.05 mm Width on tagger harp (2C24) <~0.5 +/- 0.1mm Background levels on harp scans are comparable to those of previous scans. Before sending a beam to the Faraday cup If HPS chicane must be ON, make sure that chicane GUI says "Chicane Ready" Set Hall-B Collimator to 20 mm. Check that SVT protection collimator is ON THE BEAM (2.82 mm). If the beam was off for more than 4 hours or the configuration has changed, start with 8 mm HPS target is OUT and Hodoscope and ECAL HVs are OFF SVT is OUT (position=0.000 mm on the main HPS scaler GUI) and bias HV is off (all red/green indicators RED in SVT bias GUI) If any uncertainty, page the experts Pay attention to the following corrector values: 2C22H, 2C23V, 2H00H, 2H00V, Compare them to ones that are in [9]. Make sure their values don't differ more than 100%. If there is such a difference, tell MCC about this. Send beam to the Faraday cup If the beam optics is correct, then you should immediately see the beam spot on the Downstream Viewer and on the 2H00 and 2H02 BPMS. If you don't see it immediately, and rates on halo counters are more than 100 Khz, then ask MCC, to change to pulsed (tune mode) beam, and ask to restore corrector values. At this point don't accept any CW beam, until the beam spot is visible on Downstream Viewer. If the MCC operator is not able to tune the beam for more than 30 minutes, then notify RC! Follow the instructions under "Procedures" on the documentation tab for "Beamline"[10] to establish beam to the electron dump. Note: in order to have reliable readings on two important for HPS BPMs, 2H00 and 2H02, beam current should be >30 nA. Ask MCC to establish 30 nA beam with HPS orbit locks on (We need HallBHPSOrb not HallBOrb configuration). For orbit lock positions on 2H00(X=1.0,Y=1.5) and on 2H02(X=-1.7,Y=0.3). Use the 2.82 mm SVT collimator. (positions changed 6/25/19 by mg). Tune beam profile at HPS using measured widths on 2H01A and 2H02A harps. The required beam profile at 2H02A harp is: X-width <~0.1 mm, Y-width <~ 0.05 mm. Beam profile using 2H01A and 2H02A harps with previous scans ([11],[12]) to compare. Check and log the beam spot on chromax viewer The halo counter rates before HPS must be very low: Upstream Left and Right, and the tagger counters few 10's of Hz, Downstream counters should count <Hz/nA The halo counter rates on HPS, HPS-L/R/T/SC, depends on the collimator and HPS chicane settings, but should not be more than 50 Hz/nA [13] Positions on BPMs must be close to what they were before [14] When everything is stable, perform SVT wire scan and compare with the nominal [15] Once all the above is achieved, turn ECAL and Hodoscope HV ON to monitor and log ECal rates Insert the 20 um W target (turn beam off first). Before accepting the beam, make sure all the previous conditions are met. Always read previous log entries, compare settings of BPMs and correctors with previous settings using scaler_hps GUI.

RC daily meetings at 3 pm in the counting-house 2nd-floor conference room.

BlueJeans Info:

URL: https://jlab.bluejeans.com/759437905

Meeting ID: 759437905

Status of the run

Run Coordinator 08/23 - 09/01 Stepan Stepanyan 09/01 - 09/08 09/08 - 09/15 Maurik Holtrop 09/15 - 09/22 09/22 - 09/29 Tim Nelson 09/29 - 10/06 Rafayel Paremuzyan 10/06 - 10/13 10/13 - 10/20 Cameron Bravo Physics Division Liaison HPS-2019 Valery Kubarovsky

Beamline 08/23 - Eugene Pasyuk - SlowControls 08/23 - Nathan Baltzell ECAL/HODOSCOPE 08/23 - Nathan Baltzell - DAQ 24/7/365 Sergey Boyarinov

SVT 08/23 - 09/02 Tim Nelson 09/02 - Cameron Bravo - Omar Moreno - Matt Solt - Vitaliy Fadeyev - Matt Solt

Webcams: Tagger Dump Faraday Cup Alcove, SVT Chiller

Accelerator: Accelerator EPICS-WEB (offsite access) Accelerator Status Page HPS EPICS-WEB (offsite access) End Station Status Accelerator Ops 1 Accelerator Ops 2 Accelerator White Board Schedule Accelerator OPS Documents

Slow Controls: HPS MYA Variables Hall B EPICS Database

Online & Offline: DQM Monitoring Gui Run Database Run Conditions Database HPS Data Catalog Jenkins / Nexus / SVN Confluence Shift Docs @ GitHub

System/Person	Pager/Phone Number
Run Coordinator	(757) 575-7540 (cell)
Physics Div. Liaison	(757) 876-1789 (cell)
MCC-OPS	7048
Crew Chief	7045
Crew Chief	9-879-3367 (cell)
Program Deputy	9-876-7997 (cell)
Gate House Guard	5822
DAQ/Online	(757) 869-2188 (cell)
SVT	(757) 329-4844 (cell)
ECAL/Hodo	(757) 310-7198 (cell)
Slow Controls	(757) 748-6922 (cell)
Beamline	(757) 303-3996 (cell)
Engineering	(757) 748-5048
Hall-B Floor	5165
Hall-B Space Frame	5170, 5171
Hall-B Forward Carriage	5371
Hall-B Counting Room	5244(Shift1), 5245(Shift2)
Hall-B Counting Room	5247(Expert), 5502(Target)
Hall-B Counting Room	5246(RC1), 5126(RC2)
Hall-B Gas Shed	7115

Overview Bluejeans for 24-7 communication with counting house: https://bluejeans.com/950041022 Remote VNC connection instructions: https://logbooks.jlab.org/entry/3880107 All necessary applications should be avaible from the desktop menu (left/right click on the desktop) EPICS GUIs should be accessed ONLY via the desktop menu or by running hps_epics_remote. Tasks Fill shift checklist? Upload plots to the Hall B logbook once per run EPICS beamline overview screen Trigger GUI ECAL and HODO scaler screens Monitor beam quality EPICS overview screen In VNC or Web Browser Strip charts In VNC or Web Browser: Upstream/Midstream Halo Counters, Downstream Halo Counters, Beam Currents, BPM Positions Occupancy & Expert Monitoring from any clon machine, log in as hpsrun and run these commands: ECAL: startEcalMonitoring HODO: startHodoMonitoring SVT: startSVTCheckout Recon: startReconMonitoring In order for occupancies to be useful, they must be acquired without beam trips. see Monitoring Gui for description of how GUI works Online Full Reconstruction (work in progress) jas3 or http://clonfarm11.jlab.org:8080/HPSRecon/ Insert link to a good reference here Expert

Shift Worker Backup Table To add your name, edit this wiki page or send email to Maurik or Nathan. Worker Shift Backup Date Day Swing Owl Sun, Aug 22 - - - Mon, Aug 23 - - - Tue, Aug 24 - - - Wed, Aug 25 - - - Thu, Aug 26 Raffaella De Vita Valeria Sipala Raphaël Dupré Fri, Aug 27 Mariangela Bondi Valeria Sipala Raphaël Dupré Sat, Aug 28 Mariangela Bondi Valeria Sipala Raphaël Dupré Sun, Aug 29 Mariangela Bondi Valeria Sipala Raphaël Dupré Mon, Aug 30 - Natasa Dashyan Raffaella De Vita Tue, Aug 31 - Natasa Dashyan Mariangela Bondi Wed, Sep 1 - Natasa Dashyan Mariangela Bondi Thu, Sep 2 Silvia Niccolai Natasa Dashyan Raffaella De Vita Fri, Sep 3 Silvia Niccolai Nunzio Randazzo Raphaël Dupré Sat, Sep 4 Silvia Niccolai Nunzio Randazzo Raphaël Dupré Sun, Sep 5 Silvia Niccolai Nunzio Randazzo Raphaël Dupré Mon, Sep 6 Silvia Niccolai Nunzio Randazzo Raphaël Dupré Tue, Sep 7 Alessandra Filippi Natasa Dashyan Raphaël Dupré Wed, Sep 8 Alessandra Filippi Natasa Dashyan Raphaël Dupré Thu, Sep 8 Alessandra Filippi Natasa Dashyan - Fri, Sep 10 Alessandra Filippi Natasa Dashyan - Sat, Sep 11 Raffaella De Vita Valeria Sipala Domenico D'Urso Sun, Sep 12 Andrea Celentano Valeria Sipala Domenico D'Urso Mon, Sep 13 Luca Marsicano Valeria Sipala Domenico D'Urso Tue, Sep 14 Luca Marsicano Valeria Sipala Domenico D'Urso Wed, Sep 15 Raffaella De Vita - Valeria Sipala Thu, Sep 16 Luca Marsicano - Valeria Sipala Fri, Sep 17 Andrea Celentano - Valeria Sipala Sat, Sep 18 Andrea Celentano - Valeria Sipala Sun, Sep 19 - Annalisa D'Angelo - Mon, Sep 20 - Alessandra Filippi - Tue, Sep 21 - Alessandra Filippi - Wed, Sep 22 - Alessandra Filippi - Thu, Sep 23 - Andrea Celentano Nunzio Randazzo Fri, Sep 24 - Raffaella De Vita Nunzio Randazzo Sat, Sep 25 - Raffaella De Vita Nunzio Randazzo Sun, Sep 26 - Luca Marsicano Nunzio Randazzo Mon, Sep 27 Gabriele Simi - - Tue, Sep 28 Gabriele Simi - - Wed, Sep 29 Gabriele Simi - - Thu, Sep 30 Gabriele Simi - - Fri, Oct 1 - - Marzio de Napoli Sat, Oct 2 - - Marzio de Napoli Sun, Oct 3 - - Marzio de Napoli Mon, Oct 4 - - Marzio de Napoli Tue, Oct 5 - - Annalisa D'Angelo Wed, Oct 6 - - Annalisa D'Angelo Thu, Oct 7 - - Annalisa D'Angelo Fri, Oct 8 - - Annalisa D'Angelo Sat, Oct 9 Alessandra Filippi Gabriele Simi Luca Marsicano Sun, Oct 10 Annalisa D'Angelo Gabriele Simi Luca Marsicano Mon, Oct 11 Annalisa D'Angelo Gabriele Simi Andrea Celentano Tue, Oct 12 Annalisa D'Angelo Gabriele Simi Andrea Celentano Wed, Oct 13 - Luca Marsicano Domenico D'Urso Thu, Oct 14 - Andrea Celentano Domenico D'Urso Fri, Oct 15 - Mariangela Bondì Domenico D'Urso Sat, Oct 16 - Mariangela Bondì Domenico D'Urso Backup shifter contact info Name Email Cell phone Andrea Celentano andrea.celentano@ge.infn.it ‭+39 340 9831283‬ Domenico D'Urso ddurso@uniss.it +39 349 3630 242 Gabriele Simi gabriele.simi@pd.infn.it +39 320 748 3385 Hakob Voskania voskania@jlab.org +37495909998 Luca Marsicano luca.marsicano@ge.infn.it +39 333 9893725‬ Mariangela Bondì mariangela.bondi@ge.infn.it +39 ‭327 1895733‬ Marzio de Napoli marzio.denapoli@ct.infn.it +39-3498834468 Maurik Holtrop holtrop@jlab.org +1-603-868-8088 Natasa Dashyan natasha@jlab.org +37477538360 Nathan Baltzell baltzell@jlab.org +1 757 748 6922 Nunzio Randazzo nunzio.randazzo@ct.infn.it +39-3472591331 Raffaella De Vita Raffaella.Devita@ge.infn.it +39 340 8110156 Raphaël Dupré raphael.dupre@ijclab.in2p3.fr +33 670 977 761 Silvia Niccolai silvia@jlab.org +33 624 81 67 78 Valeria Sipala vsipala@uniss.it +39 339 339 57 04