Difference between revisions of "Feb runplan"

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(Straight-through Optics (Mar 2nd- Mar 4th))
 
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== Straight-through Beamline Commissioning (Y. Roblin) 29 Feb - Mar 1st ==
+
== Straight-through Beamline Commissioning 2nd Feb (swing) thru 1st Mar (owl) ==
  
 
Initial Beam Accelerator Ops, with assistance from the Hall A shift crew. This includes delivery of beam to the Hall A (not local) dump, commissioning of the BPMs, calibration with the Harp and power up of the rasters.
 
Initial Beam Accelerator Ops, with assistance from the Hall A shift crew. This includes delivery of beam to the Hall A (not local) dump, commissioning of the BPMs, calibration with the Harp and power up of the rasters.
  
Full Details for ONLY straight-through beam delivery are provided at:
+
Full Details for ONLY straight-through beam delivery are provided in Yves Roblin's testplan  ([http://opsweb.acc.jlab.org/CSUEApps/atlis/task/12015 atlis]) ([http://hallaweb.jlab.org/experiment/g2p/docs/12015.pdf pdf])
* Initial straight-through beam delivery [http://opsweb.acc.jlab.org/CSUEApps/atlis/task/12015 atlis] [http://hallaweb.jlab.org/experiment/g2p/docs/12015.pdf pdf]
+
  
 
<U>Start-up configuration</U>
 
<U>Start-up configuration</U>
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# Spectrometers at 12.5 degrees, <math>P_0=2251.8</math> MeV/c (carbon elastic).
 
# Spectrometers at 12.5 degrees, <math>P_0=2251.8</math> MeV/c (carbon elastic).
 
# Sieve slits : OUT.
 
# Sieve slits : OUT.
# Septa settings: 5.69 degrees.
+
# Septa settings: <STRIKE>5.69 degrees</STRIKE>. Current=0
 
# Compton chicane: OFF.
 
# Compton chicane: OFF.
 
# Polarized Target chicane : OFF and degaussed.
 
# Polarized Target chicane : OFF and degaussed.
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# Check BCM signals in the scalers (HRS, third arm)
 
# Check BCM signals in the scalers (HRS, third arm)
  
<U> Tungsten Calorimeter Check-out </U> (Alexandre, Pengjia)
+
<U> Tungsten Calorimeter Check-out </U> (Alexandre, Pengjia, Arne, Mahmoud ) [http://devweb.acc.jlab.org/CSUEApps/atlis/task/11755 ATLis]
  
 
(Can be done either in straight-through or when going through Chicane)
 
(Can be done either in straight-through or when going through Chicane)
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== HRS/Detector Checkout  ==
 
== HRS/Detector Checkout  ==
  
(Resp: g2p students)
+
Most of these check-out can be done during the initial beamline commissioning( both straight-through or when going through Chicane). The order in which these checks are done do not matter (some of them are independent). After we finish these checks we should be ready to do optics runs with target field.
 
+
* Most of these check-out can be done during the initial beamline commissioning( both straight-through or when going through Chicane).  
+
* The order in which these checks are done do not matter (some of them are independent).
+
* After we finish these checks we should be ready to do optics runs with target field.
+
  
 
<U> HRS Detectors Check-out </U> (Melissa, Ryan, Vince)
 
<U> HRS Detectors Check-out </U> (Melissa, Ryan, Vince)
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# Establish non linearity of the Lumi detectors  
 
# Establish non linearity of the Lumi detectors  
 
# Measure lumi asymmetries
 
# Measure lumi asymmetries
 
== Straight-through Optics (Mar 2nd- Mar 4th)==
 
(Resp : Jixie, Min et al.)
 
 
<U> HRS and Septum Magnet Checks</U>
 
# Controlled Access to insert Sieve Slit (if they are not already in position).
 
# Cycle magnets?
 
# Use carbon target and set HRS to elastic setting.
 
# Septum field vs current, checks with carbon elastic peaks
 
## Set the dipole first and then tune quads?
 
  
 
== On-line Analysis  ==  
 
== On-line Analysis  ==  
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# Make sure all on-line analysis scripts are up to date on both arms
 
# Make sure all on-line analysis scripts are up to date on both arms
# Post easy instructions for the shift crew on how to start online analysis (stick notes near the DAQ machine)
+
# Post easy instructions for the shift crew on how to start online analysis on [https://hallaweb.jlab.org/wiki/index.php/G2p_shifts the shift worker instruction page]
 
# Make sure all the important information is recorded correctly in the datastream:
 
# Make sure all the important information is recorded correctly in the datastream:
 
## EPICS: Beam diagnostics(BCM, BPM, HARP etc..)
 
## EPICS: Beam diagnostics(BCM, BPM, HARP etc..)
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# Start-of-Run and End-of-Run information is up to date with all relevant info
 
# Start-of-Run and End-of-Run information is up to date with all relevant info
  
== Compton Test (2 shifts, Mar 3-4) ==
+
==  Moller Commissioning (1 shift, Mar. 3) ==
 
+
(Resp: Sirish et al.)
+
 
+
# Establish beam through Compton chicane
+
# 2nd shift is contingent on clean tune established by end of first shift.
+
#??
+
 
+
==  Moller Commissioning (1 shift, Mar. 3- 4) ==
+
  
 
(Resp: O. Glamazdin, J. Zhang)
 
(Resp: O. Glamazdin, J. Zhang)
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# Larger charge asymmetry runs to check BCM/helicity signals in HAPPEX, HRS, thirdarm, Moller DAQs simultaneously
 
# Larger charge asymmetry runs to check BCM/helicity signals in HAPPEX, HRS, thirdarm, Moller DAQs simultaneously
 
# Establish that there are no problems by checking Hall-A beam charge asymmetries measured in Hall-C
 
# Establish that there are no problems by checking Hall-A beam charge asymmetries measured in Hall-C
 +
 +
== Straight-through Optics (Mar 2nd- Mar 4th)==
 +
(Resp : Jixie, Min et al.)
 +
 +
<U>Overview</U> (Full details [http://hallaweb.jlab.org/experiment/g2p/collaborators/jixie/20120226_Optics_Final/g2p_optics_plan.pdf here])
 +
# Preparation:
 +
## Escorted Access to insert Sieve Slits. Drain liquid helium out to expose the target.
 +
## Cycle Q2 and Q3, set HRS momentum to 2.254 GeV/c, Use C12 target
 +
## Tune septum, start from 810A till 660A, 15A each step, expected value: 730.3A
 +
## Tune quardroples,  change it to: +2%, 1%, -1% -2% (Min will provide more details)
 +
# Escorted Access to insert Sieve Slits.
 +
# Delta scan.
 +
# Beam position scan
 +
# Escorted Access to move Sieve Slits out. Do acceptance calibration: use large C12(40 mil) foil in the 6th cell, rasters on and off
 +
# Refill liquid helium. Escorted Access to insert Sieve Slits.
 +
# Change to CH2 target, do pointing
 +
 +
== Compton Test (2 shifts, Mar 4-5) ==
 +
 +
(Resp: Sirish et al.)
 +
 +
# Establish beam through Compton chicane
 +
# 2nd shift is contingent on clean tune established by end of first shift.
 +
# Full details in Sirish testplan.
  
 
== Commissioning Beamline Chicane I (March 5th)==
 
== Commissioning Beamline Chicane I (March 5th)==
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# Move to GEp production
 
# Move to GEp production
  
== Optics with chicane (March 5th onwards) ==
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== Optics with chicane (March 6th onwards) ==
  
 
(Resp: Jixie, Min, Vince et al.)
 
(Resp: Jixie, Min, Vince et al.)
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(Resp : Kalyan, Jixie)  
 
(Resp : Kalyan, Jixie)  
  
# E0= 2.2 GeV, B = 5 T and theta_target = 6 deg
+
# Take 2 hour runs on NH3 elastic setting for every g2p production configuration and every target cup
## Run with thick Carbon target, raster on, 100nA  (approximation for N2 contribution)
+
# For the background contribution (can be done once):
## Run with Empty Cell which should include Al end caps + NMR coil + He4
+
## Run(<1hr for 2.5T) with thick Carbon target, raster on, 100nA  (approximation for N2 contribution)
## Run with No target to get contribution from He4 only ?
+
## Run(<1hr for 2.5T) with Empty Cell which should include Al end caps + NMR coil + He4
# Repeat these measurement in every g2p/gep configuration
+
### This cell should be requested during the production, when target stick is changed
 
+
## Run (<1hr for 2.5T)) with No target to get contribution from He4 only ? (can be done any time)
== Target Thickness Runs ==
+
 
+
# For every g2p production setting take NH3 elastic runs
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# This should be done for every target stick
+
  
 
== Beam Energy Measurement  ==
 
== Beam Energy Measurement  ==

Latest revision as of 00:57, 4 March 2012

E08-027/E08-007 Commissioning Runplan (K. Slifer / K. Allada)


Straight-through Beamline Commissioning 2nd Feb (swing) thru 1st Mar (owl)

Initial Beam Accelerator Ops, with assistance from the Hall A shift crew. This includes delivery of beam to the Hall A (not local) dump, commissioning of the BPMs, calibration with the Harp and power up of the rasters.

Full Details for ONLY straight-through beam delivery are provided in Yves Roblin's testplan (atlis) (pdf)

Start-up configuration

  1. Two pass beam, E0 =2.2 GeV, polarized, no raster.
  2. Current: Initially pulsed up to 2-4<math>\mu</math>A pulsed, then up to 5 <math>\mu</math>A CW.
  3. Spectrometers at 12.5 degrees, <math>P_0=2251.8</math> MeV/c (carbon elastic).
  4. Sieve slits : OUT.
  5. Septa settings: 5.69 degrees. Current=0
  6. Compton chicane: OFF.
  7. Polarized Target chicane : OFF and degaussed.
  8. Tungsten Calorimeter : Retracted.
  9. Polarized Target: Field OFF

Beam Diagnostics Check-out (Pengjia, Alexandre, Kalyan)

  1. Check BPM, slow and fast raster signals in the data
  2. Is spot++ working for both arms?
  3. Do HARP scan
  4. BPM calibration by Pengjia here
    1. It includes calibrating beam positions with both straight-thru and target field ON
  5. Check BCM signals in the scalers (HRS, third arm)

Tungsten Calorimeter Check-out (Alexandre, Pengjia, Arne, Mahmoud ) ATLis

(Can be done either in straight-through or when going through Chicane)

  1. Commission tungsten calorimeter
  2. BCM calibration ?
  3. How do we establish that we can achieve ~1% measurement ?

HRS/Detector Checkout

Most of these check-out can be done during the initial beamline commissioning( both straight-through or when going through Chicane). The order in which these checks are done do not matter (some of them are independent). After we finish these checks we should be ready to do optics runs with target field.

HRS Detectors Check-out (Melissa, Ryan, Vince)

  1. Check all the detectors in both arm to establish that we don't have problems.
  2. Post ALL the online plots for the detectors (ADC, TDC etc..) in the Halog
    1. VDC (efficiencies etc..)
    2. Gas Cerenkov (ADC and timing peaks)
    3. S1 and S2m (ADC and timing peaks)
    4. Lead-glass Calorimeter (ADC)
  3. Check HV on all the detectors, align the peaks if necessary

DAQ/Trigger Check-out (Melissa, Ryan, Vince)

  1. Establish the DAQ conditions for production
    1. What is the max rate DAQ can run with < 20% DT (Buffered and unbuffered mode) ?
    2. Record deadtime as a function of DAQ rate. Change rate via current or prescalers.
    3. Check synchronization of ROCs in buffered mode
    4. Make sure all important scaler channels are working (BCM, Helicity, triggers, L1A, clock)
    5. Check scalers in S1 and S2m detectors for double pulsing

Third Arm Detector Check-out (Chao, Kalyan)

  1. Set thresholds for 2.2 GeV beam
  2. Check for bad channels, double peaks etc ..
  3. Check deadtime, helicity, BCM scalers

Lumi Detector Check-out (Pengjia, Kalyan)

  1. Adjust HV with 100nA current to make sure all channels are roughly aligned and there is no saturation in Happex ADC
  2. Establish non linearity of the Lumi detectors
  3. Measure lumi asymmetries

On-line Analysis

(Resp: Toby)

  1. Make sure all on-line analysis scripts are up to date on both arms
  2. Post easy instructions for the shift crew on how to start online analysis on the shift worker instruction page
  3. Make sure all the important information is recorded correctly in the datastream:
    1. EPICS: Beam diagnostics(BCM, BPM, HARP etc..)
    2. Target variables
    3. Helicity sorted scalers information ( triggers, L1A, BCM, helicity etc.)
    4. Helicity in ADC, scaler, TIR
  4. Start-of-Run and End-of-Run information is up to date with all relevant info

Moller Commissioning (1 shift, Mar. 3)

(Resp: O. Glamazdin, J. Zhang)

  1. Detector HV tuning (30min)
  2. Q1 and Q2 quadruple magnets scan (1hour)
  3. Moller target longitudinal scan (30 min)
  4. Beam polarization measurement (30-40min)
  5. MCC job (to set Moller settings and to restore previous beam parameters) (~2hours)

Total: 5 hours.

Helicity Checks

(Resp: Chao, Pengjia, Kalyan)

  1. Better to do this during Moller runs
  2. Larger charge asymmetry runs to check BCM/helicity signals in HAPPEX, HRS, thirdarm, Moller DAQs simultaneously
  3. Establish that there are no problems by checking Hall-A beam charge asymmetries measured in Hall-C

Straight-through Optics (Mar 2nd- Mar 4th)

(Resp : Jixie, Min et al.)

Overview (Full details here)

  1. Preparation:
    1. Escorted Access to insert Sieve Slits. Drain liquid helium out to expose the target.
    2. Cycle Q2 and Q3, set HRS momentum to 2.254 GeV/c, Use C12 target
    3. Tune septum, start from 810A till 660A, 15A each step, expected value: 730.3A
    4. Tune quardroples, change it to: +2%, 1%, -1% -2% (Min will provide more details)
  2. Escorted Access to insert Sieve Slits.
  3. Delta scan.
  4. Beam position scan
  5. Escorted Access to move Sieve Slits out. Do acceptance calibration: use large C12(40 mil) foil in the 6th cell, rasters on and off
  6. Refill liquid helium. Escorted Access to insert Sieve Slits.
  7. Change to CH2 target, do pointing

Compton Test (2 shifts, Mar 4-5)

(Resp: Sirish et al.)

  1. Establish beam through Compton chicane
  2. 2nd shift is contingent on clean tune established by end of first shift.
  3. Full details in Sirish testplan.

Commissioning Beamline Chicane I (March 5th)

  1. FZ2 magnet to Yves config #5 (As early in day shift as possible).
  2. Alignment and survey.
  3. Ramp up Target Magnet from 0T to 2.5T.
  4. Target in beam : Carbon.
  5. Restablish beam. Mostly Y. Roblin will be driving this part (I will put an ATLis link when it is available):
  6. Start with E0 = 2.2 GeV , B = 2.5 T and theta_target = 90 deg
    1. Check beam diagnostics again, when going through chicane
    2. We can do some of our optics while Yves is doing this checks (Jixie et al.)
    3. BPM+slow raster calibration can also be done during this time (Pengjia)
  7. Initial GEp production

Commissioning Beamline Chicane II (March 6th)

  1. FZ2 magnet to Yves config #8. (As early in day shift as possible).
  2. Alignment and survey.
  3. Target magnet rotation from 90 to 6 degrees.
  4. Ramp up Target Magnet from 2.5T to 5.0T.
  5. Target reconfiguration: 70GHz to 140 GHz.
  6. Target in beam : Carbon.
  7. Reestablish beam. Mostly Y. Roblin will be driving this part (I will put an ATLis link when it is available):
    1. Check beam diagnostics again, when going through chicane
    2. We can do some of our optics while Yves is doing this checks (Jixie et al.)
    3. BPM+slow raster calibration can also be done during this time (Pengjia)
  8. E0= 2.2 GeV, B = 5 T and theta_target = 6 deg
    1. Continue doing optics (Jixie et al.)
  9. Move to GEp production

Optics with chicane (March 6th onwards)

(Resp: Jixie, Min, Vince et al.)

  1. With beam going through chicane:
    1. Full details are provided at : Optics run plan

Dilution/Packing fraction Runs

(Resp : Kalyan, Jixie)

  1. Take 2 hour runs on NH3 elastic setting for every g2p production configuration and every target cup
  2. For the background contribution (can be done once):
    1. Run(<1hr for 2.5T) with thick Carbon target, raster on, 100nA (approximation for N2 contribution)
    2. Run(<1hr for 2.5T) with Empty Cell which should include Al end caps + NMR coil + He4
      1. This cell should be requested during the production, when target stick is changed
    3. Run (<1hr for 2.5T)) with No target to get contribution from He4 only ? (can be done any time)

Beam Energy Measurement

(Resp: Doug?)

  1. Mott ?