Difference between revisions of "CH Weekly Reports"
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* Continued MCNP work. | * Continued MCNP work. | ||
− | ** Discovered | + | ** Discovered issue with tagging photons produced via pair annihilation, worked to debug. |
** Started to recreate simulations such that MCNPVised can parse the input card correctly. | ** Started to recreate simulations such that MCNPVised can parse the input card correctly. | ||
** Adjusted low energy cut off for electrons in sample state of PAS simulation to search for trend in annihilated photons seen in detector. | ** Adjusted low energy cut off for electrons in sample state of PAS simulation to search for trend in annihilated photons seen in detector. |
Revision as of 17:34, 9 December 2022
09/19/22
- Investigated non-linearity of peak sensing ADC due to issues arising in energy calibrations and efficiency measurements.
- Modified existing calibration code to use non-linear regression to account for ADC.
- Sourced material needed for CaGaS Phase II setup.
- Calculated ADC dead time for live-time correction to efficiency measurement count rates and calculated dead time per experiment.
- Designed holder for Gd foils needed for CaGaS Phase II experiment. To be 3D printed and tested for tolerances.
09/26/22
- Printed both parts of the Gd foil holder for CaGaS Phase II.
- Parts fit together adequately considering they're 3D printed and not machined.
- M3 bolts threaded through first part of the holder.
- M3 nuts pressed into the second part of the holder.
- Parts printed out of PETG plastic with low density infill (10%).
- Edited rebinning code for energy calibrations for data sets collected with ADC to account for changes in calibration code.
- Energy calibration script now uses 2nd order polynomial regression to account for nonlinearity of ADC
- The coefficients from the regression are passed to another script to rebin ADC data from channel to energy, preserving bin count, but bin width will increase as a function of energy.
- End goal is to pass coefficients into rebinning function and draw energy calibrated plot in the same script.
- Designed Gd2O3 powder holder for CaGaS Phase II.
- Have spray on clear coat to seal plastic after printing is complete in hopes that powder will not stick between printed layers when used.
- Documented Gd holders in wiki with rendered images and a description of intended use.
- Continued to research live time correction for HPGe count rates and think I have applied the correction correctly at the initial measurement level, which will be propagated through to efficiency calculations.
- Researched and tested different integration methods for more accurate measurement of counts in energy peak to compare to Gaussian fit.
- Created tentative list of committee members with major advisor for PhD proposal defense and future dissertation defense.
10/03/22
- Sat in on 30 minute proposal defense presentation by another Ph.D. candidate.
- Began the 3D print of Gd2O3 holder for CaGaS Phase II.
- Both parts printed and fit together tightly. Need to be sealed for use with powder.
- Updated wiki documentation with images of the holders.
- Working with ISU Environmental Health & Safety to set up time to treat and coat lead bricks to build CaGaS Phase II setup.
- Air monitoring and respirators are required per ISU EH&S safety protocols.
- Designed and printed a holder for Cs137 calibration source for storage in lab (signed off with RSO) for easy point calibrations using HPGe.
- Researched dead time adjustment in Practical Gamma-ray Spectrometry by Gordon Gilmore
- Collected 50 data points for ADC gate width, read out controller trigger width, and the delay between end of gate and beginning of read trigger.
- Found dead time per pulse which includes memory storage time, thanks to reading the aforementioned book.
- Worked to re-plot and integrate Eu152 peaks, but source data file seems to be corrupted. Will collect new set of data on Monday (10/10/22) when I can access calibration sources.
- Re-plotting is necessary for new integration with 2nd order polynomial binning and new live time correction.
- Collecting a new Eu152 spectrum is needed before CaGaS Phase II for new energy calibration as NIM bin has been power cycled and spec-amp gain has shifted.
10/10/22
- Moved extra lead for CaGaS Phase II from lead storage at ISU to lab for coating prior to use.
- Coated 30 lead bricks for CaGaS Phase II setup.
- Fixed energy calibration code thanks to input from a colleague.
- Machine precision and how ROOT interprets bins was cause of the issue.
- Designed tools to use to level and compact powder into the powder holder for use during CaGaS Phase II.
- Designed new covers for powder holder to better accommodate for different thicknesses of powder.
- Experimentally confirmed minimum dead and maximum bounds on dead time of data acquisition system per event after questions from colleague and plotted voltage traces for documentation.
- Refit 152Eu energy peaks with gaussians + linear background and recalculated efficiencies using live time correction.
- Finished replotting and calculating uncertainty in HPGe efficiency measurements to present next week, all calibration sources (152Eu, 137Cs, & 60Co).
- Met with collaborators and discussed FY23 work scope.
- Setup recurring meetings biweekly starting 10/19/22.
- Contributed to Paul's SOW for FY23.
10/17/22
- Uploaded new versions of efficiency measurement plots to wiki.
- Wrote up efficiency measurement results, explained in detail how the calculations work.
- Wrote up and defined equations for uncertainty calculations, found lack of count statistics is highly influencing uncertainty in efficiency measurements. Working to rectify by collecting new data sets with 152Eu with increased run time.
- Collected new on & off axis 152Eu spectra and overnight background for background subtraction. -> Power stability issues to clean room crashed DAQ2 for background run.
- Had data acquisition failure due to high count rate halfway through one run, estimated run time based on ratio of rates from previous measurements and decay of 152Eu source between past and present runs.
- Created slides and presented HPGe Efficiency write up to collaborators.
- Met with advisor and verified methods for calculations were reasonable.
- Adjusted design of powder flattening tool to make it easier to use and 3D print.
- Continued work on write up of experimental design and results for CaGaS Phase I.
- Started drafting run plan for CaGaS Phase II.
- Currently includes runs using He3 tube to measure thermal neutron rate in detector tunnel as a function Gd thickness.
- HPGe using varying thicknesses of Gd foils and powder.
- Plan is to vary the distance between detector & gadolinium to be able to account for coincidence peaks problem.
10/24/22
- Finished 3D printing all Gd2O3 powder flattening/compacting tools designed previously.
- Stayed up to date with INL required training modules.
- Used feedback from Ph.D. committee members to improve efficiency measurements.
- Debugged and replaced part of signal propagation chain for HPGe electronics chain.
- Finished full automation of energy calibration code. Now takes ADC spectrum, energy calibrates, rebins, replots, and scales by runtime.
- Commented code and uploaded to ISU wiki & DAQ2 for preservation with brief explanations of functionality and methods.
- Wiped down the freshly coated lead bricks from last week and moved them into the clean room to use in CaGaS Phase II construction.
- Discussed efficiency measurements with Paul and received his feedback on how to improve the analysis, mostly pertaining to the fitting function used in integrating energy peaks.
- Also covered altering construction plans of CaGaS Phase II to increase shielding, will depend on material available, and plans for collaboration through FY23.
- Dismantled efficiency measurement setup and began construction of CaGaS Phase II setup.
- Assembled 2" of borated poly on 4ftx4ft steel table
- Flattened sheets of BorAl and laid out base for CaGaS apparatus.
- Met with Chuting, Paul, major advisor, and OSU faculty to discuss experiment details for next spring/summer.
10/31/22
- Continued to construct CaGaS Phase II and document construction process in order to simulate after.
- Milled polyethylene for Gd holders to sit flush with BorAl window.
- Finished construction wednesday morning and began tuning data acquisition system for optimal dead time (Jefferson Lab CODA).
- Began CaGaS Phase II experiments.
- Analyzed first run found that energy resolution is very poor, ~5 KeV FWHM.
- Tested Cs137 source in setup instead of Cf252 to determine if smearing due to higher count rate with large energy range.
- One problem seems to be pre-amp in HPGe is adding heat and increasing detector temp, which reduces resolution. Could be disconnected ground cable, not sure yet.
- Paul has reached out to Craig Maddigan at Ametek (who has helped us previously) to help debug detector. Began working through checklist Craig Maddigan had provided us previously when having detector issues.
- Count rate is not in the range of causing issues for daq system, allowing for minimum dead time.
- Mirrored Phase II setup after determining it is necessary to thermal cycle detector over weekend.
- Detector tunnel and source tunnel have been exchanged and detector is cooling again.
- This orientation seems to shield detector better than before due to lack of concrete wall/BPoly scattering neutrons into rear of detector.
- Detector tunnel and source tunnel have been exchanged and detector is cooling again.
- Presented first design to collaborators on Wednesday afternoon.
11/07/22
- HPGe is nonfunctional currently (Monday)
- Had conference call with John Barncord from Ortec and Paul. John is 2 day air shipping a new sieve pill, o-ring, and high vacuum grease to ISU to use in X-Cooler here.
- Arranged for poptop pumpdown at IAC as detector must be warm to swap sieve pill and o-ring.
- Swapped HPGe out for He3 tube in CaGaS Phase II setup and began taking measurements.
- Set event limit to 10,000,000 events so run will automatically end. Count rate without converter is ~130Hz, with 0.1mm Gd is ~17Hz.
- Sheared 0.13mm Gd foil to 10cm x 10cm for use in Phase II setup and began collecting data using the foil.
- Analyzed spectrum collected from He3 tube and overlaid the data for no converter and 0.1mm Gd converter.
- Did not continue with more thicknesses due to mean free path of neutrons in Gd is so small.
- Removed He3 detector and swapped in NaI detector, energy resolution is poor and signal is too fast currently.
- Finding a way to delay the NaI signal after triggering ADC gate.
- Removed poptop and delivered to IAC for pumpdown.
- HPGe poptop has been pumped down to 1·10-6 torr and I have delivered it back to ISU.
- Will be reattached to cooler as soon as o-ring, sieve pill, and high vacuum grease arrive.
- Worked with colleague at LLNL who has experience with this specific detector, conclusion is issue is most likely electronics.
- Borrowed tail pulse generator to test HPGe pre-amp, which may show distortion in signal if that is the problem.
- Cleaned HPGe thermal contacts and received new parts from ortec.
- Reassembled poptop and X-Cooler assembly, put HPGe detector back in position in CaGaS setup, and began the cooling process.
- Verified that inhibit system works as intended and bias voltage will ramp down if positive voltage is measured across shutdown cable.
- Swapped NIMbin for one with a blackmax power supply, should be more stable.
- Added magnetic switch to X-Cooler and HPGe pre-amp power such that if UPS battery is drained, X-Cooler will turn off and warm detector up. Bias voltage will be killed by power outage, and if X-Cooler loses power for >10mins, full thermal cycle is needed.
11/14/22
- HPGe is functional.
- Maintaining ~110K with new sieve pill, o-ring, high vacuum grease, and fresh poptop pumpdown.
- Used tail pulse generator to pass signal through pre-amp, signal looks somewhat noisy, however could be due to length of cables and noise intrinsic to lab setup. Bias voltage was not active at the time of test, but detector was at operating temperature.
- Noise is not an issue and system was designed to work around this.
- Acquired Gd foil data with thickness beginning at 0.1mm & ending at 0.62mm.
- Had one failure of CODA during a Gd foil run. CODA was restarted, run restarted, original failed run marked as failure to be excluded from data set.
- CODA restarted at the end of each day now. No failures since.
- Had one failure of CODA during a Gd foil run. CODA was restarted, run restarted, original failed run marked as failure to be excluded from data set.
- Measured Gd powder mass and associated thicknesses while setting up for Gd powder measurements.
- Started with ~0.7mm thick layer of compacted powder in 10cm x 10cm basin.
- Performed quick analysis after each CaGaS Phase II run to verify functionality maintained for HPGe detector.
- Held regular check-ins with Paul and discussed optimal way to perform Gd powder mass measurements and deposit/removal of powder when varying thickness.
- Discussed what the "background" measurement would be for this setup. Options are either no 252Cf source or no form of Gd converter. MCNP simulation run by Paul says no converter gives fast neutron flux of 1.3, compared to 1 with converter (volume averaged).
- Collected all Gd thickness measurements, overnight backgrounds, and no converter. CaGaS Phase II data collection complete.
11/21/22
- Compiled CaGaS Phase II data by run type and copied to a second data acquisition machine at ISU, then copied to local machine for analysis.
- Multiple copies now exist in across 3 computers as backups.
- Developed game plan for next step of work with Paul, including MCNP simulations, CaGaS Phase II analysis, Lithium dead layer of HPGe, etc.
- Uploaded remaining images & organized all of CaGaS Phase II setup images.
- Started CaGaS Phase II analysis.
- Overnight background runs show no noticeable change detector resolution or effects due to neutron damage. Slight shift in gain from beginning to end but can easily be compensated for.
- Note: Change in gain most likely due to power to room causing rapid power cycle in NIMbin containing spec-amp. Shift is very minor, ~3 ADC channels which is ~1.2 KeV.
- Overnight background runs show no noticeable change detector resolution or effects due to neutron damage. Slight shift in gain from beginning to end but can easily be compensated for.
- Revised first draft of proposal document.
- Brought previous parts in line with CaGaS Phase II and began drafting CaGaS Phase II write up.
11/28/22
- Worked on mcnp with Paul.
- Successfully implemented tally plotting after having prior issues with Xming & XQuartz on laptop and desktop.
- Began optimizing number of cores used for mcnp sims. Variance reduction being enabled changes this dramatically.
- Got MCNPVised working on windows 10, next is trying to import complicated geometries from our simulations and not examples from manual.
- Discussed OSURR design in-depth with Paul. Proposed shielding/converter design changes that may reduce noise and while preserving signal.
- Met with Chuting, Paul, & Mirion regarding detector type and purchase.
- Included design overview and proposed changes.
- Continued to revise and expand proposal document/dissertation draft.
12/05/22
- Continued MCNP work.
- Discovered issue with tagging photons produced via pair annihilation, worked to debug.
- Started to recreate simulations such that MCNPVised can parse the input card correctly.
- Adjusted low energy cut off for electrons in sample state of PAS simulation to search for trend in annihilated photons seen in detector.
- Simulation time decreases as energy cut off increases.
- Decided on 1KeV electron energy cut off as photon flux due to annihilation does not seem to have a strong dependence on cut off energy, and 1KeV is MCNP default.
- Discovered 4 inch Bismuth plug in fast neutron beam line at OSURR that we had not accounted for in MCNP.
- Successfully added Bismuth as material.
- Added planes to define extent of Bi plug in beam port.
- Rendered simulation setup with Bi plug and can run simulation without errors.
- Began optimization of Gd in In Situ PAS experiment simulations. Currently looking for annihilation photon rate from sample to drop off as function of Gd thickness.
- Researched the fast neutron beam line at OSURR and found multiple documents informing the simulation design. The neutron spectrum exiting the beam port may not be as expected and will need to be simulated. Began work on designing new MCNP simulation using code found in a document written by an OSU graduate student and creating a new source spectrum to estimate the exit spectrum from the collimator at OSURR.