PMT Gain & Resolution Measurements in High Magnetic Fields

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PMT Gain & Resolution Measurements in High Magnetic Fields Vincent Sulkosky University of Virginia August 11 th, 2015 SoLID EC Meeting

High-B Sensor-Testing Facility 2 The facility was designed for the EIC PID Consortium Motivation: DIRC configuration with readout inside a solenoid magnet. PMTs operate inside a 3-T field. Purpose: Evaluation of small photon sensors in magnetic fields. Goal: Determine design characteristics, suitable for DIRC readout.

High-B Sensor-Testing Facility 3 Commissioning: July/August 2014 Data taking: Nov. 2014, July 2015 People: JLab P. Nadel-Turonski, C. Zorn; USC: Y. Ilieva, T. Cao, C. Barber, E. Bringley; ODU: K. Park, G. Kalicy, L. Allison, UVA: K. Jin, V. Sulkosky, N. Ton, X. Zheng

4 Major Components

Sensor Orientation Capabilities 5

6 Electronics Diagram

PMT Properties 7 PMT Assembly Length [cm] Assembly Diameter [cm] Rise Time [ns] Transit Time [ns] TTS [ns] Gain R11102 13.7 4.61 3.2 34 ---- 5e6 H6152-70 12.8 3.1 1.5 5.6 0.35 5e5 H6614-70 8.0 6.0 2.5 9.5 0.44 1e7 1. A magnetic shield provided by Hamamatsu was added to the R11102 PMT. 2. The H6152-70 and H6614-70 are fine-mesh PMTs. 3. Properties are from the Hamamatsu.

8 Data Collected R11102: B = (0, 100) G; θ= (0, 20 ); φ = 0, HV = 1.25 kv H6614-70: B = (0, 1.9) T; θ= (-35,0-50, 215 ); φ = 0,90 ; HV = 1.5 kv and 2.0 kv H6152-70: B = (0, 1.4) T; θ= (-30,0-40 ); φ = 0 ; HV = 2.0 kv (and two points at 2.1 kv) 20x preamp used before the fadc and TDC for the R11102 and H6152-70, and only before the TDC for the H6614-70

9 Preliminary Data Analysis Preliminary analysis only consists of the first 60,000 events of 7e5 events taken. At each Setting, evaluate the relative gain of the PMT and timing resolution; map both as a function of setting: when the sensor is rotated to a different θ, the LED does not rotate with the sensor. The timing data for each θ is normalized to (0 T, 0 ). results are sensitive to interval of integration of fadc signals timing resolution determined from the difference between the PMT time and trigger time.

fadc Spectra 10 H6614-70 assembly Signal height is averaged over 60,000 events in the run Average pedestal is determined from dark current runs and for each run between 0 and 40 time units All bins above the pedestal are integrated in a sum (average-pulse area) Average pedestal number of bins integrated is subtracted from the sum

fadc Pedestal 11 H6614-70 assembly fadc Pedestal determined for each run taken (over four days) In general the pedestal is fairly stable at a level much better than 1%

R6614-70 Timing Resolution vs Angle 12 Early in the measurements, it was seen that the timing resolution worsened with PMT angle. At 0 T, it s clear the amplitude decreases at larger angles, which is caused by a loss of collected light; the timing resolution also worsens. There was no easy way to rotate the LED fiber with the PMT; timing results were scaled based on the results at 0.

H6614-70 Symmetry 13 Data were taken at a series of symmetric angles about 35 : θ= 35 and φ = 0 θ= -35 and φ = 0 θ= 35 and φ = 90 θ= 215 and φ = 0 The relative amplitudes compared to 0 for each field setting are higher No discernible difference is seen for ±35 and φ = 0 or 90

H6614-70 Symmetry 14 Data were taken at a series of symmetric angles about 35 : θ= 35 and φ = 0 θ= -35 and φ = 0 θ= 35 and φ = 90 θ= 215 and φ = 0 The relative resolutions compared to 0 for each field setting are worse No discernible difference is seen for ±35 and φ = 0 or 90

H6614-70 All Angles 15 Data were taken at a series of angles between 0 and 50 for magnetic fields up to 1.9 T Between 35 and 45 the relative amplitudes are approximately the same The analysis with full statistics should be able to determine if any difference actually exists.

16 H6614-70 All Angles Data were taken at a series of angles between 0 and 50 for magnetic fields up to 1.9 T The timing resolutions were scaled to account for the loss of light collection as the PMT was rotated wrt the LED source The resolutions at 35 and 40 are approximately the same Above 1.6 T, the resolutions significantly worsen The analysis with full statistics should be able to determine if any difference actually exists.

H6152-70 Test Conditions 17 At HV = 2.0 kv, compared to the H6614-70, a factor of 20x gain reduction is expected. The achieved timing resolution for the small PMT was considerably worse compared to the H6614-70 Some adjustments were made with limited success in improving the resolution: The amplitude on the pulse generator was changed from 7.0 V to 7.5 V The 20x preamp was placed right after the PMT, so the signal going to the fadc was also amplified A splitter used with the H6614-70 was removed from the electronics The distance between the PMT and LED source was decreased by a factor of two, though no improvement was seen.

H6152-70 All Angles 18 Data were taken at a series of angles between 0 and 40 for magnetic fields up to 1.4 T Between 30 and 40 the relative amplitudes are approximately the same It appears that at 330 (-30 ) that the relative amplitude is a bit better than +30.

H6152-70 All Angles 19 Data were taken at a series of angles between 0 and 40 for magnetic fields up to 1.4 T The timing resolutions were scaled to account for the loss of light collection as the PMT was rotated wrt the LED source The timing resolutions become progressively worse with field and angles above 10, and the timing peaks are fairly asymmetric

Summary 20 A set of measurements at various angles wrt a magnetic field with a range of field strengths were collected for three Hamamatsu PMTs with two of them being fine-mesh PMTs. Results for the R11102 are also available. The performance of the larger PMT (H6614-70) appears to meet our requirements for SoLID, though the results are based on only about 9% of the acquired data. The minimum value of the timing resolution appears to be directly related the amount of light collected. Analysis of the full data set is in progress. Performance of the smaller fine-mesh PMT at least regarding the timing resolution were considerably worse. The four times smaller active area for light collection may have been a cause.