Difference between revisions of "09-08-2016"
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+ | =End of Run summary= | ||
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+ | #The back wall was a source of photons that can be reduced best with blinders | ||
+ | #The ToF spectrum needs better separation between gamma flash and neutrons, Move detectors back? | ||
+ | #The tunnel of love improved D150's shielding | ||
+ | #Opening the collimator slit fully caused gamma flash to appear close to the neutron ToF | ||
=No target run= | =No target run= |
Revision as of 23:16, 8 September 2016
Study forward detector gamma flash
with Pb curtains
Shielding & Beam dump impact on gamma flash
Tuning impact on gamma flash
We set up a veto to create a signal that represented the second peak of the gamma flash in D270 & others. A veto pulse was created for the LED to prevent it from outputing a logic high during the first 20 ns after the beam pulse.
Run # | D90 n Rate (Counts/pulse) | Configuration |
5309 | 11.1 MeV , 2 ns pulse width , 300 mA , 200 Hz , Accelerator side collimator open to 0.2563 cm, Cell side collimator OPEN to 2 cm , radiator 3/4" IN , Target is EMPTY , D30 HV changed -1550V, All other detectors at -1700 V, removed pair spectrometer magnet, poly, and stand,Removed 3rd collimator wall, D30 has NO thick lead curtain, Veto OUT40px | |
5310 | 11.1 MeV , 2 ns pulse width , 300 mA , 200 Hz , Accelerator side collimator open to 0.2563 cm, Cell side collimator OPEN to 2 cm , radiator 3/4" IN , Target is EMPTY , D30 HV changed -1550V, All other detectors at -1700 V, removed pair spectrometer magnet, poly, and stand,Removed 3rd collimator wall, D30 has NO thick lead curtain, Veto IN40px |
Thorium plate rates.
End of Run summary
- The back wall was a source of photons that can be reduced best with blinders
- The ToF spectrum needs better separation between gamma flash and neutrons, Move detectors back?
- The tunnel of love improved D150's shielding
- Opening the collimator slit fully caused gamma flash to appear close to the neutron ToF