Has anyone measured effect of temperature on response of scintillators in Cosmic Watch muon detectors?

Yes — there have been a few measurements and discussions of temperature effects in CosmicWatch-style scintillator/SiPM muon detectors, though not many formal dedicated studies.

The main effect is usually not the plastic scintillator itself, but the SiPM gain drift with temperature.

Key findings:

  • The CosmicWatch detector uses a SensL SiPM whose breakdown voltage changes with temperature by about 21.5 mV/°C. With fixed bias voltage, this changes gain and therefore trigger efficiency.
  • One recent analysis found roughly a 4.4% gain variation over an 11.7 °C detector temperature range. They observed detector temperature correlated with apparent muon rate at r = +0.49. After correcting for detector temperature, most of the apparent atmospheric-temperature correlation disappeared.
  • The newer CosmicWatch v3 documentation explicitly mentions logging temperature so corrections for “temperature-dependent gain shifts” can be applied, although the correction is apparently not yet implemented in firmware/software.
  • Another portable scintillator coincidence detector study found little dependence of coincidence count rate on modest temperature changes, while noting that single-channel SiPM rates are more temperature-sensitive.

Practically, for CosmicWatch detectors:

  • Single detector count rates can drift noticeably with temperature because threshold crossing depends on SiPM gain.
  • Coincidence setups are much more stable.
  • The scintillator light yield itself changes only weakly over normal room/outdoor temperatures.
  • Most temperature dependence comes from:
    • SiPM gain
    • dark count rate
    • discriminator threshold interaction

Typical magnitude:

  • Roughly a few percent over ~10 °C is plausible for uncorrected systems.

If you are doing precision muon flux work with your coincidence setup, useful approaches are:

  • log onboard temperature continuously
  • keep detector temperature stable
  • use coincidence triggering
  • or implement active bias compensation:

Vbias(T) = V0 + k(T – T0)

where k is about +21.5 mV/°C for the SensL device.

The original and the paper The Physics Behind the CosmicWatch Desktop Muon Detectors discuss atmospheric studies but only lightly touch on thermal effects.

By Admin

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