MiniPrototype SinglesCosmicRuns 2008

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Goal

Use singles Cosmic events to measure rate differences between Metalica and Plastica

Apparatus

  • Plastica and Metalica are stacked on top of each other. High Voltage and ionization gas are connected in parallel.
  • A discriminator is connector to the amplified output (an on board preamp and the VPI Post amp) of sense wire 4.
  • The discriminator output is connected to a VME scaler.

Proposed Tests

  1. Measure the singles rate as a function of DC high voltage
  2. Measure the singles rate as a function of Discriminator Threshold


30-04-2008

The DC high voltage is on. The DC outputs of Plastika and Metalica from sense wire 3 are connected to the Model 777 Octal Variable Gain Amplifier.

HV settings
Wire Volts
Sense 1700
Field -800
Guard 800


Scope picture below shows the Noise level on the DC measured in infinite persist time mode.
Noise level of plastika and metalica using gain amplifier 30-04-2008.png

Scope pictures representing the cosmic signals from Plastika and Metalica(Amplifier is connected)

  • Plastika

Plastika output wire 3 amplifier HV on 1800V 30-04-2008 1.png
Plastika output wire 3 amplifier HV on 1800V 30-04-2008 2.png
Plastika output wire 3 amplifier HV on 1800V 30-04-2008 3.png

  • Metalica

Metalica output wire 3 amplifier HV on 1800V 30-04-2008 1.png
Metalica output wire 3 amplifier HV on 1800V 30-04-2008 2.png
Metalica output wire 3 amplifier HV on 1800V 30-04-2008 3.png

OUTPUTS FROM DISCRIMINATOR

Discriminator Threshold=450MV

Plastika output wire 3 amplifier discriminator HV on 1800V 30-04-2008 1.png

Rate -vs- Discriminator Threshold

Gas is ArCo2 . 75/25 mixture
HV settings
Wire Volts
Sense 1700
Field -850
Guard 850


Threshold (mV) Metalica (Events/hr) plastica (Events/hr)
300 [math]\pm \sqrt{\frac{16.5}{2153324}}[/math] [math]\pm \sqrt{\frac{16.5}{56758}}[/math]
300 [math]\pm \sqrt{\frac{1.1439}{378}}[/math] [math]\pm \sqrt{\frac{1.1439}{3746}}[/math]




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