Difference between revisions of "New HVB"

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[[Image:newHVB_cosmics_amp_2050V.jpg|thumb|400px|New preamp and HVB - max amplitude histo for cosmics at 2050V ]]
 
[[Image:newHVB_cosmics_amp_2050V.jpg|thumb|400px|New preamp and HVB - max amplitude histo for cosmics at 2050V ]]
 
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<br>Fe55 with premixed 50/50 Ar/CO<sub>2</sub>, New preamp and new HVB, ADC half-range, for a range of HV<br>
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[[Image:newHVB_Fe55_amp.jpg|thumb|400px|New preamp and HVB - max amplitude histo for 55Fe ]]
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The beginnings of a new HV efficiency plot
 
The beginnings of a new HV efficiency plot

Revision as of 10:06, 7 September 2010

Max amplitude histograms for cosmics at 2100V with 50/50 Ar/CO2
Left: new preamp and new HVB, ADC half-range; right: old preamp and HVB, ADC full-range
Purple: untracked, blue: tracked (less of this with old preamp because of 2 dead central channels)

New preamp and HVB - max amplitude histo for cosmics at 2100V
Old preamp and HVB - max amplitude histo for cosmics at 2100V


Cosmics with premixed 50/50 Ar/CO2, New preamp and new HVB, ADC half-range

Left: 2000V; Right: 2050V - NB expanded x-axis

New preamp and HVB - max amplitude histo for cosmics at 2000V
New preamp and HVB - max amplitude histo for cosmics at 2050V



Fe55 with premixed 50/50 Ar/CO2, New preamp and new HVB, ADC half-range, for a range of HV

New preamp and HVB - max amplitude histo for 55Fe


The beginnings of a new HV efficiency plot

New preamp and HVB - tracked/triggers with HV for software threshold=5

Scope traces for premixed 50/50 Ar/CO2

Fe55 at 2100V (50mV/div 100ns/div)
Cosmics at 2100V (50mV/div 100ns/div)