Difference between revisions of "Preamp 3"
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|width="415pt"|[[Image:new_preamp_cosmics_2100V.jpg|thumb|none|400px|new preamp, cosmic rays, 50/50 Ar/CO2, 2100V]] | |width="415pt"|[[Image:new_preamp_cosmics_2100V.jpg|thumb|none|400px|new preamp, cosmic rays, 50/50 Ar/CO2, 2100V]] | ||
+ | |width="415pt"|[[Image:new_preamp_cosmics_2100V_longer.jpg|thumb|none|400px|new preamp, cosmic rays, 50/50 Ar/CO2, 2100V (as left, for longer) ]] | ||
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|width="415pt"|[[Image:old_preamp_cosmics_2100V.jpg|thumb|none|400px|old preamp, cosmic rays, 50/50 Ar/CO2, 2100V]] | |width="415pt"|[[Image:old_preamp_cosmics_2100V.jpg|thumb|none|400px|old preamp, cosmic rays, 50/50 Ar/CO2, 2100V]] | ||
+ | |width="415pt"|[[Image:old_preamp_cosmics_2100V_longer.jpg|thumb|none|400px|old preamp, cosmic rays, 50/50 Ar/CO2, 2100V (as left, for longer) ]] | ||
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Revision as of 13:15, 16 April 2010
The pictures below show oscilloscope traces for gas mixture 50/50 Ar/CO2.
The following were obtained with increased anode voltages.