Difference between revisions of "Preamp 4: Comparison of cosmic data with original preamp"
From GlueXWiki
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− | The pictures below show ADC amplitude histograms for cosmic ray data with 50/50 Ar/CO2 gas mixture (the maximum ADC amplitude for each event contributes one entry for that amplitude in the histogram). | + | The pictures below show ADC amplitude histograms for cosmic ray data with 50/50 Ar/CO2 gas mixture (the maximum ADC amplitude for each event contributes one entry for that amplitude in the histogram) and energy spectra obtained by integrating the amplitude histograms. |
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− | 2050V | + | 2050V - cosmics - amplitude, old (left) and new (right) preamps |
{| border="1" cellpadding="2" | {| border="1" cellpadding="2" | ||
|width="415pt"|[[Image:cosmic_amplitude_2050V_old_preamp.jpg|thumb|none|400px|old preamp, cosmics, 50/50 Ar/CO2, 2050V]] | |width="415pt"|[[Image:cosmic_amplitude_2050V_old_preamp.jpg|thumb|none|400px|old preamp, cosmics, 50/50 Ar/CO2, 2050V]] | ||
|width="415pt"|[[Image:cosmic_amplitude_2050V_preamp4.jpg|thumb|none|400px|new preamp, cosmics, 50/50 Ar/CO2, 2050V]] | |width="415pt"|[[Image:cosmic_amplitude_2050V_preamp4.jpg|thumb|none|400px|new preamp, cosmics, 50/50 Ar/CO2, 2050V]] | ||
+ | |} | ||
+ | |||
+ | 2050V - cosmics - energy, old (left) and new (right) preamps | ||
+ | {| border="1" cellpadding="2" | ||
+ | |width="415pt"|[[Image:cosmic_energy_2050V_old_preamp.jpg|thumb|none|400px|old preamp, cosmics, energy, 50/50 Ar/CO2, 2050V]] | ||
+ | |width="415pt"|[[Image:cosmic_energy_2050V_preamp4.jpg|thumb|none|400px|new preamp, cosmics, energy, 50/50 Ar/CO2, 2050V]] | ||
|} | |} | ||
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− | 2100V - the new preamp is saturating at this voltage | + | 2100V - cosmics - amplitude, old (left) and new (right) preamps - the new preamp is saturating at this voltage |
{| border="1" cellpadding="2" | {| border="1" cellpadding="2" | ||
|width="415pt"|[[Image:cosmic_amplitude_2100V_old_preamp.jpg|thumb|none|400px|old preamp, cosmics, 50/50 Ar/CO2, 2100V]] | |width="415pt"|[[Image:cosmic_amplitude_2100V_old_preamp.jpg|thumb|none|400px|old preamp, cosmics, 50/50 Ar/CO2, 2100V]] | ||
|width="415pt"|[[Image:cosmic_amplitude_2100V_preamp4.jpg|thumb|none|400px|new preamp, cosmics, 50/50 Ar/CO2, 2100V]] | |width="415pt"|[[Image:cosmic_amplitude_2100V_preamp4.jpg|thumb|none|400px|new preamp, cosmics, 50/50 Ar/CO2, 2100V]] | ||
|} | |} |
Latest revision as of 13:14, 13 June 2010
The pictures below show ADC amplitude histograms for cosmic ray data with 50/50 Ar/CO2 gas mixture (the maximum ADC amplitude for each event contributes one entry for that amplitude in the histogram) and energy spectra obtained by integrating the amplitude histograms.
These compare data taken using the old and new preamps - the "old" preamp is the original one and the "new" preamp is Preamp4, described in Table 2 row 2 of GlueX-doc-1364 and labelled 27.
2050V - cosmics - amplitude, old (left) and new (right) preamps
2050V - cosmics - energy, old (left) and new (right) preamps
2100V - cosmics - amplitude, old (left) and new (right) preamps - the new preamp is saturating at this voltage