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SUMMARY:Characteristics and Performances of the electronics for the fluore
 scence detectors of the Telescope Array experiment
DTSTART;VALUE=DATE-TIME:20070706T194500Z
DTEND;VALUE=DATE-TIME:20070706T194500Z
DTSTAMP;VALUE=DATE-TIME:20260417T052327Z
UID:indico-contribution-790@cern.ch
DESCRIPTION:Speakers: Dr. TOKUNO\, Hisao (Institute for Cosmic Ray Researc
 h\, The University of Tokyo)\nThe three stations of the Telescope Array fl
 uorescence detectors (FDs)\ncontain 12 telescopes each\, and each of the t
 elescopes has a 256 pixel\nPMT camera with a field of view of 18 degree x 
 16 degrees.\nThe fluorescence signals of each pixel are digitized with the
 ir\nwaveforms by the Signal Digitizer/Finder modules (SDFs). The signal\na
 lerts from the SDFs are send to the Track Finder modules (TF) to\ngenerate
  first trigger signals for air shower events. When a shower\ntrack image i
 s found in one camera\, the Central Trigger Distributor\n(CTD) module send
 s the final trigger signal to all the telescopes to\nstore their data. Her
 e we will describe the characteristic features\nand performances of the el
 ectronics\, which are developed and measured\nthrough laboratory tests and
  actual fluorescence light measurements.\n\nhttps://indico.nucleares.unam.
 mx/event/4/session/39/contribution/790
LOCATION:Merida\, Mexico Regency (Hyatt)
URL:https://indico.nucleares.unam.mx/event/4/session/39/contribution/790
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