TY - JOUR
T1 - Self-triggered image intensifier tube for high-resolution UHECR imaging detector
AU - Sasaki, M.
AU - Asaoka, Y.
AU - Jobashi, M.
PY - 2003/4/1
Y1 - 2003/4/1
N2 - The authors have developed a self-triggered image intensifier tube with high-resolution imaging capability. An image detected by a first image intensifier tube as an electrostatic lens with a photocathode diameter of 100 mm is separated by a half-mirror into a path for CCD readout (768 × 494 pixels) and a fast control to recognize and trigger the image. The proposed system provides both a high signal-to-noise ratio to improve single photoelectron detection and excellent spatial resolution between 207 and 240 μm rendering this device a potentially essential tool for high-energy physics and astrophysics experiments, as well as high-speed photography. When combined with a 1-arcmin resolution optical system with 50° field-of-view proposed by the present authors, the observation of ultra high-energy cosmic rays and high-energy neutrinos using this device is expected, leading to revolutionary progress in particle astrophysics as a complementary technique to traditional astronomical observations at multiple wavelengths.
AB - The authors have developed a self-triggered image intensifier tube with high-resolution imaging capability. An image detected by a first image intensifier tube as an electrostatic lens with a photocathode diameter of 100 mm is separated by a half-mirror into a path for CCD readout (768 × 494 pixels) and a fast control to recognize and trigger the image. The proposed system provides both a high signal-to-noise ratio to improve single photoelectron detection and excellent spatial resolution between 207 and 240 μm rendering this device a potentially essential tool for high-energy physics and astrophysics experiments, as well as high-speed photography. When combined with a 1-arcmin resolution optical system with 50° field-of-view proposed by the present authors, the observation of ultra high-energy cosmic rays and high-energy neutrinos using this device is expected, leading to revolutionary progress in particle astrophysics as a complementary technique to traditional astronomical observations at multiple wavelengths.
KW - CCD
KW - Fluorescence detection
KW - High signal-to-noise ratio
KW - Image intensifier
KW - Self-triggered
KW - Ultra high-energy cosmic ray
UR - http://www.scopus.com/inward/record.url?scp=0037390638&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=0037390638&partnerID=8YFLogxK
U2 - 10.1016/S0168-9002(03)00620-X
DO - 10.1016/S0168-9002(03)00620-X
M3 - Article
AN - SCOPUS:0037390638
SN - 0168-9002
VL - 501
SP - 359
EP - 366
JO - Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
JF - Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
IS - 2-3
ER -