Published May 30, 2001 | Version v1
Journal article

Electronics for the KLYPVE Detector

  • 1. D.V. Skobeltsyn Institute of Nuclear Physics of Moscow State University, Moscow (Russian Federation)
  • 2. Department of Applied Research of Moscow State University, Moscow (Russian Federation)
  • 3. Facultad de Ciencias Fisico Matematicas, Universidad de Puebla, Puebla (Mexico)
  • 4. University of New Mexico, Albuquerque, New Mexico (United States)
  • 5. Rocket Space Corporation 'ENERGIA', Space Regatta Consortium, Moscow Region, Korolev (Russian Federation)
  • 6. Instituto de Fisica y Matematicas, Universidad Michoacana, Morelia, Michoacan (Mexico)
  • 7. Physics Department, Cinvestav, D. F. (Mexico)

Description

The KLYPVE optical detector on board the Russian segment of the ISS will observe 10 thousand km2 of the Earth atmosphere registering the extremely high energy cosmic ray (EHECR) particles producing fluorescent tracks in the atmosphere. In this article the design of the detector is presented, including: the Fresnel type mirror of 10 m2 area, the PMT retina of 2500 pixels, the pixel electronics, the data acquisition electronics, and the trigger system. The detector design is suited to conditions of the space experiment (wide range of temperature, short day-night cycle etc). The problem of selection of rare EHECR events in the presence of high intensity background light is discussed

Additional details

Identifiers

Publishing Information

Journal Title
AIP Conference Proceedings
Journal Volume
566
Journal Issue
1
Journal Page Range
p. 76-90
ISSN
0094-243X
CODEN
APCPCS

Conference

Title
International workshop on observing ultra high energy cosmic rays from space and earth
Dates
9-12 Aug 2000
Place
Metepec, Puebla (Mexico)

Optional Information

Notes
(c) 2001 American Institute of Physics.