UV-sensitivity of a gas proportional counter
Technical Report
·
OSTI ID:6153770
This report is an account of the investigation of UV-sensitivity of a gas proportional counter. The detector used in this investigation has been developed for the observation of low-energy cosmic X-rays; i.e. 0.05-2.0 keV. A major source of background at very low energies (<0.2 keV) is due to the sensitivity of the counter to UV-radiation of stellar origin in the wavelength band 1600-3000 A. The purpose of this investigation is to establish in a quantitive way the parameters governing the UV-sensitivity of a gas proportional detector.
- Research Organization:
- Huygens Lab., Leiden (Netherlands)
- OSTI ID:
- 6153770
- Report Number(s):
- PB-83-161620
- Country of Publication:
- United States
- Language:
- English
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Related Subjects
440101* -- Radiation Instrumentation-- General Detectors or Monitors & Radiometric Instruments
46 INSTRUMENTATION RELATED TO NUCLEAR SCIENCE AND TECHNOLOGY
ELECTROMAGNETIC RADIATION
MEASURING INSTRUMENTS
PERFORMANCE
PROPORTIONAL COUNTERS
RADIATION DETECTORS
RADIATIONS
SENSITIVITY
ULTRAVIOLET RADIATION
46 INSTRUMENTATION RELATED TO NUCLEAR SCIENCE AND TECHNOLOGY
ELECTROMAGNETIC RADIATION
MEASURING INSTRUMENTS
PERFORMANCE
PROPORTIONAL COUNTERS
RADIATION DETECTORS
RADIATIONS
SENSITIVITY
ULTRAVIOLET RADIATION