DocumentCode
1224339
Title
High amplitude events in microchannel plates
Author
Siegmund, O.H.W. ; Lammert, P. ; Vallerga, J.V. ; Priedhorsky, W. ; Smith, B.W.
Author_Institution
Space Sci. Lab., California Univ., Berkeley, CA, USA
Volume
36
Issue
1
fYear
1989
fDate
2/1/1989 12:00:00 AM
Firstpage
830
Lastpage
835
Abstract
Measurements have been made to determine the characteristics of high-amplitude events in microchannel plates (MCPs). The background-pulse-amplitude spectrum is found to extend to >30x to MCP modal gain. The majority of the background events are initiated by 40K beta decay in the MCP glass. However, up to 40% of the events are due to cosmic rays. Comparison of background pulse-amplitude spectra for horizontal and vertical MCP orientations suggests that the largest events are predominantly cosmic-ray-induced. Anticoincidence measurements confirm this result. A model describing the 40K beta decay and cosmic-ray interactions in the MCP predicts spectra in accord with these observations. The response of MCPs subjected to simultaneous multiphoton input was also determined, showing that pulse amplitudes many times the modal gain are possible event though the response becomes nonlinear at high amplitudes
Keywords
electron multipliers; image intensifiers; position sensitive particle detectors; 40K beta decay; background-pulse-amplitude spectrum; cosmic rays; high-amplitude events; microchannel plates; modal gain; multiphoton input; Blades; Cosmic rays; Detectors; Feedback; Glass; Laboratories; Microchannel; Postal services; Predictive models; Pulse shaping methods;
fLanguage
English
Journal_Title
Nuclear Science, IEEE Transactions on
Publisher
ieee
ISSN
0018-9499
Type
jour
DOI
10.1109/23.34560
Filename
34560
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