Paper
28 July 2000 Development challenges for the GALEX UV sealed tube detectors
Darrel L. Doliber, Joseph M. Stock, Sharon R. Jelinsky, James M. Malloy, Patrick N. Jelinsky, Oswald H. W. Siegmund, Jeffrey S. Hull
Author Affiliations +
Abstract
We will describe the development of the design and processing of the near ultraviolet (NUV, 1800 - 3000 angstroms) and far ultraviolet (FUV, 1350 - 1800 angstroms) sealed tube microchannel plate cross delay line detectors for the NASA Galaxy Evolution Explorer Satellite. Specifications for the two detector systems for GALEX define a large 65 mm diameter circular format, with high spatial resolution (< 30 micrometers FWHM, approximately 2200 X 2200 resolution elements) and good image linearity (+/- 50 micrometers ), low diffuse background rates of < 1 event cm-1 sec-1, and event processing rates of > 2 X 105 events sec-1. We have implemented a detector design using a microchannel plate Z stack to amplify the signals detected by the photocathodes, and a cross delay line anode to provide the photon event position encoding. These detectors were produced using a new sealed tube production facility installed at the Space Sciences Laboratory, University of California, Berkeley.
© (2000) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Darrel L. Doliber, Joseph M. Stock, Sharon R. Jelinsky, James M. Malloy, Patrick N. Jelinsky, Oswald H. W. Siegmund, and Jeffrey S. Hull "Development challenges for the GALEX UV sealed tube detectors", Proc. SPIE 4013, UV, Optical, and IR Space Telescopes and Instruments, (28 July 2000); https://doi.org/10.1117/12.394022
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Cited by 4 scholarly publications.
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KEYWORDS
Sensors

Microchannel plates

Ultraviolet radiation

Signal detection

Magnesium fluoride

Near ultraviolet

Computer programming

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