Tags: astrophysics group, detection efficiencies, double delay, experimental astrophysics, field images, fixed pattern noise, fuse detectors, high spatial resolution, jeffrey hull, joseph stock, microchannel plate, microchannel plates, narrow pulse, pulse height distributions, resolution elements, space sciences laboratory, ultraviolet spectroscopic explorer, ultraviolet spectroscopy, university of california berkeley, university of california berkeley ca,
Performance of the double delay line microchannel
plate detectors for the Far Ultraviolet Spectroscopic Explorer
Oswald H.W. Siegmund, Mark Gummin, Geoffrey Gaines, Giampiero Naletto,
Joseph Stock, Richard Raffanti, Jeffrey Hull, Robert Abiad, Ted Rodriguez-Bell,
Tony Magoncelli, Patrick Jelinsky, William Donakowski, and Karl Kromer
Experimental Astrophysics Group
Space Sciences Laboratory
University of California
Berkeley, CA 94720
Phone 510-642-0895, Fax 510-643-9729
email, ossy@ssl.berkeley.edu
ABSTRACT
The microchannel plate, delay line, detectors developed for the Far Ultraviolet Spectroscopic Explorer1
mission to be launched in 1998 are described. The two FUSE detectors have a large format (·184mm x 10mm
split into two 88.5 x 10mm segments), with high spatial resolution (9000 x 200
resolution elements) and good linearity (±25µm), high image stability, and counting rates in excess of 4 x 104
events sec-1. KBr opaque photocathodes have been employed to provide quantum detection efficiencies of 30-
40% in the 900 - 1200Å range. Microchannel plates with 10µm pores and an 80:1 pore length to diameter ratio,
with a 95mm x 20mm format have been used in a Z stack configuration to provide the photon amplification (gain
· 2 x 107). These show narrow pulse height distributions (