DocumentCode
1138058
Title
Optical transmission of low-level DC, slowly varying and pulsed current signals using the optically coupled current mirror architecture
Author
Camin, Daniel V. ; Grassi, Valerio ; Levati, Federico
Author_Institution
Phys. Dept., Univ. of Milano, Milan, Italy
Volume
51
Issue
5
fYear
2004
Firstpage
1948
Lastpage
1952
Abstract
The optically coupled current mirror (OCCM) is a novel optoelectronic architecture that replicates at ground potential a current flowing in an isolated conductor. The mirroring action is done without need to bring any power to the potential of the conductor where the current flows, as its input stage is completely passive. This feature is particularly important when the conductor is at high voltage (HV), a typical case being the photomultiplier tubes (PMTs) biased with positive HV, or when the number of channels is very large as it is the case of many particle physics experiments. The OCCM has been used to equip the two prototype telescopes, each one comprising 440 PMTs, of the ultra-high-energy cosmic-ray experiment Pierre Auger. Despite that the PMT´s anodes were at HV, the DC or slowly varying component of the anode current was measured with high resolution, clearly revealing the presence of faint stars, planets, and other similar objects which determine the sky background light. In this paper we describe the principle of operation of the OCCM and its application to the measurement of the anode current of PMTs biased with cathode grounded, as well as the first results obtained with the OCCM on linear transmission of 2-μs-width pulses, via fiber optics.
Keywords
astronomical telescopes; cosmic ray apparatus; current mirrors; nuclear electronics; optical fibres; optoelectronic devices; photomultipliers; planets; stars; analog-signal transmission; anode current; faint stars; fiber optics; galvanically isolated amplifier; ground potential; isolated conductor; linear transmission; low-level DC; mirroring action; optical current mirror; optical transmission; optically coupled current mirror architecture; optoelectronic architecture; passive input stage; photomultiplier tubes; planets; positive high voltage; prototype telescopes; pulsed current signals; sky background light; slowly varying component; slowly varying signals; ultra-high-energy cosmic-ray experiment; Anodes; Conductors; Current measurement; Extraterrestrial measurements; Mirrors; Optical coupling; Optical pulses; Photomultipliers; Pulse measurements; Voltage; Analog-signal transmission; galvanically isolated amplifier; optical current mirror; passive input stage;
fLanguage
English
Journal_Title
Nuclear Science, IEEE Transactions on
Publisher
ieee
ISSN
0018-9499
Type
jour
DOI
10.1109/TNS.2004.834710
Filename
1344266
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