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Characterization of Position-Sensitive Microchannel Plate DetectorsMicrochannel plate (MCP) position-sensitive detectors (PSDs) are now commonly used in a wide range of areas including, imaging spectroscopy, mass spectrometry, electron spectroscopy, astronomy, and atomic collision studies. The particular style of detector we use is composed of a pair of microchannel plates stacked in a chevron configuration above a resistive anode. Particles, or photons, striking the front MCP may start a cascade of secondary electrons. As the MCP's each have a large gain, a burst of 106-107 electrons will impact the resistive anode. By comparing the currents to the four corners of the anode it is possible to determine the position of impact of the initial particle or photon. With the addition of a few components to the bias network it is also possible to use these devices for highly accurate timing. In order to use these devices for quantitative measurements we carried out a fairly comprehensive study of their properties focusing on, the effect of MCP bias, absolute detection efficiency, and the effect of the particle impact angle. We still routinely conduct such tests on the PSDs that we use for our experiments. Further details can be found in Gao et al., Rev. Sci. Inst. 55, 1756 (1984). A higher spatial resolution study is described in Gao et al., Rev. Sci. Inst. 59, 1954 (1988). |
| One simple method of determining the flux of oxygen atoms employs the use of a catalytic probe. This method relies on measuring the temperature rise due to recombination of oxygen atoms on a silver oxide coated probe surface. Sometimes, as in the present design, a second reference probe, identical to the catalytic probe but uncoated, is used to compensate for temperature changes unrelated to atomic oxygen recombination. Variations of this general concept have been widely used with some quantitative success. The specific design we are developing will hopefully overcome some of the shortcomings of previous implementations. Our prototype device, shown to the right, was built by one of our summer students, Brian White. |
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Physics and Astronomy | Rice Quantum Institute| Rice Space Institute
Updated March 19, 2001