view Abstract Citations (2) References Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS Temperature Effects in Photomultipliers. Young, Andrew T. Abstract The effect of temperature changes on the spectral response curves of RCA 1P21, EMI 6256 and 9558, and Farnsworth FW-1 18 photomultipliers has been measured for two tubes of each type. The cathodes are respectively S-4 (Sb-Cs), S-13 (Sb-Cs), S-20 (Sb-Na-K-Cs), and S-1 (Ag-O-Cs). All but the FW-1 18 have Sb-Cs dynode surfaces. Cooling from room temperature to dry-ice temperature causes changes in relative spectral response of the order of 10% or less for the Sb-Cs cathodes for A~5000 A, for the S-20 cathode for x~6250, and for the S-1 cathode over at least the range from 6250 to 10 000 A. At A=7300, the S-20 cathode loses about 30% of its normal sensitivity when it is refrigerated. The data are consistent with a temperature coefficient of -0.04%/0C per stage for the Sb-Cs dynodes. The Sb-Cs cathodes lose a large fraction of their sensitivity for A> 5000 A when they are refrigerated. This loss is more than enough to account for the discrepancy between observed B - V colors of stars and colors computed from stellar atmosphere theory. The coefficient of the temperature effect between 5000 and 6000A is 1.12x10-5 mag./0Q/A. This typically requires a temperature stabilization of one or two degrees if a 1P21 is required to carry a color zero point in this part of the spectrum with an accuracy of 1%. Publication: The Astronomical Journal Pub Date: June 1962 DOI: 10.1086/108726 Bibcode: 1962AJ.....67..286Y full text sources ADS |
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