Time and temperature instability of continuous-action radioluminescent emitters

Details Time and temperature instability of continuous-action radioluminescent emitters Time and temperature instability of continuous-action radioluminescent emitters

Jun 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976opmep..43...10s&link_type=abstract

(Optiko-Mekhanicheskaia Promyshlennost', vol. 43, June 1976, p. 10-13.) Soviet Journal of Optical Technology, vol. 43, June 1976

Physics

Continuous Radiation, Luminescence, Radiation Sources, Radioactive Decay, Stellar Models, Thermal Instability, Carbon 14, Copper, Radium 226, Solar Simulation, Strontium 90, Time Response, Zinc Sulfides

Scientific paper

A number of continuous-action radioluminescent radiation sources for monitoring the flux variations of stellar simulators have been tested. The temperature dependences of radiation sources on the basis of ZnS-Cu, activated by Sr-90; ZnS-Ag, activated by C-14; and ZnS-Cu, activated by Ra-226 were examined. The time instabilities of the same sources along with that of ZnS-Cu, activated by C-14 were also tested. It was shown that ZnS-Cu with Sr-90 and C-14 activators are the most suitable as monitors of simulator stability.

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