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- W2010110180 abstract "An upper limit on the continuous emission of 2.22-MeV photons (neutron-proton capture $ensuremath{gamma}$ rays) from the sun has been determined from day and night balloon flights in May and June of 1967, from Palestine, Texas at an atmospheric depth of ensuremath{sim}3.8 g/${mathrm{cm}}^{2}$. The experimental apparatus consisted of a 3 in.ifmmodetimeselsetexttimesfi{}3 in. CsI(Tl) $ensuremath{gamma}$-ray spectrometer and airborne telemetry to transmit the pulse-height distribution to the receiving station, where it was recorded on magnetic tape for later analysis by a laboratory multichannel analyzer. On-board calibration sources giving lines below 2.22 MeV were always present in the spectrum and allowed a continual check on the stability of the apparatus. Comparison of the day and night average counting rates as well as the daytime absence of any line leads to a null result for any statistically significant solar flux of 2.22-MeV photons. Our resulting upper-limit flux is comparable with the value of 5ifmmodetimeselsetexttimesfi{}${10}^{ensuremath{-}3}$ photon ${mathrm{cm}}^{ensuremath{-}2}$ ${mathrm{sec}}^{ensuremath{-}1}$ determined from the Ranger-3 experiment in January 1962 at a considerably different phase of the solar cycle." @default.
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- W2010110180 date "1968-02-25" @default.
- W2010110180 modified "2023-09-23" @default.
- W2010110180 title "Limit on the Continuous Solar Flux of the 2.22-MeV Neutron-Proton Capture Gamma Ray" @default.
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- W2010110180 doi "https://doi.org/10.1103/physrev.166.1299" @default.
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