@article{oai:jaxa.repo.nii.ac.jp:00031886,
 author = {中川, 重雄 and NAKAGAWA, Shigeo},
 issue = {3_B},
 journal = {東京大学宇宙航空研究所報告},
 month = {Sep},
 note = {Using rocket-borne solid state detectors, the intensity distribution of proton and electron fluxes up to nearely 100km was obtained. The proton flux in the energy range 20 to 60 MeV is very weak and its altitude variation was not accurately measured. The average intensity obtained was 0.007 ± 0.0025 (cm^2 sec str)^<-1>. The electron flux above 470 keV energy increased with the rocket height and it seems to indicate the prepitation of electrons from the radiation belt. The presence of deuterons, tritons and α-particles in the inner radiation belt according to the disintegration of oxygen nuclei by trapped protons and the relation of these secondary particles emitted from the belt with the low energy deuteron flux at the top of the atmosphere which was observed in the nuclear emulsion stack exposed to cosmic rays by the balloon, are discussed., 資料番号: SA0124945000},
 pages = {1269--1274},
 title = {L-3ロケットによる粒子線の測定},
 volume = {2},
 year = {1966}
}