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1“... of the cosmic ray meson component, recommended by DORMAN and other authors, were examined on the basis...”
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2“...Cosmic-ray intensities have been measured along a constant ship-route between Japan...”
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3“...Cosmic ray helium flux at the energy around 100 MeV/N was measured by four balloon flights...”
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4“...Using 5-minute data of cosmic-ray neutron and meson intensities observed at Syowa Station...”
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7by Masahiro KODAMA“...-rays carried out at Syowa Station, Antarctica during 1971-1973. Dual sets of sounding rockets were...”
Published 1975
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8“..., the atmospheric particulate matter at Syowa Station, Antarctica was characterized by X-ray fluorescence...”
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9“... newly installed X-ray fluorescence analyzer (RIGAKURIX3000) at the National Institute of Polar Research...”
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10“...), using an X-ray fluorescence analyzer (RIGAKU RIX3000) at the National Institute of Polar Research...”
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12“..., are summarized. The analyses were performed by means of an X-ray fluorescence analyzer RIGAKU RIX3000 with a dual...”
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13“... of an X-ray fluorescnece analyzer RIGAKU RIX3000 at the National Institute of Polar Research...”
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14“...To explore the solar cycle dependence of the latitude effect of cosmic ray intensity, measurements...”
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15REPORT OF COSMIC-RAY NEUTRON OBSERVATION IN THE 8TH JAPANESE ANTARCTIC RESEARCH EXPEDITION 1967-1968“...At Syowa Station, Antarctica, the cosmic-ray neutron observation was made, at the initial stage...”
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16by Hiromu Suzuki“...-area characteristics of bremsstrahlung X-rays radiated from energetic precipitated electrons. PPB No.6...”
Published 1996
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17by Tadao MAKINO“...The fourth cosmic ray latitude survey in nucleonic and meson components was carried out on M...”
Published 1962
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18by Koichi OGURA“... the period of 1968-1970. The latitude dependence of cosmic-ray intensities was observed aboard the icebreaker...”
Published 1971
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19“..., and rare earth elements in silicate rocks by X-ray fluorescence spectrometry (RIX3000) at the National...”
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20“...From February 1968 to January 1969, cosmic ray nucleonic component was observed at Syowa Station...”
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