Cosmic Ray Helium Flux during the Period 1970-1972
Cosmic ray helium flux at the energy around 100 MeV/N was measured by four balloon flights in the summer during the period from 1970 to 1972 at Syowa Station, Antarctica, with the aid of scintillation counter telescopes. The observed helium intensity of 1972 at the energy of 100 MeV/N showed about 1...
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National Institute of Polar Research
1974
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Online Access: | https://doi.org/10.15094/00007745 https://doaj.org/article/a995e3d078b34e5fb379856c213c08a5 |
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fttriple:oai:gotriple.eu:oai:doaj.org/article:a995e3d078b34e5fb379856c213c08a5 2023-05-15T14:02:15+02:00 Cosmic Ray Helium Flux during the Period 1970-1972 Eiji TAMAI Takasuke SAKAI Nobuo NARITA Koichi OGURA Shinichi KOGAMI 1974-03-01 https://doi.org/10.15094/00007745 https://doaj.org/article/a995e3d078b34e5fb379856c213c08a5 en other eng National Institute of Polar Research doi:10.15094/00007745 0085-7289 2432-079X https://doaj.org/article/a995e3d078b34e5fb379856c213c08a5 undefined Antarctic Record, Iss 49, Pp 1-12 (1974) geo Journal Article https://vocabularies.coar-repositories.org/resource_types/c_6501/ 1974 fttriple https://doi.org/10.15094/00007745 2023-01-22T19:28:05Z Cosmic ray helium flux at the energy around 100 MeV/N was measured by four balloon flights in the summer during the period from 1970 to 1972 at Syowa Station, Antarctica, with the aid of scintillation counter telescopes. The observed helium intensity of 1972 at the energy of 100 MeV/N showed about 100% increase over that of 1970. This value seems to be consistent with the estimated values from the data obtained by Mt. Washington neutron monitor, balloons and satellites in other years. Also the absolute intensity of the present data seems to be 20-30 % higher than the value extrapolated from the data obtained by LEZNIAK and WEBBER in 1965-1968. Article in Journal/Newspaper Antarc* Antarctica Unknown Syowa Station |
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Open Polar |
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Unknown |
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fttriple |
language |
English |
topic |
geo |
spellingShingle |
geo Eiji TAMAI Takasuke SAKAI Nobuo NARITA Koichi OGURA Shinichi KOGAMI Cosmic Ray Helium Flux during the Period 1970-1972 |
topic_facet |
geo |
description |
Cosmic ray helium flux at the energy around 100 MeV/N was measured by four balloon flights in the summer during the period from 1970 to 1972 at Syowa Station, Antarctica, with the aid of scintillation counter telescopes. The observed helium intensity of 1972 at the energy of 100 MeV/N showed about 100% increase over that of 1970. This value seems to be consistent with the estimated values from the data obtained by Mt. Washington neutron monitor, balloons and satellites in other years. Also the absolute intensity of the present data seems to be 20-30 % higher than the value extrapolated from the data obtained by LEZNIAK and WEBBER in 1965-1968. |
format |
Article in Journal/Newspaper |
author |
Eiji TAMAI Takasuke SAKAI Nobuo NARITA Koichi OGURA Shinichi KOGAMI |
author_facet |
Eiji TAMAI Takasuke SAKAI Nobuo NARITA Koichi OGURA Shinichi KOGAMI |
author_sort |
Eiji TAMAI |
title |
Cosmic Ray Helium Flux during the Period 1970-1972 |
title_short |
Cosmic Ray Helium Flux during the Period 1970-1972 |
title_full |
Cosmic Ray Helium Flux during the Period 1970-1972 |
title_fullStr |
Cosmic Ray Helium Flux during the Period 1970-1972 |
title_full_unstemmed |
Cosmic Ray Helium Flux during the Period 1970-1972 |
title_sort |
cosmic ray helium flux during the period 1970-1972 |
publisher |
National Institute of Polar Research |
publishDate |
1974 |
url |
https://doi.org/10.15094/00007745 https://doaj.org/article/a995e3d078b34e5fb379856c213c08a5 |
geographic |
Syowa Station |
geographic_facet |
Syowa Station |
genre |
Antarc* Antarctica |
genre_facet |
Antarc* Antarctica |
op_source |
Antarctic Record, Iss 49, Pp 1-12 (1974) |
op_relation |
doi:10.15094/00007745 0085-7289 2432-079X https://doaj.org/article/a995e3d078b34e5fb379856c213c08a5 |
op_rights |
undefined |
op_doi |
https://doi.org/10.15094/00007745 |
_version_ |
1766272407891345408 |