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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Main Authors: Eiji TAMAI, Takasuke SAKAI, Nobuo NARITA, Koichi OGURA, Shinichi KOGAMI
Format: Article in Journal/Newspaper
Language:English
Published: National Institute of Polar Research 1974
Subjects:
geo
Online Access:https://doi.org/10.15094/00007745
https://doaj.org/article/a995e3d078b34e5fb379856c213c08a5
id fttriple:oai:gotriple.eu:oai:doaj.org/article:a995e3d078b34e5fb379856c213c08a5
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spelling 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
institution Open Polar
collection Unknown
op_collection_id 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
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