1970年,1971年,1972年における銀河宇宙線中のヘリウム成分

玉井 英次, 境 孝祐, 成田 信男, 小倉 紘一, 湖上 晨一, Eiji TAMAI, Takasuke SAKAI, Nobuo NARITA, Koichi OGURA, Shinichi KOGAMI

doi:10.15094/00007745

書誌事項

タイトル別名

1970ネン 1971ネン 1972ネンニオケルギンガウチュウセンチュウノヘリウムセイブン
Cosmic Ray Helium Flux during the Period 1970-1972

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説明

type:P(論文)

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.

収録刊行物

南極資料

南極資料 49 1-12, 1974-03

国立極地研究所

詳細情報詳細情報について

CRID: 1390009224683230592

NII論文ID: 120005508686; 110001182347

NII書誌ID: AN00181831

ISSN: 00857289

DOI: 10.15094/00007745

NDL書誌ID: 7601056

Web Site: http://id.nii.ac.jp/1291/00007745/; http://id.ndl.go.jp/bib/7601056; https://ndlsearch.ndl.go.jp/books/R000000004-I7601056

本文言語コード: ja

資料種別: departmental bulletin paper

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