From Nobeyama Radio Observatory to the international project ALMA —Evolution of millimeter and submillimeter wave astronomy in Japan

From Nobeyama Radio Observatory to the international project ALMA —Evolution of millimeter and submillimeter wave astronomy in Japan—

Published:2022-10-11 Issue:8 Volume:98 Page:439-469
ISSN:0386-2208
Container-title:Proceedings of the Japan Academy, Series B
language:en
Short-container-title:Proceedings of the Japan Academy. Ser. B: Physical and Biological Sciences

Author:

ISHIGURO Masato¹,CHIBA Kurazo²,SAKAMOTO Seiichi¹^ORCID

Affiliation:

1. National Astronomical Observatory of Japan

2. School of Environment and Society, Tokyo Institute of Technology

Publisher

Japan Academy

Subject

General Physics and Astronomy,General Agricultural and Biological Sciences,General Medicine

Link

https://www.jstage.jst.go.jp/article/pjab/98/8/98_PJA9808B-04/_pdf

Reference100 articles.

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2. 2) Shimoda, K., Orchiston, W., Akabane, K. and Ishiguro, M. (2013) Highlighting the history of Japanese radio astronomy. 2: Koichi Shimoda and the 1948 solar eclipse. JAHH 16, 98–106.

3. 3) Oda, M. and Takakura, T. (1951) A study on the solar noise at 3300 m.c. J. Phys. Soc. Jpn. 6, 202A.

4. 4) Wendt, H., Orchiston, W., Ishiguro, M. and Nakamura, T. (2017) Highlighting the history of Japanese radio astronomy. 5: The 1950 Osaka solar grating array proposal. JAHH 20, 112–118.

5. 5) Tanaka, H. and Kakinuma, T. (1953) Equipment under construction for locating sources of solar noise at 4000 Mc/s. Proc. Res. Inst. Atmos. Nagoya Univ. 1, 89.

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