Cryogenic systems of the cryogenic laser interferometer observatory

Takashi Uchiyama; Shinji Miyoki; Masatake Ohashi; Kazuaki Kuroda; Kazuhiro Yamamoto; Masao Tokunari; Tomomi Akutsu; Shohgo Kamagasako; Noriyasu Nakagawa; Hiroyuki Kirihara; Kazuhiro Agatsuma; Hideki Ishitsuka; Daisuke Tatsumi; Souichi Telada; Masaki Ando; Takayuki Tomaru; Toshikazu Suzuki; Nobuaki Sato; Tomiyoshi Haruyama; Akira Yamamoto; Takakazu Shintomi

doi:10.1088/1742-6596/32/1/038

Cryogenic systems of the cryogenic laser interferometer observatory

Takashi Uchiyama^*, Shinji Miyoki, Masatake Ohashi, Kazuaki Kuroda, Kazuhiro Yamamoto, Masao Tokunari, Tomomi Akutsu, Shohgo Kamagasako, Noriyasu Nakagawa, Hiroyuki Kirihara, Kazuhiro Agatsuma, Hideki Ishitsuka, Daisuke Tatsumi, Souichi Telada, Masaki Ando, Takayuki Tomaru, Toshikazu Suzuki, Nobuaki Sato, Tomiyoshi Haruyama, Akira YamamotoTakakazu Shintomi

^*Corresponding author for this work

Department of Physics

Research output: Contribution to journal › Article › peer-review

11 Scopus citations

Abstract

Cryogenic Laser Interferometer Observatory (CLIO) is a laser interferometric gravitational wave detector using cryogenic cooled mirrors. In order to cool the mirrors, cryogenic environment is necessary. We made four vacuum chambers with cryogenic cooled shields inside. The mirror is suspended by a mirror suspension system with a heat path for transferring heat from the mirror to the shield. Test cooling of the chambers and the mirror suspension system has been done. After one week cooling, the chambers was cooled from 8K to 10K and the mirror were cooled at 21K successfully.

Original language	English
Pages (from-to)	259-264
Number of pages	6
Journal	Journal of Physics: Conference Series
Volume	32
Issue number	1
DOIs	https://doi.org/10.1088/1742-6596/32/1/038
State	Published - 2006/03/02

ASJC Scopus subject areas

General Physics and Astronomy

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Uchiyama, T., Miyoki, S., Ohashi, M., Kuroda, K., Yamamoto, K., Tokunari, M., Akutsu, T., Kamagasako, S., Nakagawa, N., Kirihara, H., Agatsuma, K., Ishitsuka, H., Tatsumi, D., Telada, S., Ando, M., Tomaru, T., Suzuki, T., Sato, N., Haruyama, T., ... Shintomi, T. (2006). Cryogenic systems of the cryogenic laser interferometer observatory. Journal of Physics: Conference Series, 32(1), 259-264. https://doi.org/10.1088/1742-6596/32/1/038

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title = "Cryogenic systems of the cryogenic laser interferometer observatory",

abstract = "Cryogenic Laser Interferometer Observatory (CLIO) is a laser interferometric gravitational wave detector using cryogenic cooled mirrors. In order to cool the mirrors, cryogenic environment is necessary. We made four vacuum chambers with cryogenic cooled shields inside. The mirror is suspended by a mirror suspension system with a heat path for transferring heat from the mirror to the shield. Test cooling of the chambers and the mirror suspension system has been done. After one week cooling, the chambers was cooled from 8K to 10K and the mirror were cooled at 21K successfully.",

author = "Takashi Uchiyama and Shinji Miyoki and Masatake Ohashi and Kazuaki Kuroda and Kazuhiro Yamamoto and Masao Tokunari and Tomomi Akutsu and Shohgo Kamagasako and Noriyasu Nakagawa and Hiroyuki Kirihara and Kazuhiro Agatsuma and Hideki Ishitsuka and Daisuke Tatsumi and Souichi Telada and Masaki Ando and Takayuki Tomaru and Toshikazu Suzuki and Nobuaki Sato and Tomiyoshi Haruyama and Akira Yamamoto and Takakazu Shintomi",

year = "2006",

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doi = "10.1088/1742-6596/32/1/038",

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Uchiyama, T, Miyoki, S, Ohashi, M, Kuroda, K, Yamamoto, K, Tokunari, M, Akutsu, T, Kamagasako, S, Nakagawa, N, Kirihara, H, Agatsuma, K, Ishitsuka, H, Tatsumi, D, Telada, S, Ando, M, Tomaru, T, Suzuki, T, Sato, N, Haruyama, T, Yamamoto, A & Shintomi, T 2006, 'Cryogenic systems of the cryogenic laser interferometer observatory', Journal of Physics: Conference Series, vol. 32, no. 1, pp. 259-264. https://doi.org/10.1088/1742-6596/32/1/038

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T1 - Cryogenic systems of the cryogenic laser interferometer observatory

AU - Uchiyama, Takashi

AU - Miyoki, Shinji

AU - Ohashi, Masatake

AU - Kuroda, Kazuaki

AU - Yamamoto, Kazuhiro

AU - Tokunari, Masao

AU - Akutsu, Tomomi

AU - Kamagasako, Shohgo

AU - Nakagawa, Noriyasu

AU - Kirihara, Hiroyuki

AU - Agatsuma, Kazuhiro

AU - Ishitsuka, Hideki

AU - Tatsumi, Daisuke

AU - Telada, Souichi

AU - Ando, Masaki

AU - Tomaru, Takayuki

AU - Suzuki, Toshikazu

AU - Sato, Nobuaki

AU - Haruyama, Tomiyoshi

AU - Yamamoto, Akira

AU - Shintomi, Takakazu

PY - 2006/3/2

Y1 - 2006/3/2

N2 - Cryogenic Laser Interferometer Observatory (CLIO) is a laser interferometric gravitational wave detector using cryogenic cooled mirrors. In order to cool the mirrors, cryogenic environment is necessary. We made four vacuum chambers with cryogenic cooled shields inside. The mirror is suspended by a mirror suspension system with a heat path for transferring heat from the mirror to the shield. Test cooling of the chambers and the mirror suspension system has been done. After one week cooling, the chambers was cooled from 8K to 10K and the mirror were cooled at 21K successfully.

AB - Cryogenic Laser Interferometer Observatory (CLIO) is a laser interferometric gravitational wave detector using cryogenic cooled mirrors. In order to cool the mirrors, cryogenic environment is necessary. We made four vacuum chambers with cryogenic cooled shields inside. The mirror is suspended by a mirror suspension system with a heat path for transferring heat from the mirror to the shield. Test cooling of the chambers and the mirror suspension system has been done. After one week cooling, the chambers was cooled from 8K to 10K and the mirror were cooled at 21K successfully.

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EP - 264

JO - Journal of Physics: Conference Series

JF - Journal of Physics: Conference Series

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Cryogenic systems of the cryogenic laser interferometer observatory

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