Zobrazeno 1 - 10
of 90
pro vyhledávání: '"Hosokawa, Mizuhiko"'
Autor:
Kawamura, Seiji, Ando, Masaki, Seto, Naoki, Sato, Shuichi, Musha, Mitsuru, Kawano, Isao, Yokoyama, Jun'ichi, Tanaka, Takahiro, Ioka, Kunihito, Akutsu, Tomotada, Takashima, Takeshi, Agatsuma, Kazuhiro, Araya, Akito, Aritomi, Naoki, Asada, Hideki, Chiba, Takeshi, Eguchi, Satoshi, Enoki, Motohiro, Fujimoto, Masa-Katsu, Fujita, Ryuichi, Futamase, Toshifumi, Harada, Tomohiro, Hayama, Kazuhiro, Himemoto, Yoshiaki, Hiramatsu, Takashi, Hong, Feng-Lei, Hosokawa, Mizuhiko, Ichiki, Kiyotomo, Ikari, Satoshi, Ishihara, Hideki, Ishikawa, Tomohiro, Itoh, Yousuke, Ito, Takahiro, Iwaguchi, Shoki, Izumi, Kiwamu, Kanda, Nobuyuki, Kanemura, Shinya, Kawazoe, Fumiko, Kobayashi, Shiho, Kohri, Kazunori, Kojima, Yasufumi, Kokeyama, Keiko, Kotake, Kei, Kuroyanagi, Sachiko, Maeda, Kei-ichi, Matsushita, Shuhei, Michimura, Yuta, Morimoto, Taigen, Mukohyama, Shinji, Nagano, Koji, Nagano, Shigeo, Naito, Takeo, Nakamura, Kouji, Nakamura, Takashi, Nakano, Hiroyuki, Nakao, Kenichi, Nakasuka, Shinichi, Nakayama, Yoshinori, Nakazawa, Kazuhiro, Nishizawa, Atsushi, Ohkawa, Masashi, Oohara, Kenichi, Sago, Norichika, Saijo, Motoyuki, Sakagami, Masaaki, Sakai, Shin-ichiro, Sato, Takashi, Shibata, Masaru, Shinkai, Hisaaki, Shoda, Ayaka, Somiya, Kentaro, Sotani, Hajime, Takahashi, Ryutaro, Takahashi, Hirotaka, Akiteru, Takamori, Taniguchi, Keisuke, Taruya, Atsushi, Tsubono, Kimio, Tsujikawa, Shinji, Ueda, Akitoshi, Ueda, Ken-ichi, Watanabe, Izumi, Yagi, Kent, Yamada, Rika, Yokoyama, Shuichiro, Yoo, Chul-Moon, Zhu, Zong-Hong
Deci-hertz Interferometer Gravitational Wave Observatory (DECIGO) is the future Japanese space mission with a frequency band of 0.1 Hz to 10 Hz. DECIGO aims at the detection of primordial gravitational waves, which could be produced during the inflat
Externí odkaz:
http://arxiv.org/abs/2006.13545
Autor:
Matsubara, Kensuke, Hachisu, Hidekazu, Li, Ying, Nagano, Shigeo, Locke, Clayton, Nogami, Asahiko, Kajita, Masatoshi, Hayasaka, Kazuhiro, Ido, Tetsuya, Hosokawa, Mizuhiko
Publikováno v:
Opt. Express 20 (2012) 22034-22041
Optical frequency comparison of the 40Ca+ clock transition \nu_{Ca} (2S1/2-2D5/2, 729nm) against the 87Sr optical lattice clock transition \nu_{Sr}(1S0-3P0, 698nm) has resulted in a frequency ratio \nu_{Ca} / \nu_{Sr} = 0.957 631 202 358 049 9(2 3).
Externí odkaz:
http://arxiv.org/abs/1208.4654
Akademický článek
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Akademický článek
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K zobrazení výsledku je třeba se přihlásit.
Autor:
Kawamura, Seiji, Ando, Masaki, Nakamura, Takashi, Tsubono, Kimio, Tanaka, Takahiro, Funaki, Iklkoh, Seto, Naoki, Numata, Kenji, Sato, Shuichi, Ioka, Kunihito, Kanda, Nobuyuki, Takashima, Takeshi, Agatsuma, Kazuhiro, Akutsu, Tomotada, Akutsu, Tomomi, Aoyanagi, Koh-suke, Arai, Koji, Arase, Yuta, Araya, Akito, Asada, Hideki, Aso, Yoichi, Chiba, Takeshi, Ebisuzaki, Toshikazu, Fukushima, Mitsuhiro, Futamase, Toshifumi, Ganzu, Katsuhiko, Harada, Tomohiro, Hashimoto, Tatsuaki, Hayama, Kazuhiro, Hikida, Wataru, Himemoto, Yoshiaki, Hirabayashi, Hisashi, Hiramatsu, Takashi, Hong, Feng-Lei, Horisawa, Hideyuki, Hosokawa, Mizuhiko, Ichiki, Kiyotomo, Ikegami, Takeshi, Inoue, Kaiki T., Ishidoshiro, Koji, Ishihara, Hideki, Ishikawa, Takehiko, Ishizaki, Hideharu, Ito, Hiroyuki, Itoh, Yousuke, Kamagasako, Shogo, Kawashima, Nobuki, Kawazoe, Fumiko, Kirihara, Hiroyuki, Kishimoto, Naoko, Kiuchi, Kenta, Kobayashi, Shiho, Kohri, Kazunori, Koizumi, Hiroyuki, Kojima, Yasufumi, Kokeyama, Keiko, Kokuyama, Wataru, Kotake, Kei, Kozai, Yoshihide, Kudoh, Hideaki, Kunimori, Hiroo, Kuninaka, Hitoshi, Kuroda, Kazuaki, Maeda, Kei-ichi, Matsuhara, Hideo, Mino, Yasushi, Miyakawa, Osamu, Miyoki, Shinji, Morimoto, Mutsuko Y., Morioka, Tomoko, Morisawa, Toshiyuki, Moriwaki, Shigenori, Mukohyama, Shinji, Musha, Mitsuru, Nagano, Shigeo, Naito, Isao, Nakagawa, Noriyasu, Nakamura, Kouji, Nakano, Hiroyuki, Nakao, Kenichi, Nakasuka, Shinichi, Nakayama, Yoshinori, Nishida, Erina, Nishiyama, Kazutaka, Nishizawa, Atsushi, Niwa, Yoshito, Ohashi, Masatake, Ohishi, Naoko, Ohkawa, Masashi, Okutomi, Akira, Onozato, Kouji, Oohara, Kenichi, Sago, Norichika, Saijo, Motoyuki, Sakagami, Masaaki, Sakai, Shin-ichiro, Sakata, Shihori, Sasaki, Misao, Sato, Takashi, Shibata, Masaru, Shinkai, Hisaaki, Somiya, Kentaro, Sotani, Hajime, Sugiyama, Naoshi, Suwa, Yudai, Tagoshi, Hideyuki, Takahashi, Kakeru, Takahashi, Keitaro, Takahashi, Tadayuki, Tahahashi, Hirotaka, Takahashi, Ryuichi, Takahashi, Ryutaro, Takamori, Akiteru, Takano, Tadashi, Taniguchi, Keisuke, Taruya, Atsushi, Tashiro, Hiroyuki, Tokuda, Mitsuru, Tokunari, Masao, Toyoshima, Morio, Tsujikawa, Shinji, Tsunesada, Yoshiki, Ueda, Ken-ichi, Utashima, Masayoshi, Yamakawa, Hiroshi, Yamamoto, Kazuhiro, Yamazaki, Toshitaka, Yokoyama, Jun'ichi, Yoo, Chul-Moon, Yoshida, Shijun, Yoshino, Taizoh
Publikováno v:
Journal of Physics: Conference Series. 122(1):1-8
DECi-hertz Interferometer Gravitational wave Observatory (DECIGO) is the future Japanese space gravitational wave antenna. The goal of DECIGO is to detect gravitational waves from various kinds of sources mainly between 0.1 Hz and 10 Hz and thus to o
Autor:
Arias, Elisa Felicitas, Hosokawa, Mizuhiko, Matsakis, Demetrios, Tuckey, Philip, Zhang, Shougang
Publikováno v:
IAU Symposium
IAU General Assembly XXIX, Meeting #29, #2254766
IAU General Assembly XXIX, Meeting #29, #2254766, Aug 2015, Honolulu, Hawaii, United States
IAU General Assembly XXIX, Meeting #29, #2254766
IAU General Assembly XXIX, Meeting #29, #2254766, Aug 2015, Honolulu, Hawaii, United States
International audience; International Atomic Time (TAI) is a realization of Terrestrial Time (TT), stable at the level of 4 x 10-16 over one month. It is computed at the International Bureau of Weights and Measures (BIPM) using clock and primary/seco
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______2417::ee71c4c5dfc571280a4a8700dc3fe3b7
https://hal.science/hal-03743462
https://hal.science/hal-03743462
Autor:
ILOMグループ, Hanada, Hideo, Kunimori, Hiroo, Hosokawa, Mizuhiko, Katayama, Masato, Sasaki, Sho, Kawano, Nobuyuki, Noda, Hirotomo, Araki, Hiroshi, ILOM, Group
Publikováno v:
第27回太陽系科学シンポジウム 平成17年度 = 27th Solar System Exploration Symposium 2005. :77-80
第27回太陽系科学シンポジウム 平成17年度(2005年12月13-14日. 宇宙航空研究開発機構宇宙科学研究本部(JAXA)(ISAS)), 相模原市, 神奈川県
27th Solar System Exploration Symposium 2005 (December 13-14, 2005
27th Solar System Exploration Symposium 2005 (December 13-14, 2005
Publikováno v:
VLBI技術による宇宙研究シンポジウム = Symposium on Space Research with VLBI Technology. :4-10
The observed position of QSOs may vary due to the gravitational deflection by foreground objects. This effect is eminent in the direction of the Galactic Center. To measure the distance to the Galactic Center with the relative error of a few percent,
Autor:
Nagano, Shigeo, Yoshino, Taizoh, Kunimori, Hiroo, Hosokawa, Mizuhiko, Kawamura, Seiji, Sato, Takashi, Ohkawa, Masashi
Publikováno v:
Measurement Science and Technology. 15(12):2406-2411
We present a new displacement measuring technique with simplicity, robustness, high sensitivity and wide measurement range. A set of a frequency shifter and a voltage–frequency converter is used to lock a homodyne interferometer on the half-bright
Autor:
Hanada, Hideo, Araki, Hiroshi, Katayama, Masato, Sasaki, Sho, Tsuruta, Seiitsu, Noda, Hirotomo, Funazaki, Kenichi, Iwata, Takahiro, Kunimori, Hiroo, Hosokawa, Mizuhiko
Publikováno v:
第8回宇宙科学シンポジウム 講演集 = Proceedings of the 8th Space Science Symposium.
第8回宇宙科学シンポジウム (2008年1月8日-9日. 宇宙航空研究開発機構宇宙科学研究本部(JAXA)(ISAS)相模原キャンパス), 相模原市, 神奈川県
8th Space Science Symposium (January 8-9, 2008. Institute of S
8th Space Science Symposium (January 8-9, 2008. Institute of S