Zobrazeno 1 - 10
of 45
pro vyhledávání: '"Tomoki MIYAKAWA"'
Autor:
Daisuke Takasuka, Chihiro Kodama, Tamaki Suematsu, Tomoki Ohno, Yohei Yamada, Tatsuya Seiki, Hisashi Yashiro, Masuo Nakano, Hiroaki Miura, Akira T. Noda, Tomoe Nasuno, Tomoki Miyakawa, Ryusuke Masunaga
Publikováno v:
Journal of Advances in Modeling Earth Systems, Vol 16, Iss 2, Pp n/a-n/a (2024)
Abstract Toward the achievement of reliable global kilometer‐scale (k‐scale) climate simulations, we improve the Nonhydrostatic ICosahedral Atmospheric Model (NICAM) by focusing on moist physical processes. A goal of the model improvement is to e
Externí odkaz:
https://doaj.org/article/904a5c073bc44ef1a1a2fcc59369cf64
Autor:
Yohei Yamada, Tomoki Miyakawa, Masuo Nakano, Chihiro Kodama, Akiyoshi Wada, Tomoe Nasuno, Ying‐Wen Chen, Akira Yamazaki, Hisashi Yashiro, Masaki Satoh
Publikováno v:
Geophysical Research Letters, Vol 50, Iss 3, Pp n/a-n/a (2023)
Abstract Typhoon Faxai hit Japan in 2019 and severely damaged the Tokyo metropolitan area. To mitigate such damages, a good track forecast is necessary even before the typhoon formation. To investigate the predictability of the genesis and movement o
Externí odkaz:
https://doaj.org/article/0700ffad02f14afc81599909ecf643a8
Autor:
Masaki Satoh, Hirofumi Tomita, Hisashi Yashiro, Yoshiyuki Kajikawa, Yoshiaki Miyamoto, Tsuyoshi Yamaura, Tomoki Miyakawa, Masuo Nakano, Chihiro Kodama, Akira T. Noda, Tomoe Nasuno, Yohei Yamada, Yoshiki Fukutomi
Publikováno v:
Progress in Earth and Planetary Science, Vol 4, Iss 1, Pp 1-24 (2017)
Abstract This article reviews the major outcomes of a 5-year (2011–2016) project using the K computer to perform global numerical atmospheric simulations based on the non-hydrostatic icosahedral atmospheric model (NICAM). The K computer was made av
Externí odkaz:
https://doaj.org/article/4b5f679e0cee4767a6b203231456fe7d
Autor:
Daisuke Takasuka, Chihiro Kodama, Tamaki Suematsu, Tomoki Ohno, Yohei Yamada, Tatsuya Seiki, Hisashi Yashiro, Masuo Nakano, Hiroaki Miura, Akira T. Noda, Tomoe Nasuno, Tomoki Miyakawa, Ryusuke Masunaga
Toward the achievement of reliable global kilometer-scale (k-scale) climate simulations, we improve the Nonhydrostatic ICosaherdral Atmospheric Model (NICAM) by focusing on moist physical processes. A goal of the model improvement is to establish a c
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::22dbcb0a045c98545ce8eb052d4b4201
https://doi.org/10.22541/essoar.167839719.95840260/v1
https://doi.org/10.22541/essoar.167839719.95840260/v1
Autor:
Yohei Yamada, Tomoki Miyakawa, Masuo Nakano, Chihiro Kodama, Akiyoshi Wada, Tomoe Nasuno, Ying‐Wen Chen, Akira Yamazaki, Hisashi Yashiro, Masaki Satoh
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ff72c872c66512d59003409f5e46043b
https://doi.org/10.1002/essoar.10512027.1
https://doi.org/10.1002/essoar.10512027.1
Autor:
Chihiro Kodama, Woosub Roh, Tomoki Miyakawa, Yohei Yamada, Tomoki Ohno, Tatsuya Seiki, Hiroaki Miura, Tomoko Nitta, Masato Sugi, Tomoe Nasuno, Masaki Satoh, Daisuke Goto, Akira Noda, Ying-Wen Chen, Hisashi Yashiro, Masuo Nakano
Publikováno v:
Geoscientific Model Development, Vol 14, Pp 795-820 (2021)
The Nonhydrostatic ICosahedral Atmospheric Model (NICAM), a global model with an icosahedral grid system, has been under development for nearly two decades. This paper describes NICAM16-S, the latest stable version of NICAM (NICAM.16), modified for t
Autor:
Tomoki Miyakawa, Hiroaki Miura, Masaki Satoh, Tomoe Nasuno, Chihiro Kodama, Kazuyoshi Kikuchi, Masuo Nakano, Ryosuke Shibuya
Publikováno v:
Journal of the Meteorological Society of Japan. Ser. II. 99:973-992
Publikováno v:
Journal of the Meteorological Society of Japan; 2023, Vol. 101 Issue 3, p175-189, 15p
Autor:
Takanori Kodama, Daisuke Takasuka, Sam Sherriff-Tadano, Takeshi Kuroda, Tomoki Miyakawa, Ayako Abe-Ouchi, Masaki Satoh
Publikováno v:
The Astrophysical Journal. 940:87
Planetary climates are strongly affected by planetary orbital parameters such as obliquity, eccentricity, and precession. In exoplanetary systems, exo-terrestrial planets should have various obliquities. High-obliquity planets would have extreme seas