Zobrazeno 1 - 10
of 101
pro vyhledávání: '"super rotation"'
Publikováno v:
Advances in Medical Education and Practice, Vol Volume 14, Pp 323-332 (2023)
Sadatoshi Watanabe,1 Koshi Kataoka,2 Miwa Sekine,2 David Aune,2 Kiyoshi Shikino,3 Yuji Nishizaki1,2 1Clinical Translational Science, Juntendo University Graduate School of Medicine, Tokyo, Japan; 2Division of Medical Education, Juntendo University Fa
Externí odkaz:
https://doaj.org/article/f9281da3bc194e3f953f3664127e64c9
Autor:
Norihiko Sugimoto, Yukiko Fujisawa, Nobumasa Komori, Hiroki Kashimura, Masahiro Takagi, Yoshihisa Matsuda
Publikováno v:
Earth, Planets and Space, Vol 75, Iss 1, Pp 1-9 (2023)
Abstract Horizontal diffusion and resolution are important factors to generate and maintain the super-rotation in the general circulation model (GCM) because waves which transport angular momentum are sensitive to them. Here, we investigated how the
Externí odkaz:
https://doaj.org/article/88970126cd23443bbab6e5595e8586ae
Autor:
Kylash Rajendran, Stephen R. Lewis, James A. Holmes, Paul M. Streeter, Anna A. Fedorova, Manish R. Patel
Publikováno v:
Geophysical Research Letters, Vol 48, Iss 16, Pp n/a-n/a (2021)
Abstract Super‐rotation affects—and is affected by—the distribution of dust in the martian atmosphere. We modeled this interaction during the 2018 global dust storm (GDS) of Mars Year 34 using data assimilation. Super‐rotation increased by a
Externí odkaz:
https://doaj.org/article/6686df7a7feb4b85a78d2e7b15f3fd68
Autor:
Norihiko Sugimoto, Yukiko Fujisawa, Mimo Shirasaka, Mirai Abe, Shin-ya Murakami, Toru Kouyama, Hiroki Ando, Masahiro Takagi, Masaru Yamamoto
Publikováno v:
Atmosphere, Vol 13, Iss 2, p 182 (2022)
At the cloud top of the Venus atmosphere, equatorial Kelvin waves have been observed and are considered to play an important role in the super-rotation. We were able to reproduce the wave in a general circulation model (GCM) by conducting an observin
Externí odkaz:
https://doaj.org/article/b9bdb7b97d5d47c88bdf1939231f9d0d
Autor:
Del Val Munilla, Andrés
Venus’s atmosphere is one of the most intriguing one within the Solar System with mysterious features such as the retrograde super-rotation, composition ambiguities or complex polar vortexes. To better understand and to enhance the research of the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______2121::4190b4d429ac7f31901d0c548339f4f6
http://hdl.handle.net/10810/60051
http://hdl.handle.net/10810/60051
Autor:
Norihiko Sugimoto, Yukiko Fujisawa, Mimo Shirasaka, Asako Hosono, Mirai Abe, Hiroki Ando, Masahiro Takagi, Masaru Yamamoto
Publikováno v:
Atmosphere, Vol 12, Iss 1, p 14 (2020)
Planetary-scale 4-day Kelvin-type waves at the cloud top of the Venus atmosphere have been reported from the 1980s, and their significance for atmospheric dynamics has been pointed out. However, these waves have not been reproduced in Venus atmospher
Externí odkaz:
https://doaj.org/article/1cca99fad43f4a168c5909905557470e
Publikováno v:
Journal of General and Family Medicine
Background In 2004, Japan introduced a mandatory 2‐year postgraduate training program for graduating medical students with a super‐rotation curriculum. A national matching system was established to determine the hospital residency programs best s
Publikováno v:
Proceedings of the National Academy of Sciences of the United States of America, 2007 Jan 01. 104(1), 31-35.
Externí odkaz:
https://www.jstor.org/stable/25426045
Autor:
Mimo Shirasaka, Yukiko Fujisawa, Mirai Abe, Masahiro Takagi, Hiroki Ando, Norihiko Sugimoto, Asako Hosono, Masaru Yamamoto
Publikováno v:
Atmosphere, Vol 12, Iss 14, p 14 (2021)
Atmosphere
Volume 12
Issue 1
Atmosphere
Volume 12
Issue 1
Planetary-scale 4-day Kelvin-type waves at the cloud top of the Venus atmosphere have been reported from the 1980s, and their significance for atmospheric dynamics has been pointed out. However, these waves have not been reproduced in Venus atmospher
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