4 results on '"Norihiko Sugimoto"'
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2. Wave analysis in the atmosphere of Venus below 100-km altitude, simulated by the LMD Venus GCM
- Author
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Norihiko Sugimoto, Gabriella Gilli, Sébastien Lebonnois, Laboratoire de Météorologie Dynamique (UMR 8539) (LMD), Département des Géosciences - ENS Paris, École normale supérieure - Paris (ENS Paris), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-École normale supérieure - Paris (ENS Paris), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-École des Ponts ParisTech (ENPC)-École polytechnique (X)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Pierre et Marie Curie - Paris 6 (UPMC), Dpt of Physics [Yokohama], Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-École polytechnique (X)-École des Ponts ParisTech (ENPC)-Centre National de la Recherche Scientifique (CNRS)-Département des Géosciences - ENS Paris, École normale supérieure - Paris (ENS-PSL), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-École normale supérieure - Paris (ENS-PSL), and Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)
- Subjects
Angular momentum ,010504 meteorology & atmospheric sciences ,Atmospheric circulation ,Baroclinity ,Equator ,Venus ,Atmospheric sciences ,01 natural sciences ,Physics::Geophysics ,Atmosphere ,Atmosphere of Venus ,0103 physical sciences ,010303 astronomy & astrophysics ,Astrophysics::Galaxy Astrophysics ,Physics::Atmospheric and Oceanic Physics ,0105 earth and related environmental sciences ,[PHYS.PHYS.PHYS-AO-PH]Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph] ,[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph] ,biology ,Atmospheric wave ,Astronomy and Astrophysics ,biology.organism_classification ,13. Climate action ,Space and Planetary Science ,Physics::Space Physics ,Astrophysics::Earth and Planetary Astrophysics ,Geology - Abstract
International audience; A new simulation of Venus atmospheric circulation obtained with the LMD Venus GCM is described and the simulated wave activity is analysed. Agreement with observed features of the temperature structure, static stability and zonal wind field is good, such as the presence of a cold polar collar, diurnal and semi-diurnal tides. At the resolution used (96 longitudes × 96 latitudes), a fully developed superrotation is obtained both when the simulation is initialised from rest and from an atmosphere already in superrotation, though winds are still weak below the clouds (roughly half the observed values). The atmospheric waves play a crucial role in the angular momentum budget of the Venus’s atmospheric circulation. In the upper cloud, the vertical angular momentum is transported by the diurnal and semi-diurnal tides. Above the cloud base (approximately 1 bar), equatorward transport of angular momentum is done by polar barotropic and mid- to high-latitude baroclinic waves present in the cloud region, with frequencies between 5 and 20 cycles per Venus day (periods between 6 and 23 Earth days). In the middle cloud, just above the convective layer, a Kelvin type wave (period around 7.3 Ed) is present at the equator, as well as a low-latitude Rossby-gravity type wave (period around 16 Ed). Below the clouds, large-scale mid- to high-latitude gravity waves develop and play a significant role in the angular momentum balance.
- Published
- 2016
- Full Text
- View/download PDF
3. Inverse insolation dependence of Venus’ cloud-level convection
- Author
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Kohei Ikeda, Yasumitsu Maejima, Hiroki Ando, Takeshi Imamura, Takehito Higuchi, Masahiro Takagi, and Norihiko Sugimoto
- Subjects
Convection ,Daytime ,biology ,Flux ,Astronomy and Astrophysics ,Venus ,biology.organism_classification ,Atmospheric sciences ,Atmosphere ,Atmosphere of Venus ,Space and Planetary Science ,Planet ,Physics::Space Physics ,Astrophysics::Solar and Stellar Astrophysics ,Environmental science ,Astrophysics::Earth and Planetary Astrophysics ,Gravity wave ,Physics::Atmospheric and Oceanic Physics - Abstract
Accepted: 2013-10-08, 資料番号: SA1004601000
- Published
- 2014
- Full Text
- View/download PDF
4. Miniaturization of carbon fibers and its applications
- Author
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Ryotaro Kohara, Masahiro Toyoda, Norihiko Sugimoto, Shinji Fukushima, Hiroyuki Muto, Satoshi Yoshinaga, and Mototsugu Sakai
- Subjects
chemistry.chemical_classification ,Nanocomposite ,Field emission display ,Materials science ,Composite number ,General Chemistry ,Molding (process) ,Field electron emission ,chemistry.chemical_compound ,Nylon 6 ,chemistry ,General Materials Science ,Compounds of carbon ,Composite material ,Elastic modulus - Abstract
Exfoliated carbon fibers (ExCFs) obtained through rapid heat-treatment of intercalation compounds of carbon fibers had changed to the bundle of thin filament. In one of applications of its ExCFs, it was tried to nanocomposite where the application of Carbon nano tube (CNT) made an attempt. Preparation of composite using Nylon 6 and the ExCFs as the matrix and fillers was carried out by the injection molding. As the result, it became clear that addition of the ExCFs as fillers could be reinforced the matrix. Bending stress and elastic modulus of composite reinforced by the ExCFs increased around 50% with increasing in addition of the ExCFs in comparison with blank. It became clear that the ExCFs also exhibited better field emission characteristic at small-applied voltage in the case of an electrode material of field emission display (FED). Its field emission characteristics surpassed the case which CNT was applied to the electrode. Future applications were expected to the ExCFs.
- Published
- 2009
- Full Text
- View/download PDF
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