Planetary-scale streak structure reproduced in high-resolution simulations of the Venus atmosphere with a low-stability layer

A planetary-scale streak structure in the Venusian lower-cloud layer was observed by the Akatsuki orbiter. Here the authors present numerical simulations that reproduce such structure and reveal that a low-stability layer, which induces baroclinic disturbances, is essential for its formation.

Guardado en:

Detalles Bibliográficos
Autores principales:	Hiroki Kashimura, Norihiko Sugimoto, Masahiro Takagi, Yoshihisa Matsuda, Wataru Ohfuchi, Takeshi Enomoto, Kensuke Nakajima, Masaki Ishiwatari, Takao M. Sato, George L. Hashimoto, Takehiko Satoh, Yoshiyuki O. Takahashi, Yoshi-Yuki Hayashi
Formato:	article
Lenguaje:	EN
Publicado:	Nature Portfolio 2019
Materias:	Science Q
Acceso en línea:	https://doaj.org/article/31d1db3a6f414d6eb3f361a520ae66fd
Etiquetas:	Agregar Etiqueta Sin Etiquetas, Sea el primero en etiquetar este registro!

id	oai:doaj.org-article:31d1db3a6f414d6eb3f361a520ae66fd
record_format	dspace
spelling	oai:doaj.org-article:31d1db3a6f414d6eb3f361a520ae66fd2021-12-02T17:32:10ZPlanetary-scale streak structure reproduced in high-resolution simulations of the Venus atmosphere with a low-stability layer10.1038/s41467-018-07919-y2041-1723https://doaj.org/article/31d1db3a6f414d6eb3f361a520ae66fd2019-01-01T00:00:00Zhttps://doi.org/10.1038/s41467-018-07919-yhttps://doaj.org/toc/2041-1723A planetary-scale streak structure in the Venusian lower-cloud layer was observed by the Akatsuki orbiter. Here the authors present numerical simulations that reproduce such structure and reveal that a low-stability layer, which induces baroclinic disturbances, is essential for its formation.Hiroki KashimuraNorihiko SugimotoMasahiro TakagiYoshihisa MatsudaWataru OhfuchiTakeshi EnomotoKensuke NakajimaMasaki IshiwatariTakao M. SatoGeorge L. HashimotoTakehiko SatohYoshiyuki O. TakahashiYoshi-Yuki HayashiNature PortfolioarticleScienceQENNature Communications, Vol 10, Iss 1, Pp 1-11 (2019)
institution	DOAJ
collection	DOAJ
language	EN
topic	Science Q
spellingShingle	Science Q Hiroki Kashimura Norihiko Sugimoto Masahiro Takagi Yoshihisa Matsuda Wataru Ohfuchi Takeshi Enomoto Kensuke Nakajima Masaki Ishiwatari Takao M. Sato George L. Hashimoto Takehiko Satoh Yoshiyuki O. Takahashi Yoshi-Yuki Hayashi Planetary-scale streak structure reproduced in high-resolution simulations of the Venus atmosphere with a low-stability layer
description	A planetary-scale streak structure in the Venusian lower-cloud layer was observed by the Akatsuki orbiter. Here the authors present numerical simulations that reproduce such structure and reveal that a low-stability layer, which induces baroclinic disturbances, is essential for its formation.
format	article
author	Hiroki Kashimura Norihiko Sugimoto Masahiro Takagi Yoshihisa Matsuda Wataru Ohfuchi Takeshi Enomoto Kensuke Nakajima Masaki Ishiwatari Takao M. Sato George L. Hashimoto Takehiko Satoh Yoshiyuki O. Takahashi Yoshi-Yuki Hayashi
author_facet	Hiroki Kashimura Norihiko Sugimoto Masahiro Takagi Yoshihisa Matsuda Wataru Ohfuchi Takeshi Enomoto Kensuke Nakajima Masaki Ishiwatari Takao M. Sato George L. Hashimoto Takehiko Satoh Yoshiyuki O. Takahashi Yoshi-Yuki Hayashi
author_sort	Hiroki Kashimura
title	Planetary-scale streak structure reproduced in high-resolution simulations of the Venus atmosphere with a low-stability layer
title_short	Planetary-scale streak structure reproduced in high-resolution simulations of the Venus atmosphere with a low-stability layer
title_full	Planetary-scale streak structure reproduced in high-resolution simulations of the Venus atmosphere with a low-stability layer
title_fullStr	Planetary-scale streak structure reproduced in high-resolution simulations of the Venus atmosphere with a low-stability layer
title_full_unstemmed	Planetary-scale streak structure reproduced in high-resolution simulations of the Venus atmosphere with a low-stability layer
title_sort	planetary-scale streak structure reproduced in high-resolution simulations of the venus atmosphere with a low-stability layer
publisher	Nature Portfolio
publishDate	2019
url	https://doaj.org/article/31d1db3a6f414d6eb3f361a520ae66fd
work_keys_str_mv	AT hirokikashimura planetaryscalestreakstructurereproducedinhighresolutionsimulationsofthevenusatmospherewithalowstabilitylayer AT norihikosugimoto planetaryscalestreakstructurereproducedinhighresolutionsimulationsofthevenusatmospherewithalowstabilitylayer AT masahirotakagi planetaryscalestreakstructurereproducedinhighresolutionsimulationsofthevenusatmospherewithalowstabilitylayer AT yoshihisamatsuda planetaryscalestreakstructurereproducedinhighresolutionsimulationsofthevenusatmospherewithalowstabilitylayer AT wataruohfuchi planetaryscalestreakstructurereproducedinhighresolutionsimulationsofthevenusatmospherewithalowstabilitylayer AT takeshienomoto planetaryscalestreakstructurereproducedinhighresolutionsimulationsofthevenusatmospherewithalowstabilitylayer AT kensukenakajima planetaryscalestreakstructurereproducedinhighresolutionsimulationsofthevenusatmospherewithalowstabilitylayer AT masakiishiwatari planetaryscalestreakstructurereproducedinhighresolutionsimulationsofthevenusatmospherewithalowstabilitylayer AT takaomsato planetaryscalestreakstructurereproducedinhighresolutionsimulationsofthevenusatmospherewithalowstabilitylayer AT georgelhashimoto planetaryscalestreakstructurereproducedinhighresolutionsimulationsofthevenusatmospherewithalowstabilitylayer AT takehikosatoh planetaryscalestreakstructurereproducedinhighresolutionsimulationsofthevenusatmospherewithalowstabilitylayer AT yoshiyukiotakahashi planetaryscalestreakstructurereproducedinhighresolutionsimulationsofthevenusatmospherewithalowstabilitylayer AT yoshiyukihayashi planetaryscalestreakstructurereproducedinhighresolutionsimulationsofthevenusatmospherewithalowstabilitylayer
_version_	1718380359488372736

Planetary-scale streak structure reproduced in high-resolution simulations of the Venus atmosphere with a low-stability layer

Ejemplares similares