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Kelvin Wave and Its Impact on the Venus Atmosphere Tested by Observing System Simulation Experiment

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 observing system simulation experiment (OSSE) with the hel...

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Xehetasun bibliografikoak
Egile Nagusiak: Norihiko Sugimoto, Yukiko Fujisawa, Mimo Shirasaka, Mirai Abe, Shin-ya Murakami, Toru Kouyama, Hiroki Ando, Masahiro Takagi, Masaru Yamamoto
Formatua: Artigo
Hizkuntza:Inglês
Argitaratua: MDPI AG 2022-01-01
Saila:Atmosphere
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Sarrera elektronikoa:https://www.mdpi.com/2073-4433/13/2/182
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