Dynamical relationship between wind speed magnitude and meridional temperature contrast: Application to an interannual oscillation in Venusian middle atmosphere GCM-Reference-Cited by-同舟云学术

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Dynamical relationship between wind speed magnitude and meridional temperature contrast: Application to an interannual oscillation in Venusian middle atmosphere GCM

Published:2018-03 Issue: Volume:303 Page:131-148
ISSN:0019-1035
Container-title:Icarus
language:en
Short-container-title:Icarus

Author:

Yamamoto Masaru,Takahashi Masaaki

Funder

Scientific Research/Japan Society for the Promotion of Science (MEXT/JSPS KAKENHI

Publisher

Elsevier BV

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference42 articles.

1. Middle Atmosphere Dynamics;Andrews,1987

2. On the stability of internal baroclinic jets in a rotating atmosphere;Charney;J. Atmos. Sci.,1962

3. Ground-based near-infrared imaging observations of Venus during the Galileo encounter;Crisp;Science,1991

4. 4-day waves in the Venus atmosphere;Covey;Icarus,1981

5. Planetary-scale waves in the Venus atmosphere;Covey;J. Atmos. Sci.,1982

Cited by 3 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Equatorial Kelvin-like waves on slowly rotating and/or small-sized spheres: Application to Venus and Titan;Icarus;2019-04

2. Solar-locked and geographical atmospheric structures inferred from a Venus general circulation model with radiative transfer;Icarus;2019-03

3. Mitigation of the alternative energy for the wind farm center considering temperature and wind speed;MATEC Web of Conferences;2018

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