Circulation of Venusian Atmosphere at 90–110 km Based on Apparent Motions of the O 2 1.27 μm Nightglow From VIRTIS‐M (Venus Express) Data-Reference-Cited by-同舟云学术

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Circulation of Venusian Atmosphere at 90–110 km Based on Apparent Motions of the O 2 1.27 μm Nightglow From VIRTIS‐M (Venus Express) Data

Published:2018-03-15 Issue:5 Volume:45 Page:2554-2562
ISSN:0094-8276
Container-title:Geophysical Research Letters
language:en
Short-container-title:Geophys. Res. Lett.

Author:

Gorinov D. A.¹^ORCID,Khatuntsev I. V.¹^ORCID,Zasova L. V.¹,Turin A. V.¹^ORCID,Piccioni G.²^ORCID

Affiliation:

1. Space Research Institute RAS Moscow Russia

2. INAF‐IAPS Rome Italy

Funder

Ministry of Education and Science of the Russian Federation

Federal Agency for Science and Innovation

Publisher

American Geophysical Union (AGU)

Subject

General Earth and Planetary Sciences,Geophysics

Link

https://onlinelibrary.wiley.com/doi/pdf/10.1002/2017GL076380

Reference36 articles.

1. Local time asymmetries in the Venus thermosphere

2. Local time asymmetries in the Venus thermosphere

3. Modeling VIRTIS/VEX O2(a1∆g) nightglow profiles affected by the propagation of gravity waves in the Venus upper mesosphere

4. The temperature of the Venus mesosphere from O2 (aΔg1) airglow observations

5. Influence of Venus topography on the zonal wind and UV albedo at cloud top level: The role of stationary gravity waves

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3. O2 (а1Δg) Airglow at 1.27 μM and upper Mesosphere Dynamics on the Night Side of Venus;Solar System Research;2023-06

4. O2 (а1Δg) Airglow at 1.27 μM and upper Mesosphere Dynamics on the Night Side of Venus;Астрономический вестник;2023-05-01

5. Analytical Approximations of the Characteristics of Nighttime Hydroxyl on Mars and Intra-Annual Variations;Solar System Research;2023-02

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