Planetary Waves Drive Horizontal Variations in Trace Species in the Venus Deep Atmosphere

The deep atmosphere of Venus remains mysterious because of the planet’s high, optically thick cloud decks. While phenomena such as the observed decadal fluctuations in sulfur dioxide abundance above the clouds could shed light on conditions below, poor understanding of vertical and horizontal transp...

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Bibliographic Details

Published in:	The Planetary Science Journal
Main Authors:	Maureen Cohen, James Holmes, Stephen Lewis, Manish Patel
Format:	Article
Language:	English
Published:	IOP Publishing 2024-01-01
Subjects:	Venus Atmospheric dynamics Atmospheric structure Planetary atmospheres
Online Access:	https://doi.org/10.3847/PSJ/ad76a8