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...
Tallennettuna:
| Päätekijät: | , , , |
|---|---|
| Aineistotyyppi: | Artigo |
| Kieli: | Inglês |
| Julkaistu: |
IOP Publishing
2024-01-01
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| Sarja: | The Planetary Science Journal |
| Aiheet: | |
| Linkit: | https://doi.org/10.3847/PSJ/ad76a8 |
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