Phosphine on Venus Cannot Be Explained by Conventional Processes

Phosphine on Venus Cannot Be Explained by Conventional Processes

The recent candidate detection of ~1 ppb of phosphine in the middle atmosphere of Venus is so unexpected that it requires an exhaustive search for explanations of its origin. Phosphorus-containing species have not been modelled for Venus' atmosphere before and our work represents the first atte...

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Xehetasun bibliografikoak
Egile Nagusiak: Bains, William, Petkowski, Janusz J, Seager, Sara, Ranjan, Sukrit, Sousa-Silva, Clara, Rimmer, Paul B, Zhan, Zhuchang, Greaves, Jane S, Richards, Anita MS
Beste egile batzuk: Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences
Formatua: Artikulua
Hizkuntza:English
Argitaratua: Mary Ann Liebert Inc 2021
Sarrera elektronikoa:https://hdl.handle.net/1721.1/135598

Internet

https://hdl.handle.net/1721.1/135598

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