# Cordiner 2022: Phosphine in the Venusian Atmosphere: A Strict Upper Limit From SOFIA GREAT Observations

> M. A. Cordiner, G. L. Villanueva, H. Wiesemeyer et al., 2022. 8 records on Mysteries Department cite it. The strictest upper limit at high altitude.

Source: https://mysteriesdept.com/sources/SRC0CQY1KN03DN2/phosphine-in-the-venusian-atmosphere-a-strict-upper-limit  
Publisher: Mysteries Department  
Licence: CC BY 4.0 (credit Mysteries Department and link the page)  

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[Sources](https://mysteriesdept.com/sources)[Phosphine in the clouds of Venus](https://mysteriesdept.com/mysteries/venus-phosphine)Cordiner 2022

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# Phosphine in the Venusian Atmosphere: A Strict Upper Limit From SOFIA GREAT Observations

M. A. Cordiner, G. L. Villanueva, H. Wiesemeyer et al., 2022. _Geophysical Research Letters 49(22), e2022GL101055_.

Three SOFIA flights in November 2021 targeted phosphine lines near 533 and 1,067 GHz and found none; radiative transfer gives a disk-averaged upper limit of 0.8 ppb from 75 to 110 km.

**Phosphine in the clouds of Venus** ArticleCopy of **[SOFIA GREAT spectra of Venus, November 2021](https://mysteriesdept.com/mysteries/venus-phosphine/artifacts/ART0CQY28MW1K0S/sofia-great-spectra-of-venus-november-2021)** doi: **[10.1029/2022gl101055](https://doi.org/10.1029/2022gl101055)** Checked against the original0

## What it's used for here

The strictest upper limit at high altitude.

## Cited by on this site 8 records

[The upper limits exclude phosphine at the claimed levels.](https://mysteriesdept.com/mysteries/venus-phosphine/answers/ANS0CQY221Y38RV/the-upper-limits-exclude-phosphine-at-the-claimed-levels)

Answer

ANS

[SOFIA GREAT spectra of Venus, November 2021](https://mysteriesdept.com/mysteries/venus-phosphine/artifacts/ART0CQY28MW1K0S/sofia-great-spectra-of-venus-november-2021)

ART

[SOFIA GREAT spectra of Venus, November 2021: document](https://mysteriesdept.com/mysteries/venus-phosphine/copies/CPY0CQY294G6K5J/sofia-great-spectra-of-venus-november-2021-document)

CPY

[SOFIA found no phosphine lines at 533 and 1,067 GHz, limit 0.8 ppb at 75–110 km.](https://mysteriesdept.com/mysteries/venus-phosphine/evidence/EVD0CQY1ZVM37ZF/sofia-found-no-phosphine-lines-at-533-and-1-067-ghz-limit-0)

Evidence

EVD

[SOFIA's 0.8 ppb limit is more stringent than earlier ground-based studies.](https://mysteriesdept.com/mysteries/venus-phosphine/evidence/EVD0CQY229R6233/sofias-0-8-ppb-limit-is-more-stringent-than-earlier-ground)

Evidence

EVD

[SOFIA flights find no phosphine above 75 km](https://mysteriesdept.com/mysteries/venus-phosphine/events/EVT0CQY1SRA7833/sofia-flights-find-no-phosphine-above-75-km)

EVT

[Phosphine in the clouds of Venus](https://mysteriesdept.com/mysteries/venus-phosphine)

The mystery article

MYS

[Can the claimed phosphine be reconciled with the upper limits from other instruments?](https://mysteriesdept.com/mysteries/venus-phosphine/questions/QST0CQY1TZC4EZE/can-the-claimed-phosphine-be-reconciled-with-the-upper)

Question

QST

## Cite it

```
Cordiner, M. A., Villanueva, G. L., Wiesemeyer, H., Milam, S. N., de Pater, I., & et al. (2022). Phosphine in the Venusian Atmosphere: A Strict Upper Limit From SOFIA GREAT Observations. Geophysical Research Letters 49(22), e2022GL101055. https://doi.org/10.1029/2022gl101055
```

[Read it free at doi.org](https://doi.org/10.1029/2022gl101055)

Key

**SRC** 0CQY1KN03DN2

Kind

Journal article

Rights

The publisher's

Checked

Against the published article

Added by

[apollo](https://mysteriesdept.com/u/apollo)

The record

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