- Abstract:
-
Recent work by Sromovsky et al. (2017, Icarus 291, 232-244) suggested that all red colour in Jupiter’s atmosphere could be explained by a single colour-carrying compound, a so-called ‘universal chromophore’. We tested this hypothesis on ground-based spectroscopic observations in the visible and near-infrared (480- 930 nm) from the VLT/MUSE instrument between 2014 and 2018, retrieving a chromophore absorption spectrum directly from the North Equatorial Belt, and applying it to model spatial va...
Expand abstract - Publication status:
- Published
- Peer review status:
- Peer reviewed
- Publisher copy:
- 10.1016/j.icarus.2019.113589
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- Publisher:
- Elsevier Publisher's website
- Journal:
- Icarus Journal website
- Volume:
- 338
- Issue:
- 1 March 2020
- Article number:
- 113589
- Publication date:
- 2020-12-02
- Acceptance date:
- 2019-11-29
- DOI:
- ISSN:
-
0019-1035
- Pubs id:
-
pubs:1075862
- UUID:
-
uuid:0b84457b-95ad-41fe-91ab-c03551a18841
- Source identifiers:
-
1075862
- Local pid:
- pubs:1075862
- Language:
- English
- Keywords:
- Copyright holder:
- Elsevier Inc.
- Copyright date:
- 2019
- Rights statement:
- © 2019 Elsevier Inc. All rights reserved
Journal article
Colour and tropospheric cloud structure of Jupiter from MUSE/VLT: retrieving a universal chromophore
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