- Abstract:
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Observations of the visible/near-infrared reflectance spectrum of Jupiter have been made with the Very Large Telescope (VLT) Multi Unit Spectroscopic Explorer (MUSE) instrument in the spectral range 0.48 – 0.93 μm in support of the NASA/Juno mission. These spectra contain spectral signatures of gaseous ammonia (NH3), whose abundance above the cloud tops can be determined if we have reliable information on its absorption spectrum. While there are a number of sources of NH3 absorption data in t...
Expand abstract - Publication status:
- Published
- Peer review status:
- Peer reviewed
- Version:
- Accepted Manuscript
- Files:
-
-
(pdf, 1.2mb)
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- Publisher copy:
- 10.1016/j.icarus.2017.11.031
-
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- Publisher:
- Elsevier Publisher's website
- Journal:
- Icarus Journal website
- Volume:
- 302
- Pages:
- 426–436
- Publication date:
- 2017-11-29
- Acceptance date:
- 2017-11-27
- DOI:
- ISSN:
-
0019-1035
- Pubs id:
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pubs:800959
- URN:
-
uri:c3578a00-e833-4fdb-8d99-335c26b3a330
- UUID:
-
uuid:c3578a00-e833-4fdb-8d99-335c26b3a330
- Local pid:
- pubs:800959
- Copyright holder:
- Elsevier Inc.
- Copyright date:
- 2017
- Notes:
-
Copyright © 2017 Elsevier Inc. This is the accepted manuscript version of the article. The final version is available online from Elsevier at: https://doi.org/10.1016/j.icarus.2017.11.031
.
Journal article
Analysis of gaseous ammonia (NH3) absorption in the visible spectrum of Jupiter
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