Journal article
Jupiter's auroral-related stratospheric heating and chemistry I: Analysis of Voyager-IRIS and Cassini-CIRS spectra
- Abstract:
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Auroral processes are evident in Jupiter's polar atmosphere over a large range in wavelength (X-ray to radio). In particular, previous observations in the mid-infrared (5-15 μm) have shown enhanced emission from CH4, C2H2 and C2H4 and further stratospheric hydrocarbon species in spatial regions coincident with auroral processes observed at other wavelengths. These regions, described as auroral-related hotspots, observed at approximately 160°W to 200°W (System III) at high-northern latitudes a...
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- Publication status:
- Published
- Peer review status:
- Peer reviewed
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- Files:
-
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(Preview, Accepted manuscript, pdf, 13.8MB, Terms of use)
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- Publisher copy:
- 10.1016/j.icarus.2016.12.033
Authors
+ National Aeronautics and Space Administration
More from this funder
- Funding agency for:
- Sinclair, J
- Orton, G
- Publisher:
- Elsevier
- Journal:
- Icarus More from this journal
- Volume:
- 292
- Pages:
- 182-207
- Publication date:
- 2017-01-06
- Acceptance date:
- 2016-12-22
- DOI:
- EISSN:
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1090-2643
- ISSN:
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0019-1035
- Keywords:
- Pubs id:
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pubs:675313
- UUID:
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uuid:a79849a4-2152-4ff6-81af-e159fc982a32
- Local pid:
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pubs:675313
- Source identifiers:
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675313
- Deposit date:
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2017-02-22
Terms of use
- Copyright holder:
- © 2017 Elsevier Inc All rights reserved
- Copyright date:
- 2017
- Notes:
- This is the author accepted manuscript following peer review version of the article. The final version is available online from Elsevier at: 10.1016/j.icarus.2016.12.033
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