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dc.contributor.authorCravens, Thomas Edward
dc.contributor.authorMoore, L.
dc.contributor.authorWaite, J. H., Jr.
dc.contributor.authorPerryman, R.
dc.contributor.authorPerry, M.
dc.contributor.authorWahlund, J.‐E.
dc.contributor.authorPersoon, A.
dc.contributor.authorKurth, W. S.
dc.date.accessioned2021-02-17T16:12:44Z
dc.date.available2021-02-17T16:12:44Z
dc.date.issued2018-05-21
dc.identifier.citationCravens, T. E., Moore, L., Waite, J. H.., Perryman, R., Perry, M., Wahlund, J.‐E., et al. (2019). The ion composition of Saturn's equatorial ionosphere as observed by Cassini. Geophysical Research Letters, 46, 6315– 6321. https://doi.org/10.1029/2018GL077868en_US
dc.identifier.urihttp://hdl.handle.net/1808/31434
dc.descriptionAn edited version of this paper was published by AGU. Copyright 2018 American Geophysical Union.en_US
dc.description.abstractThe Cassini Orbiter made the first in situ measurements of the upper atmosphere and ionosphere of Saturn in 2017. The Ion and Neutral Mass Spectrometer (INMS) found molecular hydrogen and helium as well as minor species including water, methane, ammonia, and organics. INMS ion mode measurements of light ion species (H+, H2+, H3+, and He+) and Radio and Plasma Wave Science instrument measurements of electron densities are presented. A photochemical analysis of the INMS and Radio and Plasma Wave Science data indicates that the major ion species near the ionospheric peak must be heavy and molecular with a short chemical lifetime. A quantitative explanation of measured H+ and H3+ densities requires that they chemically react with one or more heavy neutral molecular species that have mixing ratios of about 100 ppm.en_US
dc.publisherWileyen_US
dc.rights© 2018. American Geophysical Union. All Rights Reserved.en_US
dc.titleThe Ion Composition of Saturn's Equatorial Ionosphere as Observed by Cassinien_US
dc.typeArticleen_US
kusw.kuauthorCravens, Thomas Edward
kusw.kudepartmentPhysics and Astronomyen_US
dc.identifier.doi10.1029/2018GL077868en_US
dc.identifier.orcidhttps://orcid.org/0000-0003-0912-8353en_US
dc.identifier.orcidhttps://orcid.org/0000-0003-4481-9862en_US
dc.identifier.orcidhttps://orcid.org/0000-0002-1978-1025en_US
dc.identifier.orcidhttps://orcid.org/0000-0003-1858-4692en_US
dc.identifier.orcidhttps://orcid.org/0000-0003-1600-6856en_US
dc.identifier.orcidhttps://orcid.org/0000-0002-2107-5859en_US
dc.identifier.orcidhttps://orcid.org/0000-0001-8161-2225en_US
dc.identifier.orcidhttps://orcid.org/0000-0002-5471-6202en_US
kusw.oaversionScholarly/refereed, publisher versionen_US
kusw.oapolicyThis item meets KU Open Access policy criteria.en_US
dc.rights.accessrightsopenAccessen_US


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