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Empirical Photochemical Modeling of Saturn's Ionization Balance Including Grain Charging
Uppsala universitet, Teknisk-naturvetenskapliga vetenskapsområdet, Fysiska sektionen, Institutet för rymdfysik, Uppsalaavdelningen.ORCID-id: 0000-0003-2647-8259
Uppsala universitet, Teknisk-naturvetenskapliga vetenskapsområdet, Fysiska sektionen, Institutet för rymdfysik, Uppsalaavdelningen.ORCID-id: 0000-0003-3038-3359
Uppsala universitet, Teknisk-naturvetenskapliga vetenskapsområdet, Fysiska sektionen, Institutet för rymdfysik, Uppsalaavdelningen.ORCID-id: 0000-0003-2926-6761
Uppsala universitet, Teknisk-naturvetenskapliga vetenskapsområdet, Fysiska sektionen, Institutet för rymdfysik, Uppsalaavdelningen.ORCID-id: 0000-0002-5386-8255
Vise andre og tillknytning
2022 (engelsk)Inngår i: The Planetary Science Journal, E-ISSN 2632-3338, Vol. 3, nr 2, artikkel-id 49Artikkel i tidsskrift (Fagfellevurdert) Published
Abstract [en]

We present a semianalytical photochemical model of Saturn's near-equatorial ionosphere and adapt it to two regions (similar to 2200 and similar to 1700 km above the 1 bar level) probed during the inbound portion of Cassini's orbit 292 (2017 September 9). The model uses as input the measured concentrations of molecular hydrogen, hydrogen ion species, and free electrons, as well as the measured electron temperature. The output includes upper limits, or constraints, on the mixing ratios of two families of molecules, on ion concentrations, and on the attachment rates of electrons and ions onto dust grains. The model suggests mixing ratios of the two molecular families that, particularly near similar to 1700 km, differ notably from what independent measurements by the Ion Neutral Mass Spectrometer suggest. Possibly connected to this, the model suggests an electron-depleted plasma with a level of electron depletion of around 50%. This is in qualitative agreement with interpretations of Radio Plasma Wave Science/Langmuir Probe measurements, but an additional conundrum arises in the fact that a coherent photochemical equilibrium scenario then relies on a dust component with typical grain radii smaller than 3 angstrom.

sted, utgiver, år, opplag, sider
Institute of Physics (IOP), 2022. Vol. 3, nr 2, artikkel-id 49
HSV kategori
Identifikatorer
URN: urn:nbn:se:uu:diva-495353DOI: 10.3847/PSJ/ac4eeeISI: 000911845800001OAI: oai:DiVA.org:uu-495353DiVA, id: diva2:1732041
Forskningsfinansiär
Swedish National Space BoardTilgjengelig fra: 2023-01-30 Laget: 2023-01-30 Sist oppdatert: 2023-10-03bibliografisk kontrollert
Inngår i avhandling
1. Diving Deep into Saturn's Equatorial Ionosphere with Cassini: Insights from the Grand Finale
Åpne denne publikasjonen i ny fane eller vindu >>Diving Deep into Saturn's Equatorial Ionosphere with Cassini: Insights from the Grand Finale
2023 (engelsk)Doktoravhandling, med artikler (Annet vitenskapelig)
Abstract [en]

In the summer of 2017, the Cassini mission concluded its nearly 13 years orbiting Saturn with a series of daring dives between the rings and the upper reaches of Saturn's atmosphere. This last phase of the mission, called the Grand Finale, revealed a highly variable equatorial ionosphere dominated by a large influx of ring material from Saturn's D ring. The papers included in this thesis utilize data gathered during these proximal orbits to gain insights into the nature and effects of the infalling ring material.

Initially, we derive upper limits for the effective recombination coefficient in Saturn's equatorial ionosphere at altitudes below 2500 km, where photochemical equilibrium can be assumed, to constrain the composition of the positive ion species. Our inceptive results indicate that ion species with low recombination coefficients are dominant.

We follow up on this by developing a photochemical model, incorporating grain charging, to investigate the effects of the ring influx on the plasma composition. The model results at an altitude of 1700 km yield vastly different abundances of two types of neutral species when compared to those derived from measurements, ultimately representing the difficulty of reconciling the observed H+ and H3+ densities with our and other model results.

Exploring the nature of narrow decreases in the ionospheric H2+ densities reveals a time shift in the ion data. After correcting for this, the decreases line up very well with calculated shadows for substructures in Saturn's C ring. We can further estimate the optical depths of these substructures and investigate at which altitudes photochemical equilibrium for H2+ is applicable.

The direct measurement of heavier neutral species during the proximal orbits is complicated by the high spacecraft speed. We devise a method to utilize helium ion chemistry to independently derive the mixing ratios of these heavier neutrals in Saturn's ionosphere. Our results show considerable variability, which may suggest temporal and/or spatial changes in the ring influx. A comparison with other studies indicates that potentially only the most volatile ring-sourced species significantly ablate to enter the gas phase in this region of Saturn's ionosphere.

Finally, we compare the fixed-bias Langmuir probe electron densities and the light ion densities. They exhibit a strong positive correlation for most parts of the proximal orbits even on short timescales. We find three distinct regions in the proximal orbits, which can provide further insight into the ionospheric composition, connection to the rings, and measurement uncertainties.

sted, utgiver, år, opplag, sider
Uppsala: Acta Universitatis Upsaliensis, 2023. s. 59
Serie
Digital Comprehensive Summaries of Uppsala Dissertations from the Faculty of Science and Technology, ISSN 1651-6214 ; 2313
Emneord
Saturn, Cassini, Grand Finale, Ionosphere, Photochemistry, Planetary Rings, Planetary Science, Space Plasma, Space Physics
HSV kategori
Forskningsprogram
Fysik med inriktning mot rymd- och plasmafysik
Identifikatorer
urn:nbn:se:uu:diva-512834 (URN)978-91-513-1910-0 (ISBN)
Disputas
2023-11-23, Sonja Lyttkens (101121), Ångströmlaboratoriet, Lägerhyddsvägen 1, Uppsala, 13:00 (engelsk)
Opponent
Veileder
Forskningsfinansiär
Swedish National Space Board, 143/18
Tilgjengelig fra: 2023-11-02 Laget: 2023-10-03 Sist oppdatert: 2023-11-02

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Vigren, ErikDreyer, JoshuaEriksson, Anders I.Johansson, Fredrik L.Morooka, MichikoWahlund, Jan-Erik

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