File:Altitude profile for H2+ PUIs, Europa moon.png
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From the study "Oxygen production from dissociation of Europa’s water-ice surface"
Summary
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| Description |
English: "H2+ density coloured by XEPhiO such that densities observed upstream from the centre of Europa are blue and are red or orange downstream. The outbound portion of the trajectory, ‘Fit’ in the inset, is compared to a PUI advection solution (Methods). Overlaid curves show PUI densities corresponding to the advection solution for a PUI population from: (1) an ionized neutral atmosphere varying as exp(−h/λ)r−2 where λ = 6,090 ± 890 km (grey), (2) scaled from a comprehensive DSMC atmosphere model (blue)3 and (3) scaled from a sputtered-only model (purple)20. The grey region at the bottom shows the expected density of Europa-genic H2+ PUIs already incorporated into Jupiter’s magnetospheric plasma29.
Source data" |
| Date | |
| Source | https://www.nature.com/articles/s41550-024-02206-x |
| Author | Authors of the study: J. R. Szalay, F. Allegrini, R. W. Ebert, F. Bagenal, S. J. Bolton, S. Fatemi, D. J. McComas, A. Pontoni, J. Saur, H. T. Smith, D. F. Strobel, S. D. Vance, A. Vorburger & R. J. Wilson |
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| current | 13:19, 1 June 2024 | | 1,559 × 1,154 (208 KB) | Prototyperspective (talk | contribs) | Uploaded a work by Authors of the study: J. R. Szalay, F. Allegrini, R. W. Ebert, F. Bagenal, S. J. Bolton, S. Fatemi, D. J. McComas, A. Pontoni, J. Saur, H. T. Smith, D. F. Strobel, S. D. Vance, A. Vorburger & R. J. Wilson from https://www.nature.com/articles/s41550-024-02206-x with UploadWizard |
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