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Sökning: WFRF:(Chaufray Y. Y) > Ganymede's atmosphe...

  • Leblanc, F.Sorbonne Univ, LATMOS, CNRS, UVSQ, Paris, France. (författare)

Ganymede's atmosphere as constrained by HST/STIS observations

  • Artikel/kapitelEngelska2023

Förlag, utgivningsår, omfång ...

  • Elsevier BV,2023
  • printrdacarrier

Nummerbeteckningar

  • LIBRIS-ID:oai:DiVA.org:kth-327187
  • https://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-327187URI
  • https://doi.org/10.1016/j.icarus.2023.115557DOI

Kompletterande språkuppgifter

  • Språk:engelska
  • Sammanfattning på:engelska

Ingår i deldatabas

Klassifikation

  • Ämneskategori:ref swepub-contenttype
  • Ämneskategori:art swepub-publicationtype

Anmärkningar

  • QC 20230523
  • A new analysis of aurora observations of Ganymede's atmosphere on the orbital leading and trailing hemispheres has been recently published by Roth et al. (2021), suggesting that water is its main constituent near noon. Here, we present two additional aurora observations of Ganymede's sub-Jovian and anti-Jovian hemispheres, which suggest a modulation of the atmospheric H2O/O-2 ratio on the moon's orbital period, and analyze the orbital evolution of the atmosphere. For this, we propose a reconstruction of aurora observations based on a physical modelling of the exosphere taking into account its orbital variability (the Exospheric Global Model; Leblanc et al., 2017). The solution described in this paper agrees with Roth et al. (2021) that Ganymede's exosphere should be dominantly composed of water molecules. From Ganymede's position when its leading hemisphere is illuminated to when it is its trailing hemisphere, the column density of O-2 may vary between 4.3 x 10(14) and 3.6 x 10(14) cm(-2) whereas the H2O column density should vary between 5.6 x 10(14) and 1.3 x 10(15) cm(-2). The water content of Ganymede's atmosphere is essentially constrained by its sublimation rate whereas the O-2 component of Ganymede's atmosphere is controlled by the radiolytic yield. The other species, products of the water molecules, vary in a more complex way depending on their sources, either as ejecta from the surface and/or as product of the dissociation of the other atmospheric constituents. Electron impact on H2O and H-2 molecules is shown to likely produce H Lyman-alpha emissions close to Ganymede, in addition to the observed extended Lyman-alpha corona from H resonant scattering. All these conclusions being highly dependent on our capability to accurately model the origins of the observed Ganymede auroral emissions, modelling these emissions remains poorly constrained without an accurate knowledge of the Jovian magnetospheric and Ganymede ionospheric electron populations.

Ämnesord och genrebeteckningar

Biuppslag (personer, institutioner, konferenser, titlar ...)

  • Roth, LorenzKTH,Rymd- och plasmafysik(Swepub:kth)u1ml3zu9 (författare)
  • Chaufray, J. Y.Sorbonne Univ, LATMOS, CNRS, UVSQ, Paris, France. (författare)
  • Modolo, R.Sorbonne Univ, LATMOS, CNRS, UVSQ, Paris, France. (författare)
  • Galand, M.Imperial Coll London, Dept Phys, London, England. (författare)
  • Ivchenko, NatalyaKTH,Rymd- och plasmafysik(Swepub:kth)u1x7xhc4 (författare)
  • Carnielli, G.Imperial Coll London, Dept Phys, London, England. (författare)
  • Baskevitch, C.Sorbonne Univ, LATMOS, CNRS, UVSQ, Paris, France. (författare)
  • Oza, A.CALTECH, Jet Prop Lab, Pasadena, CA USA. (författare)
  • Werner, A. L. E.Sorbonne Univ, LATMOS, CNRS, UVSQ, Paris, France.;Swedish Inst Space Phys, Uppsala, Sweden. (författare)
  • Sorbonne Univ, LATMOS, CNRS, UVSQ, Paris, France.Rymd- och plasmafysik (creator_code:org_t)

Sammanhörande titlar

  • Ingår i:Icarus: Elsevier BV3990019-10351090-2643

Internetlänk

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  • Icarus (Sök värdpublikationen i LIBRIS)

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