Simulation of Na D emission near Europa during eclipse
Résumé
The Cassini imaging science subsystem observed Europa in eclipse during Cassini's Jupiter flyby. The disk-resolved observations revealed a spatially nonuniform emission in the wavelength range of 200–1050 nm (clear filters). By building on observations and simulations of Europa's Na atmosphere and torus we find that electron-excited Na in Europa's tenuous atmosphere can account for the observed emission if the Na is ejected preferentially from Europa's dark terrain
Domaines
Océan, Atmosphère
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Cassidy_et_al-2008-Journal_of_Geophysical_Research__Solid_Earth_(1978-2012).pdf (175.25 Ko)
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