<?xml version='1.0' encoding='utf-8'?>
<oai_dc:dc xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/ http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
  <dc:contributor>R.E. Johnson</dc:contributor>
  <dc:contributor>P.E. Geissler</dc:contributor>
  <dc:contributor>F. Leblanc</dc:contributor>
  <dc:creator>T.A. Cassidy</dc:creator>
  <dc:date>2008</dc:date>
  <dc:description>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. Copyright 2008 by the American Geophysical Union.</dc:description>
  <dc:format>application/pdf</dc:format>
  <dc:identifier>10.1029/2007JE002955</dc:identifier>
  <dc:language>en</dc:language>
  <dc:title>Simulation of Na D emission near Europa during eclipse</dc:title>
  <dc:type>article</dc:type>
</oai_dc:dc>