Back to Search Start Over

The composition and structure of the Enceladus plume

Authors :
Brenton Lewis
Brian Magee
Robert A. West
J. H. Waite
A. I. F. Stewart
Donald E. Shemansky
Joshua Colwell
Larry W. Esposito
B. D. Teolis
Amanda R. Hendrix
Candice Hansen
Source :
Geophysical Research Letters. 38
Publication Year :
2011
Publisher :
American Geophysical Union (AGU), 2011.

Abstract

[1] The Cassini Ultraviolet Imaging Spectrograph (UVIS) observed an occultation of the Sun by the water vapor plume at the south polar region of Saturn's moon Enceladus. The Extreme Ultraviolet (EUV) spectrum is dominated by the spectral signature of H2O gas, with a nominal line-of-sight column density of 0.90 ± 0.23 × 1016 cm−2 (upper limit of 1.0 × 1016 cm−2). The upper limit for N2 is 5 × 1013 cm−2, or

Details

ISSN :
00948276
Volume :
38
Database :
OpenAIRE
Journal :
Geophysical Research Letters
Accession number :
edsair.doi...........fba75650d9eefaaaeb534457986ed3f1
Full Text :
https://doi.org/10.1029/2011gl047415