Title
The auroral footprint of Enceladus on Saturn
Abbreviated Journal Title
Nature
Keywords
IO FLUX TUBE; CASSINI; ATMOSPHERE; MAGNETOSPHERE; SPECTROMETER; JUPITER; ORIGIN; PLASMA; PLUME; Multidisciplinary Sciences
Abstract
Although there are substantial differences between the magnetospheres of Jupiter and Saturn, it has been suggested that cryovolcanic activity at Enceladus(1-9) could lead to electrodynamic coupling between Enceladus and Saturn like that which links Jupiter with Io, Europa and Ganymede. Powerful field-aligned electron beams associated with the Io-Jupiter coupling, for example, create an auroral footprint in Jupiter's ionosphere(10,11). Auroral ultraviolet emission associated with Enceladus-Saturn coupling is anticipated to be just a few tenths of a kilorayleigh (ref. 12), about an order of magnitude dimmer than Io's footprint and below the observable threshold, consistent with its non-detection(13). Here we report the detection of magnetic-field-aligned ion and electron beams (offset several moon radii downstream from Enceladus) with sufficient power to stimulate detectable aurora, and the subsequent discovery of Enceladus-associated aurora in a few per cent of the scans of the moon's footprint. The footprint varies in emission magnitude more than can plausibly be explained by changes in magnetospheric parameters-and as such is probably indicative of variable plume activity.
Journal Title
Nature
Volume
472
Issue/Number
7343
Publication Date
1-1-2011
Document Type
Article
Language
English
First Page
331
Last Page
333
WOS Identifier
ISSN
0028-0836
Recommended Citation
"The auroral footprint of Enceladus on Saturn" (2011). Faculty Bibliography 2010s. 1781.
https://stars.library.ucf.edu/facultybib2010/1781
Comments
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