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Detection of a strongly negative surface potential at Saturn's moon Hyperion
Journal article   Open access   Peer reviewed

Detection of a strongly negative surface potential at Saturn's moon Hyperion

T A Nordheim, G H Jones, E Roussos, J S Leisner, A J Coates, W S Kurth, K K Khurana, N Krupp, M K Dougherty and J H Waite
Geophysical research letters, Vol.41(20), pp.7011-7018
10/28/2014
DOI: 10.1002/2014GL061127
PMCID: PMC4459206
PMID: 26074639
url
https://doi.org/10.1002/2014GL061127View
Published (Version of record) Open Access

Abstract

On 26 September 2005, Cassini conducted its only close targeted flyby of Saturn's small, irregularly shaped moon Hyperion. Approximately 6 min before the closest approach, the electron spectrometer (ELS), part of the Cassini Plasma Spectrometer (CAPS) detected a field-aligned electron population originating from the direction of the moon's surface. Plasma wave activity detected by the Radio and Plasma Wave instrument suggests electron beam activity. A dropout in energetic electrons was observed by both CAPS-ELS and the Magnetospheric Imaging Instrument Low-Energy Magnetospheric Measurement System, indicating that the moon and the spacecraft were magnetically connected when the field-aligned electron population was observed. We show that this constitutes a remote detection of a strongly negative (∼ −200 V) surface potential on Hyperion, consistent with the predicted surface potential in regions near the solar terminator.
Cassini Hyperion Research Letters Saturn's moons surface charging

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