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Cassini RPWS Dust Observation Near the Janus/Epimetheus Orbit
Journal article   Open access   Peer reviewed

Cassini RPWS Dust Observation Near the Janus/Epimetheus Orbit

S. -Y. Ye, W. S. Kurth, G. B. Hospodarsky, A. M. Persoon, D. A. Gurnett, M. Morooka, J. -E. Wahlund, H. -W. Hsu, M. Seiss and R. Srama
Journal of geophysical research. Space physics, Vol.123(6), pp.4952-4960
06/01/2018
DOI: 10.1029/2017JA025112
url
https://doi.org/10.1029/2017JA025112View
Published (Version of record) Open Access

Abstract

During the Ring Grazing orbits near the end of Cassini mission, the spacecraft crossed the equatorial plane near the orbit of Janus/Epimetheus (similar to 2.5 Rs). This region is populated with dust particles that can be detected by the Radio and Plasma Wave Science (RPWS) instrument via an electric field antenna signal. Analysis of the voltage waveforms recorded on the RPWS antennas provides estimations of the density and size distribution of the dust particles. Measured RPWS profiles, fitted with Lorentzian functions, are shown to be mostly consistent with the Cosmic Dust Analyzer, the dedicated dust instrument on board Cassini. The thickness of the dusty ring varies between 600 and 1,000 km. The peak location shifts north and south within 100 km of the ring plane, likely a function of the precession phase of Janus orbit.
Astronomy & Astrophysics Physical Sciences Science & Technology

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