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The low-frequency source of Saturn’s kilometric radiation
Journal article   Open access   Peer reviewed

The low-frequency source of Saturn’s kilometric radiation

L. Lamy, P. Zarka, B. Cecconi, R. Prangé, W. Kurth, G. Hospodarsky, A. Persoon, M. Morooka, J.-E. Wahlund and G. Hunt
Science (American Association for the Advancement of Science), Vol.362(6410), p.2027
10/05/2018
DOI: 10.1126/science.aat2027
PMID: 30287632
url
https://doi.org/10.1126/science.aat2027View
Published (Version of record) Open Access

Abstract

Understanding how auroral radio emissions are produced by magnetized bodies requires in situ measurements within their source region. Saturn’s kilometric radiation (SKR) has been widely used as a remote proxy of Saturn’s magnetosphere. We present wave and plasma measurements from the Cassini spacecraft during its ring-grazing high-inclination orbits, which passed three times through the high-altitude SKR emission region. Northern dawn-side, narrow-banded radio sources were encountered at frequencies of 10 to 20 kilohertz, within regions of upward currents mapping to the ultraviolet auroral oval. The kilometric waves were produced on the extraordinary mode by the cyclotron maser instability from 6– to 12–kilo–electron volt electron beams and radiated quasi-perpendicularly to the auroral magnetic field lines. The SKR low-frequency sources appear to be strongly controlled by time-variable magnetospheric electron densities.
Astrophysics Instrumentation and Methods for Astrophysic Physics

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