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Latitudinal beaming of Jovian decametric radio emissions as viewed from Juno and the Nançay Decameter Array
Journal article   Open access   Peer reviewed

Latitudinal beaming of Jovian decametric radio emissions as viewed from Juno and the Nançay Decameter Array

Masafumi Imai, William S. Kurth, George B. Hospodarsky, Scott J. Bolton, John E. P. Connerney, Steven M. Levin, Alain Lecacheux, Laurent Lamy and Philippe Zarka
Geophysical research letters, Vol.44(10), pp.4455-4462
05/28/2017
DOI: 10.1002/2016GL072454
url
https://doi.org/10.1002/2016GL072454View
Published (Version of record) Open Access

Abstract

Two well‐defined Jovian decametric radio arcs were observed at latitudinal separations of 11°–16° from the Juno spacecraft near Jupiter and the Nançay Decameter Array (NDA) at Earth on 17 May and 25 August 2016. These discrete arcs are from the so‐called A source covering both Io‐related and non‐Io‐related emissions. By measuring the wave arrival time at two distant observers with propagation time correction, the remaining delay times are 92.8 ± 1.3 min for the first arc and 116.0 ± 1.2 min for the second arc. This implies that both radio sources are not controlled by the orbital motion of Io but Jupiter's rotation itself. The geometrical information for Juno and NDA and the loss cone‐driven electron cyclotron maser instability theory provide these radio sources that are located at about 173° ± 10° in system III longitude projected onto Jupiter's north surface and imply resonant electron energy ranges from 0.5 to 11 keV. Key Points Two decametric (DAM) arcs were observed from widely spaced latitudes by Juno and NDA Direct evidence of long‐lasting DAM arcs corotating with Jupiter is presented The loss cone‐driven CMI theory of fundamental X‐mode emission provides a constraint of the concurrent arcs
decametric radio emissions Juno Jupiter NDA stereoscopic observations waves

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