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Evidence for low density holes in Jupiter’s ionosphere

Masafumi Imai (), Ivana Kolmašová, William S. Kurth, Ondřej Santolík, George B. Hospodarsky, Donald A. Gurnett, Shannon T. Brown, Scott J. Bolton, John E. P. Connerney and Steven M. Levin
Additional contact information
Masafumi Imai: University of Iowa
Ivana Kolmašová: The Czech Academy of Sciences
William S. Kurth: University of Iowa
Ondřej Santolík: The Czech Academy of Sciences
George B. Hospodarsky: University of Iowa
Donald A. Gurnett: University of Iowa
Shannon T. Brown: California Institute of Technology
Scott J. Bolton: Southwest Research Institute
John E. P. Connerney: Space Research Corporation
Steven M. Levin: California Institute of Technology

Nature Communications, 2019, vol. 10, issue 1, 1-6

Abstract: Abstract Intense electromagnetic impulses induced by Jupiter’s lightning have been recognised to produce both low-frequency dispersed whistler emissions and non-dispersed radio pulses. Here we report the discovery of electromagnetic pulses associated with Jovian lightning. Detected by the Juno Waves instrument during its polar perijove passes, the dispersed millisecond pulses called Jupiter dispersed pulses (JDPs) provide evidence of low density holes in Jupiter’s ionosphere. 445 of these JDP emissions have been observed in snapshots of electric field waveforms. Assuming that the maximum delay occurs in the vicinity of the free space ordinary mode cutoff frequency, we estimate the characteristic plasma densities (5.1 to 250 cm−3) and lengths (0.6 km to 1.3 × 105 km) of plasma irregularities along the line of propagation from lightning to Juno. These irregularities show a direct link to low plasma density holes with ≤250 cm−3 in the nightside ionosphere.

Date: 2019
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DOI: 10.1038/s41467-019-10708-w

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