Published July 4, 2020 | Version v3
Dataset Open

High-Spatiotemporal Resolution Observations of Jupiter Lightning-Induced Radio Pulses Associated With Sferics and Thunderstorms

  • 1. Department of Physics and Astronomy, University of Iowa, Iowa City, Iowa, USA; Department of Electrical Engineering and Information Science, National Institute of Technology (KOSEN), Niihama College, Niihama, Ehime, Japan
  • 2. SETI Institute, Mountain View, California, USA; Astronomy Department, University of California, Berkeley, California, USA
  • 3. Department of Space Physics, Institute of Atmospheric Physics, The Czech Academy of Sciences, Prague, Czechia; Faculty of Mathematics and Physics, Charles University, Prague, Czechia
  • 4. Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California, USA
  • 5. Department of Physics and Astronomy, University of Iowa, Iowa City, Iowa, USA
  • 6. Space Science and Engineering Division, Southwest Research Institute, San Antonio, Texas, USA

Description

Abstract:
Jupiter lightning discharges produce various kinds of phenomena including radio wave pulses at different frequencies. On 6 April 2019, the Juno Waves instrument captured an extraordinary series of radio pulses at frequencies below 150 kHz on timescales of submilliseconds. Quasi-simultaneous multi-instrument data show that the locations of their magnetic footprints are very close to the locations of UHF sferics recorded by the Juno MWR instrument. Hubble Space Telescope images show that the signature of active convection includes cloud-free clearings, in addition to the convective towers and deep water clouds that were also recognized in previous spacecraft observations of lightning source regions. Furthermore, the detections of 17 VLF/LF radio pulses suggest a minimum duration of lightning processes on the order of submilliseconds. These observations provide new constraints on the physical properties of Jupiter lightning.

Note:
This paper was published in Geophysical Research Letters (https://doi.org/10.1029/2020GL088397). This page provides the digital data for all figures in this paper; please read a readme file in each figure sub-directory.

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