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Discovery of rapid whistlers close to Jupiter implying lightning rates similar to those on Earth

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216208%3A11320%2F18%3A10389441" target="_blank" >RIV/00216208:11320/18:10389441 - isvavai.cz</a>

  • Alternative codes found

    RIV/68378289:_____/18:00490176

  • Result on the web

    <a href="https://doi.org/10.1038/s41550-018-0442-z" target="_blank" >https://doi.org/10.1038/s41550-018-0442-z</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1038/s41550-018-0442-z" target="_blank" >10.1038/s41550-018-0442-z</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Discovery of rapid whistlers close to Jupiter implying lightning rates similar to those on Earth

  • Original language description

    Electrical currents in atmospheric lightning strokes generate impulsive radio waves in a broad range of frequencies, called atmospherics. These waves can be modified by their passage through the plasma environment of a planet into the form of dispersed whistlers(1). In the Io plasma torus around Jupiter, Voyager 1 detected whistlers as several-seconds-long slowly falling tones at audible frequencies(2). These measurements were the first evidence of lightning at Jupiter. Subsequently, Jovian lightning was observed by optical cameras on board several spacecraft in the form of localized flashes of light(3-7). Here, we show measurements by the Waves instrument(8) on board the Juno spacecraft(9-11) that indicate observations of Jovian rapid whistlers: a form of dispersed atmospherics at extremely short timescales of several milliseconds to several tens of milliseconds. On the basis of these measurements, we report over 1,600 lightning detections, the largest set obtained to date. The data were acquired during close approaches to Jupiter between August 2016 and September 2017, at radial distances below 5 Jovian radii. We detected up to four lightning strokes per second, similar to rates in thunderstorms on Earth(12) and six times the peak rates from the Voyager 1 observations(13).

  • Czech name

  • Czech description

Classification

  • Type

    J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database

  • CEP classification

  • OECD FORD branch

    10305 - Fluids and plasma physics (including surface physics)

Result continuities

  • Project

    <a href="/en/project/LTAUSA17070" target="_blank" >LTAUSA17070: Electromagnetic waves in planetary ionospheres and magnetospheres</a><br>

  • Continuities

    P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)<br>I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2018

  • Confidentiality

    S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Data specific for result type

  • Name of the periodical

    Nature Astronomy

  • ISSN

    2397-3366

  • e-ISSN

  • Volume of the periodical

    2

  • Issue of the periodical within the volume

    7

  • Country of publishing house

    GB - UNITED KINGDOM

  • Number of pages

    5

  • Pages from-to

    544-548

  • UT code for WoS article

    000437959800016

  • EID of the result in the Scopus database

    2-s2.0-85048235667