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
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Czech description
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Classification
Type
J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database
CEP classification
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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
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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