Juno Plasma Wave Observations at Ganymede
Identifikátory výsledku
Kód výsledku v IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378289%3A_____%2F22%3A00569493" target="_blank" >RIV/68378289:_____/22:00569493 - isvavai.cz</a>
Výsledek na webu
<a href="https://agupubs.onlinelibrary.wiley.com/doi/10.1029/2022GL098591" target="_blank" >https://agupubs.onlinelibrary.wiley.com/doi/10.1029/2022GL098591</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1029/2022GL098591" target="_blank" >10.1029/2022GL098591</a>
Alternativní jazyky
Jazyk výsledku
angličtina
Název v původním jazyce
Juno Plasma Wave Observations at Ganymede
Popis výsledku v původním jazyce
The Juno Waves instrument measured plasma waves associated with Ganymede's magnetosphere during its flyby on 7 June, day 158, 2021. Three distinct regions were identified including a wake, and nightside and dayside regions in the magnetosphere distinguished by their electron densities and associated variability. The magnetosphere includes electron cyclotron harmonic emissions including a band at the upper hybrid frequency, as well as whistler-mode chorus and hiss. These waves likely interact with energetic electrons in Ganymede's magnetosphere by pitch angle scattering and/or accelerating the electrons. The wake is accentuated by low-frequency turbulence and electrostatic solitary waves. Radio emissions observed before and after the flyby likely have their source in Ganymede's magnetosphere.
Název v anglickém jazyce
Juno Plasma Wave Observations at Ganymede
Popis výsledku anglicky
The Juno Waves instrument measured plasma waves associated with Ganymede's magnetosphere during its flyby on 7 June, day 158, 2021. Three distinct regions were identified including a wake, and nightside and dayside regions in the magnetosphere distinguished by their electron densities and associated variability. The magnetosphere includes electron cyclotron harmonic emissions including a band at the upper hybrid frequency, as well as whistler-mode chorus and hiss. These waves likely interact with energetic electrons in Ganymede's magnetosphere by pitch angle scattering and/or accelerating the electrons. The wake is accentuated by low-frequency turbulence and electrostatic solitary waves. Radio emissions observed before and after the flyby likely have their source in Ganymede's magnetosphere.
Klasifikace
Druh
J<sub>imp</sub> - Článek v periodiku v databázi Web of Science
CEP obor
—
OECD FORD obor
10305 - Fluids and plasma physics (including surface physics)
Návaznosti výsledku
Projekt
—
Návaznosti
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace
Ostatní
Rok uplatnění
2022
Kód důvěrnosti údajů
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Údaje specifické pro druh výsledku
Název periodika
Geophysical Research Letters
ISSN
0094-8276
e-ISSN
1944-8007
Svazek periodika
49
Číslo periodika v rámci svazku
23
Stát vydavatele periodika
US - Spojené státy americké
Počet stran výsledku
10
Strana od-do
e2022GL098591
Kód UT WoS článku
000928052000065
EID výsledku v databázi Scopus
2-s2.0-85143728928