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Dynamic Plasma Interaction at Io: Multispecies Hybrid Simulations

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F19%3A00519282" target="_blank" >RIV/67985815:_____/19:00519282 - isvavai.cz</a>

  • Result on the web

    <a href="http://hdl.handle.net/11104/0304281" target="_blank" >http://hdl.handle.net/11104/0304281</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1029/2018JA026153" target="_blank" >10.1029/2018JA026153</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Dynamic Plasma Interaction at Io: Multispecies Hybrid Simulations

  • Original language description

    We present analysis of an extensive simulation campaign of the Io plasma interaction under varying interaction conditions performed by using a hybrid multispecies simulation model. We test two models of electron impact ionization, one resulting in plasma production constrained to the upstream hemisphere of Io and the other producing a more symmetric distribution of the plasma with nonnegligible plasma production on the downstream side of To. In the latter case, the simulation model provides high level of agreement with Galileo measurements of magnetic field obtained during the IO flyby, where the model captures even smaller-scale features of the magnetic field profile. Our simulated results provide strong support for the existence of Io's induced dipole field. In this model we assume that induced dipole field moment is antiparallel to the direction of the inducing magnetic field, equivalent to induction in a highly conductive Io. Our results further support the idea that Io's atmosphere collapsed during the Galileo 127 flyby, which manifests itself in the lack of ion heating due to pickup processes in the extended atmosphere.

  • 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

    10308 - Astronomy (including astrophysics,space science)

Result continuities

  • Project

  • Continuities

    I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2019

  • Confidentiality

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

Data specific for result type

  • Name of the periodical

    Journal of Geophysical Research: Space Physics

  • ISSN

    2169-9402

  • e-ISSN

  • Volume of the periodical

    124

  • Issue of the periodical within the volume

    1

  • Country of publishing house

    US - UNITED STATES

  • Number of pages

    29

  • Pages from-to

    313-341

  • UT code for WoS article

    000458729500020

  • EID of the result in the Scopus database

    2-s2.0-85060578540