Ion cyclotron instability at Io: Hybrid simulation results compared to in situ observations

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F16%3A00471451" target="_blank" >RIV/67985815:_____/16:00471451 - isvavai.cz</a>
Alternative codes found
RIV/68378289:_____/16:00465320
Result on the web
<a href="http://dx.doi.org/10.1002/2016JA022477" target="_blank" >http://dx.doi.org/10.1002/2016JA022477</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1002/2016JA022477" target="_blank" >10.1002/2016JA022477</a>

Result language
angličtina
Original language name
Ion cyclotron instability at Io: Hybrid simulation results compared to in situ observations
Original language description
We present analysis of global three-dimensional hybrid simulations of Io's interaction with Jovian magnetospheric plasma. We apply a single-species model with simplified neutral-plasma chemistry and downscale Io in order to resolve the ion kinetic scales. We consider charge exchange, electron impact ionization, and photoionization by using variable rates of these processes to investigate their impact. Our results are in a good qualitative agreement with the in situ magnetic field measurements for five Galileo flybys around Io.
Czech name
—
Czech description
—

Type
J<sub>x</sub> - Unclassified - Peer-reviewed scientific article (Jimp, Jsc and Jost)
CEP classification
BN - Astronomy and celestial mechanics, astrophysics
OECD FORD branch
—

Project
—
Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Publication year
2016
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Similar results(10)