Laboratory evidence for proton energization by collisionless shock surfing

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378271%3A_____%2F21%3A00552176" target="_blank" >RIV/68378271:_____/21:00552176 - isvavai.cz</a>
Result on the web
<a href="https://doi.org/10.1038/s41567-021-01325-w" target="_blank" >https://doi.org/10.1038/s41567-021-01325-w</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1038/s41567-021-01325-w" target="_blank" >10.1038/s41567-021-01325-w</a>

Result language
angličtina
Original language name
Laboratory evidence for proton energization by collisionless shock surfing
Original language description
Charged particles can be accelerated to high energies by collisionless shock waves in astrophysical environments, such as supernova remnants. By interacting with the magnetized ambient medium, these shocks can transfer energy to particles. Despite increasing efforts in the characterization of these shocks from satellite measurements at Earth’s bow shock as well as powerful numerical simulations, the underlying acceleration mechanism or a combination thereof is still widely debated. Here we show that astrophysically relevant super-critical quasi-perpendicular magnetized collisionless shocks can be produced and characterized in the laboratory.n
Czech name
—
Czech description
—

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)

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

Publication year
2021
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Similar results(10)