uu.seUppsala University Publications
Change search
CiteExportLink to record
Permanent link

Direct link
Cite
Citation style
  • apa
  • ieee
  • modern-language-association
  • vancouver
  • Other style
More styles
Language
  • de-DE
  • en-GB
  • en-US
  • fi-FI
  • nn-NO
  • nn-NB
  • sv-SE
  • Other locale
More languages
Output format
  • html
  • text
  • asciidoc
  • rtf
Turbulence-Driven Ion Beams in the Magnetospheric Kelvin-Helmholtz Instability
UOS Cosenza, Nanotec CNR, Cubo 31C, I-87036 Arcavacata Di Rende, Italy;Escuela Politec Nacl, Dept Fis, Quito 170517, Ecuador.
Univ Calabria, Dipartimento Fis, Cubo 31C, I-87036 Arcavacata Di Rende, Italy;Sorbonne Univ, Ecole Polytech, CNRS, LPP, F-91128 Palaiseau, France.
Sorbonne Univ, Ecole Polytech, CNRS, LPP, F-91128 Palaiseau, France.
Sorbonne Univ, Ecole Polytech, CNRS, LPP, F-91128 Palaiseau, France.
Show others and affiliations
2019 (English)In: Physical Review Letters, ISSN 0031-9007, E-ISSN 1079-7114, Vol. 122, no 3, article id 035102Article in journal (Refereed) Published
Abstract [en]

The description of the local turbulent energy transfer and the high-resolution ion distributions measured by the Magnetospheric Multiscale mission together provide a formidable tool to explore the cross-scale connection between the fluid-scale energy cascade and plasma processes at subion scales. When the small-scale energy transfer is dominated by Alfvenic, correlated velocity, and magnetic field fluctuations, beams of accelerated particles are more likely observed. Here, for the first time, we report observations suggesting the nonlinear wave-particle interaction as one possible mechanism for the energy dissipation in space plasmas.

Place, publisher, year, edition, pages
AMER PHYSICAL SOC , 2019. Vol. 122, no 3, article id 035102
National Category
Astronomy, Astrophysics and Cosmology
Identifiers
URN: urn:nbn:se:uu:diva-376817DOI: 10.1103/PhysRevLett.122.035102ISI: 000456782500006OAI: oai:DiVA.org:uu-376817DiVA, id: diva2:1289978
Available from: 2019-02-19 Created: 2019-02-19 Last updated: 2019-02-19Bibliographically approved

Open Access in DiVA

No full text in DiVA

Other links

Publisher's full text

Authority records BETA

Khotyaintsev, Yuri V.

Search in DiVA

By author/editor
Khotyaintsev, Yuri V.
By organisation
Swedish Institute of Space Physics, Uppsala Division
In the same journal
Physical Review Letters
Astronomy, Astrophysics and Cosmology

Search outside of DiVA

GoogleGoogle Scholar

doi
urn-nbn

Altmetric score

doi
urn-nbn
Total: 6 hits
CiteExportLink to record
Permanent link

Direct link
Cite
Citation style
  • apa
  • ieee
  • modern-language-association
  • vancouver
  • Other style
More styles
Language
  • de-DE
  • en-GB
  • en-US
  • fi-FI
  • nn-NO
  • nn-NB
  • sv-SE
  • Other locale
More languages
Output format
  • html
  • text
  • asciidoc
  • rtf