SwePub
Sök i LIBRIS databas

  Extended search

L773:0004 2021
 

Search: L773:0004 2021 > Exact hybrid-kineti...

Exact hybrid-kinetic equilibria for magnetized plasmas with shearing flows

Guzzi, G. (author)
Univ Calabria, Dipartimento Fis, Cubo 31C, I-87036 Arcavacata Di Rende, CS, Italy.
Settino, Adriana (author)
Uppsala universitet,Institutet för rymdfysik, Uppsalaavdelningen,Univ Calabria, Dipartimento Fis, Cubo 31C, I-87036 Arcavacata Di Rende, CS, Italy.
Valentini, F. (author)
Univ Calabria, Dipartimento Fis, Cubo 31C, I-87036 Arcavacata Di Rende, CS, Italy.
show more...
Malara, F. (author)
Univ Calabria, Dipartimento Fis, Cubo 31C, I-87036 Arcavacata Di Rende, CS, Italy.
show less...
Univ Calabria, Dipartimento Fis, Cubo 31C, I-87036 Arcavacata Di Rende, CS, Italy Institutet för rymdfysik, Uppsalaavdelningen (creator_code:org_t)
2021-01-27
2021
English.
In: Astronomy and Astrophysics. - : EDP Sciences. - 0004-6361 .- 1432-0746. ; 645
  • Journal article (peer-reviewed)
Abstract Subject headings
Close  
  • Context. Magnetized plasmas characterized by shearing flows are present in many natural contexts, such as the Earth's magnetopause and the solar wind. The collisionless nature of involved plasmas requires a kinetic description. When the width of the shear layer is on the order of ion scales, the hybrid Vlasov-Maxwell approach can be adopted for this purpose.Aims. The aim of this work is to derive explicit forms for stationary configurations of magnetized plasmas with planar shearing flows within the hybrid Vlasov-Maxwell description. Two configurations are considered: the first with a uniform magnetic field obliquely directed with respect to the bulk velocity and the second with a uniform-magnitude variable-direction magnetic field.Methods. We obtained stationary ion distribution functions by combining single-particle constant of motions, which are derived through the study of particle dynamics. Preliminary information about the form of the distribution functions were analytically derived in considering a local approximation for the background electromagnetic field. Then a numerical method was set up to obtain a solution for general profiles.Results. We determined explicit distribution functions that allow us to obtain profiles of density, bulk velocity, temperature, and heat flux. Anisotropy and agyrotropy in the distribution function were also evaluated. The stationarity of the solution during numerical simulations was checked in the uniform oblique magnetic field case.Conclusions. The configurations considered here can be used as models for the Earth's magnetopause in simulations of the Kelvin-Helmholtz instability.

Subject headings

NATURVETENSKAP  -- Fysik -- Fusion, plasma och rymdfysik (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Fusion, Plasma and Space Physics (hsv//eng)
NATURVETENSKAP  -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)

Keyword

plasmas
magnetic fields
turbulence
instabilities
waves
interplanetary medium

Publication and Content Type

ref (subject category)
art (subject category)

Find in a library

To the university's database

Find more in SwePub

By the author/editor
Guzzi, G.
Settino, Adriana
Valentini, F.
Malara, F.
About the subject
NATURAL SCIENCES
NATURAL SCIENCES
and Physical Science ...
and Fusion Plasma an ...
NATURAL SCIENCES
NATURAL SCIENCES
and Physical Science ...
and Astronomy Astrop ...
Articles in the publication
Astronomy and As ...
By the university
Uppsala University

Search outside SwePub

Kungliga biblioteket hanterar dina personuppgifter i enlighet med EU:s dataskyddsförordning (2018), GDPR. Läs mer om hur det funkar här.
Så här hanterar KB dina uppgifter vid användning av denna tjänst.

 
pil uppåt Close

Copy and save the link in order to return to this view