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Characterization of Quasi-Keplerian, Differentially Rotating, Free-Boundary Laboratory Plasmas.
Valenzuela-Villaseca, V; Suttle, L G; Suzuki-Vidal, F; Halliday, J W D; Merlini, S; Russell, D R; Tubman, E R; Hare, J D; Chittenden, J P; Koepke, M E; Blackman, E G; Lebedev, S V.
Afiliación
  • Valenzuela-Villaseca V; Blackett Laboratory, Imperial College London, London SW7 2BW, United Kingdom.
  • Suttle LG; Blackett Laboratory, Imperial College London, London SW7 2BW, United Kingdom.
  • Suzuki-Vidal F; Blackett Laboratory, Imperial College London, London SW7 2BW, United Kingdom.
  • Halliday JWD; Blackett Laboratory, Imperial College London, London SW7 2BW, United Kingdom.
  • Merlini S; Blackett Laboratory, Imperial College London, London SW7 2BW, United Kingdom.
  • Russell DR; Blackett Laboratory, Imperial College London, London SW7 2BW, United Kingdom.
  • Tubman ER; Blackett Laboratory, Imperial College London, London SW7 2BW, United Kingdom.
  • Hare JD; Blackett Laboratory, Imperial College London, London SW7 2BW, United Kingdom.
  • Chittenden JP; Blackett Laboratory, Imperial College London, London SW7 2BW, United Kingdom.
  • Koepke ME; Department of Physics, West Virginia University, Morgantown, West Virginia 26506, USA.
  • Blackman EG; Department of Physics and Astronomy, University of Rochester, Rochester, New York 14627, USA.
  • Lebedev SV; Blackett Laboratory, Imperial College London, London SW7 2BW, United Kingdom.
Phys Rev Lett ; 130(19): 195101, 2023 May 12.
Article en En | MEDLINE | ID: mdl-37243644
ABSTRACT
We present results from pulsed-power driven differentially rotating plasma experiments designed to simulate physics relevant to astrophysical disks and jets. In these experiments, angular momentum is injected by the ram pressure of the ablation flows from a wire array Z pinch. In contrast to previous liquid metal and plasma experiments, rotation is not driven by boundary forces. Axial pressure gradients launch a rotating plasma jet upward, which is confined by a combination of ram, thermal, and magnetic pressure of a surrounding plasma halo. The jet has subsonic rotation, with a maximum rotation velocity 23±3 km/s. The rotational velocity profile is quasi-Keplerian with a positive Rayleigh discriminant κ^{2}∝r^{-2.8±0.8} rad^{2}/s^{2}. The plasma completes 0.5-2 full rotations in the experimental time frame (∼150 ns).

Texto completo: 1 Colección: 01-internacional Banco de datos: MEDLINE Idioma: En Revista: Phys Rev Lett Año: 2023 Tipo del documento: Article País de afiliación: Reino Unido

Texto completo: 1 Colección: 01-internacional Banco de datos: MEDLINE Idioma: En Revista: Phys Rev Lett Año: 2023 Tipo del documento: Article País de afiliación: Reino Unido