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  1. cambridge.org

    The current filamentation instability (CFI) is capable of generating strong magnetic fields relevant to the explanation of radiation processes in astrophysical objects and leads to the onset of particle acceleration in collisionless shocks.
  2. Abstract: Current Filamentation Instability (CFI) is capable of generating strong magnetic fields relevant to explain radiation processes in astrophysical objects and lead to the onset of particle acceleration in collisionless shocks. Probing such extreme scenarios in the laboratory is still an open challenge.
  3. researchgate.net

    Conditions for the onset of the current filamentation instability in the lab oratory 3 with competing instabilities, can b e suppressed as lo ng as the ratio b etween the beam density and the ...
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  5. ui.adsabs.harvard.edu

    The current filamentation instability (CFI) is capable of generating strong magnetic fields relevant to the explanation of radiation processes in astrophysical objects and leads to the onset of particle acceleration in collisionless shocks. Probing such extreme scenarios in the laboratory is still an open challenge. In this work, we investigate the possibility of using neutral e<SUP>-</SUP>e ...
  6. epp.tecnico.ulisboa.pt

    extreme plasma physics > Publications > Conditions for the onset of the current filamentation instability in the laboratory. Conditions for the onset of the current filamentation instability in the laboratory. Latest News / Press Releases. PhD position(s) in extreme plasma physics 2024
  7. link.aps.org

    The current filamentation instability, which generically arises in the counterstreaming of plasma flows, is known for its ability to convert the free energy associated with anisotropic momentum distributions into kinetic-scale magnetic fields. The saturation of this instability has been extensively studied in symmetric configurations where the interpenetrating plasmas share the same properties ...
  8. semanticscholar.org

    Conditions for the onset of the current filamentation instability in the laboratory. N. Shukla J. Vieira P. Muggli G. Sarri R. Fonseca Luís O. Silva. ... 2018; The current filamentation instability (CFI) is capable of generating strong magnetic fields relevant to the explanation of radiation processes in astrophysical objects and leads to the ...
  9. link.aps.org

    Current filamentation instability is observed and studied in a laboratory environment with a 60 MeV electron beam and a plasma capillary discharge. Multiple filaments are observed and imaged transversely at the plasma exit with optical transition radiation. By varying the plasma density the transition between single and multiple filaments is found to be ${k}_{p}{\\ensuremath{\\sigma}}_{r ...
  10. accelconf.web.cern.ch

    Current Filamentation Instability, CFI, is a basic beam-plasma instability that has a purely imaginary frequency and is purely transverse electromagnetic. It occurs due to non-uniformities in the transverse beam and plasma profiles, which lead to unequal opposite beam current and plasma return current and to the generation or
  11. pubs.aip.org

    The current filamentation instability (CFI) or Weibel-type instability is studied for a nonrelativistic electron beam penetrating an infinite uniform plasma, taking into account both the collisional effects and the space-charge effect (SCE).

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