• DocumentCode
    2440293
  • Title

    Perpendicular diffusion coefficients and Newton-Lorentz equation

  • Author

    Dosch, Alexander ; Shalchi, Andreas

  • Author_Institution
    Lehrstuhl IV: Weltraum- und Astrophys., Ruhr-Univ. Bochum, Bochum
  • fYear
    2008
  • fDate
    15-19 June 2008
  • Firstpage
    1
  • Lastpage
    1
  • Abstract
    In this paper the perpendicular transport of charged particles (cosmic rays) in a magnetized plasma is discussed. A superposition of a mean magnetic field (e.g. the magnetic field of the sun) and a turbulent component is assumed. It is also presented here how diffusion coefficients can be obtained directly from the Newton-Lorentz equation.
  • Keywords
    cosmic rays; diffusion; plasma transport processes; plasma turbulence; Newton-Lorentz equation; charged particles; cosmic rays; magnetized plasma; mean magnetic field; perpendicular diffusion coefficients; perpendicular transport; turbulent component; Cosmic rays; Differential equations; Magnetic analysis; Magnetic fields; Particle scattering; Plasma transport processes; Scattering parameters; Sun;
  • fLanguage
    English
  • Publisher
    ieee
  • Conference_Titel
    Plasma Science, 2008. ICOPS 2008. IEEE 35th International Conference on
  • Conference_Location
    Karlsruhe
  • ISSN
    0730-9244
  • Print_ISBN
    978-1-4244-1929-6
  • Electronic_ISBN
    0730-9244
  • Type

    conf

  • DOI
    10.1109/PLASMA.2008.4590943
  • Filename
    4590943
    • Link To Document
    https://search.isc.ac/dl/search/defaultta.aspx?DTC=49&DC=2440293