• Plasma heating in a sheared magnetic field

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    • Keywords


      Alfven waves; plasma heating; solar corona

    • Abstract


      The mechanism of spatial resonance of Alfven waves for heating a collisionless plasma is studied in the presence of a twisted magnetic field. In addition to modifying the equilibrium condition for a cylindrical plasma, the azimuthal component of the magnetic field gives extra contribution to the energy deposition rate of the Alfven waves. This new term clearly brings out the effects associated with the finite lifetime of the Alfven waves. The theoretical system considered here conforms to the solar coronal regions.

    • Author Affiliations


      V. Krishan1

      1. Indian Institute of Astrophysics, Bangalore - 560034
    • Dates

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