Evolution of magnetic helicity under kinetic magnetic reconnection: Part II B != 0 reconnection

T. Wiegelmann (1, 2) , J. Büchner (2)

1 School of Mathematics and Statistics [St Andrews]
2 MPI Aeronomie - Max-Planck-Institut für Aeronomie

We investigate the evolution of magnetic helicity under kinetic magnetic reconnection in thin current sheets. We use Harris sheet equilibria and superimpose an external magnetic guide field. Consequently, the classical 2D magnetic neutral line becomes a field line here, causing a B != 0 reconnection. While without a guide field, the Hall effect leads to a quadrupolar structure in the perpendicular magnetic field and the helicity density, this effect vanishes in the B != 0 reconnection. The reason is that electrons are magnetized in the guide field and the Hall current does not occur. While a B = 0 reconnection leads just to a bending of the field lines in the reconnection area, thus conserving the helicity, the initial helicity is reduced for a B != 0 reconnection. The helicity reduction is, however, slower than the magnetic field dissipation. The simulations have been carried out by the numerical integration of the Vlasov-equation.

Domaines: Cosmologie et astrophysique extra-galactique [astro-ph.CO]; Astrophysique [astro-ph]; Sciences de la Terre

T. Wiegelmann, J. Büchner. Evolution of magnetic helicity under kinetic magnetic reconnection: Part II B != 0 reconnection. Nonlinear Processes in Geophysics, 2002, 9 (2), pp.139-147. ⟨hal-00303034⟩