Magnetic Reconnection in Partially Ionized Gas: Application to the FIP Effect in the Solar Corona

D. J. Mullan and C. N. Arge

Bartol Research Institute, University of Delaware, Newark DE 19716

When reconnection occurs in partially ionized gas, only the ions respond directly to the magnetic field: these ions attempt to collapse towards the null line, so as to emerge as jets from the site according to the standard picture of reconnection. Atoms participate in the reconnection flow to the extent that they are collisionally coupled to the ions. We have adapted the ZEUS code to model this process in a two-step cycle: in the first step, we apply the hydrodynamic version of the ZEUS code to the neutral fluid, and in the second step, we apply the MHD version of ZEUS to the charged fluid. In the process of cycling back and forth between the two fluids, momentum and energy exchange terms between the species are included as source terms. In the emerging jets, we find that ion/atom number ratios are enhanced over the ambient values by amounts which depend on the degree of ionization and the plasma beta parameter. We suggest that the enhancements in ion/atom ratios give rise to the FIP effect in the corona. Because the reconnection occurs in the solar chromosphere, the ion/atom enhancements are subject to regulation.