Formation of active region and quiescent prominence magnetic field configurations.

Details Formation of active region and quiescent prominence magnetic field configurations. Formation of active region and quiescent prominence magnetic field configurations.

Dec 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986nascp2442...51a&link_type=abstract

NASA Conf. Publ., NASA CP-2442, p. 51 - 56

Physics

Magnetohydrodynamics:Solar Prominences, Solar Prominences:Formation, Solar Prominences:Magnetohydrodynamics, Solar Prominences:Numerical Simulations

Scientific paper

To investigate the formation of prominences, the authors have studied chromospheric mass injection into an overlying coronal dipole magnetic field using a 2-D ideal magnetohydrodynamic (MHD) numerical model. They try to find optimum conditions for the formation of Kippenhahn-Schuluter (K-S) type field configuration for stable support of the injected plasmas. They find that the formation of K-S type field configuration by mass injection requires a delicate balance between injection velocity, density, and overlying magnetic fields. This results may explain why a prominence does not form on every neutral line.

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