Prominence Formation
Prominences are manifestations of cold plasma suspended in the hot corona. The
plasma is supported against the gravitational pool by the magnetic field. One of
the open questions are how they are formed. Observations suggest that the
convergence of flux elements across the filament channel may provide a tricker
for the formation process. We (
Aaron Longbottom) have investigated a simple dynamical model of this
scenario. A simple quadro polar field line structure is chosen as the initial
condition and the flux patterns are followed moved towards each other. This
eventually forces magnetic reconnection to take place between the field of the
two nearest sources. The reconnection takes place above the driving photosphere
and lifts material into the upper atmosphere where it spreads along the polarity
inversion line. The experiments indicate that mass have to be continuously
supplied to the prominence structure to maintain a high density contrasts to the
ambient plasma. As the lift in the experiment occurs near adiabatic, it is
found that the lifted plasma cools as it is lifted and adjusts to the pressure
at the higher height.
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Last updated 12.06.00