Dh. Mackay et al., FORCE-FREE AND POTENTIAL MODELS OF A FILAMENT CHANNEL IN WHICH A FILAMENT FORMS, The Astrophysical journal, 486(1), 1997, pp. 534-549
Few examples of the creation of a filament channel or filament have ev
er been documented. In a recent paper, Gaizauskas and coworkers observ
ed the early stages of creation of such a channel and then the formati
on of a filament in it. The filament channel was born when a new activ
ity complex emerged near an old, decaying bipolar active region. The f
ilament itself then formed after convergence of flux in the channel. I
n this paper, force-free models are constructed for two phases of the
channel's development. For the early days, the models show that the fo
rmation of the filament channel seen in Ha is due to the emerging acti
vity complex. The field lines that give the best comparison to the fib
ril observations are low-lying and have a strong horizontal component.
Later, when the activity complex has matured and a filament has forme
d between it and the adjacent decaying bipolar region, the models give
a good representation of the path of the filament in the channel. It
is found that the presence of flat or dipped field lines and of conver
ging flux are necessary but not sufficient conditions for filament for
mation. Furthermore, the magnetic field lines of the filament itself f
orm a narrow, vertical, sheetlike flux-tube corridor that is hat and l
ow-lying. It connects one particular magnetic source to a sink and is
bounded by separatrix surfaces that separate the filament from the old
remnant region and most of the newly emerged flux.