G. Aulanier et P. Demoulin, 3-D MAGNETIC CONFIGURATIONS SUPPORTING PROMINENCES - I - THE NATURAL PRESENCE OF LATERAL FEET, Astronomy and astrophysics, 329(3), 1998, pp. 1125-1137
It is now commonly accepted that prominence plasma is supported in mag
netic dips, in particular in twisted flux-tubes. But present two-dimen
sional models are unable to explain the observed presence and structur
e of prominences feet. This requires three-dimensional models. We mode
led the field using linear force-free field equations. Combining a sma
ll number of harmonics, and using observational constraints, we have f
ound the area in the parameter space where prominences are likely to b
e present. Then, adding 3-D harmonics, we show that feet appear period
ically underneath the prominence body. For great helicity, the paramet
er space is mostly fulfilled by configurations which have feet alterna
ting between both sides of the prominence axis, as observed. The theor
etical photospheric field has a quasi-bipolar pattern and the prominen
ce stands above a magnetic corridor containing only small parasitic po
larities. The lateral feet are formed by dips in the vicinity of these
small polarities. These configurations show in a natural fashion a nu
mber of well-established as well as more recent observationnal aspects
of prominences, in particular the vector magnetic field measurements
in prominences and the chirality patterns (the dextral/sinistral, righ
t/left bearing, skew of the overlying coronal arcade and fibril organi
zation in prominence channels).