We give a short account of the most prominent structures of the interm
ediate corona. Then we propose an axially symmetrical model for corona
l streamers, according to which charged particles move along magnetic
surfaces whose sources are electrical currents situated in the vicinit
y of the photosphere. The simplest current configuration is a pair of
coaxial, coplanar, circular, and oppositely directed currents parallel
to the photosphere. Magnetic surfaces for this current distribution e
xhibit a helmet-shaped separatrix and a saddle point. The temperature
profile along the streamer can be predicted qualitatively if one takes
into account the conservation of an adiabatic invariant in the drift
theory of the charged particle motion.