Akebono (Exos D) observations demonstrate that polar cap arcs sometime
s have a fine structure, that is, multiple (double or triple) arcs wit
h spacing of a few lens of kilometers. The multiple polar cap arcs are
dominantly observed in the nightside polar cap region, suggesting tha
t low background conductance favors the appearance of the structured a
rcs. A relationship between the spacing and the average energy of the
precipitating electrons is investigated. Results show that a higher en
ergy leads to a wider spacing. Akebono observations also show the exis
tence of a downward current region embedded between upward current reg
ions (arcs). Comparison of the observations with results from a couple
d magnetosphere-ionosphere Sun-aligned are model is made, which shows
good qualitative agreement between the modeling and observational resu
lts on the spacing-energy dependence and the effect of background iono
spheric conductance.