High-resolution optical observations by the University of Calgary Port
able Auroral Imager show a frequent occurrence of asymmetric multiple
small-scale auroral are structures during auroral substorms. Whereas t
he classical multiple are array tends to exhibit a fairly symmetrical
configuration, with parallel motions within individual discrete arcs b
eing opposite in direction across the center of the are array, the mul
tiple arcs to be discussed herein are distinguished by the presence of
discrete arcs strictly equatorward of the two bright counter-streamin
g arcs that would ordinarily define the center of the are array. The i
ntensity of these parallel equatorward-lying arcs were in most cases f
ound to decrease rapidly in the equatorward direction. By considering
the topology of the structures and the spacing between arcs, observati
ons are found to be consistent with recent theories suggesting inertia
l Alfven waves as a possible cause of fine-scale auroral arcs.