Images of sprites have been recorded at 1 ms resolution revealing several n
ew sprite properties. Sprites appear to occur in a highly structured mesosp
here, and we suggest that the cause of some of this structure is the sprite
activity itself. Evidence is seen in events where a subsequent nearby spri
te appears to re-activate the volume of a previous sprite, in sprites where
tendrils and branches develop away from the normally observed vertical dir
ection, and in beads that lasts much longer that the parent sprite. Sprites
can be large with horizontal widths of more than 40 km and can extend from
the clouds up to the lower ionosphere thus affecting a large volume of the
atmosphere, The total horizontal area of sprites during one storm over Neb
raska was a significant fraction of the area covered by the associated thun
derstorm raising the possibility of larger scale measurable mesospheric eff
ects.