The inner core has the intriguing property that seismic waves travelin
g parallel to the Earth's spin axis arrive earlier than those travelin
g parallel to the equatorial plane. The travel time is some 6 s faster
from pole to pole than across the equator. This difference is not the
result of different polar and equatorial radii of the inner core, for
it would require the inner core to be elongated at the poles by more
than one third of its radius. Rather, this 6-s travel time difference
is the result of the inner core's being anisotropic; wave speeds diffe
r for different directions of wave propagation. This anisotropy, disco
vered only in the last decade, is characterized by cylindrical symmetr
y about an axis approximately aligned with the Earth's spin axis. The
anisotropy is believed to be due to a preferred orientation of anisotr
opic iron crystals composing the inner core, but the mechanisms respon
sible for creating such a preferred orientation remain uncertain. With
the anisotropy now well established as a basic property of the inner
core, its quantification and that temporal variations of its orientati
on have become a vital tool for probing the structure, composition, an
d dynamics of the Earth's deep interior.