Seismic Deformation
When an earthquake fault ruptures, it causes two types of deformation:
static;
and dynamic. Static deformation is the permanent displacement
of
the ground due to the event. The earthquake cycle progresses
from
a fault that is not under stress, to a stressed fault as the plate
tectonic
motions driving the fault slowly proceed, to rupture during an
earthquake
and a newly-relaxed but deformed state.
Typically, someone will build a straight reference line such as a road,
railroad, pole line, or fence line across the fault while it is in the
pre-rupture stressed state. After the earthquake, the formerly straight
line is distorted into a shape having increasing displacement near the
fault, a process known as
elastic rebound.
Seismic Waves
The second type of deformation, dynamic motions, are essentially sound
waves radiated from the earthquake as it ruptures. While most of the
plate tectonic
energy driving fault ruptures is taken up by static deformation, up to
10% may dissipate immediately in the form of seismic waves.
The mechanical properties of the
rocks that seismic waves travel through
quickly organize the waves into two types. Compressional waves, also
known
as primary or P waves, travel fastest, at speeds between 1.5 and 8
kilometers
per second in the Earth's crust. Shear waves, also known as secondary
or
S waves, travel more slowly, usually at 60% to 70% of the speed of P
waves.
P waves shake the ground in the direction they are propagating,
while
S waves shake perpendicularly or transverse to the direction of
propagation.
Although wave speeds vary by a factor of ten or more in the Earth,
the
ratio between the average speeds of a P wave and of its following S
wave
is quite constant. This fact enables seismologists to simply time the
delay
between the arrival of the P wave and the arrival of the S wave to get
a quick and reasonably accurate estimate of the distance of the
earthquake
from the observation station. Just multiply the S-minus-P (S-P) time,
in
seconds, by the factor 8 km/s to get the approximate distance in
kilometers.
The dynamic, transient seismic waves from any substantial earthquake
will propagate all around and entirely through the Earth. Given a
sensitive
enough detector, it is possible to record the seismic waves from even
minor
events occurring anywhere in the world at any other location on the
globe.
Nuclear test-ban treaties in effect today rely on our ability to detect
a nuclear explosion anywhere equivalent to an earthquake as small as
Richter
Magnitude 3.5.
Seismographs and Seismograms
Sensitive seismographs are the principal tool of scientists who
study earthquakes. Thousands of seismograph stations are in operation
throughout
the world, and instruments have been transported to the Moon, Mars, and
Venus. Fundamentally, a seismograph is a simple pendulum. When the
ground
shakes, the base and frame of the instrument move with it, but intertia
keeps the pendulum bob in place. It will then appear to move, relative
to the shaking ground. As it moves it records the pendulum
displacements
as they change with time, tracing out a record called a
seismogram.
One seismograph station, having three different pendulums sensitive
to the north-south, east-west, and vertical motions of the ground, will
record seismograms that allow scientists to estimate the distance,
direction,
Richter
Magnitude, and type of faulting of the earthquake. Seismologists
use
networks
of seismograph stations to determine the location of an earthquake, and
better estimate its other parameters. It is often revealing to examine
seismograms recorded at a range of distances from an earthquake:
On this example it is obvious that seismic waves take more time to
arrive at stations that are farther away. The average velocity of the
wave
is just the slope of the line connecting arrivals, or the change in
distance
divided by the change in time. Variations in such slopes reveal
variations
in the seismic velocities of rocks. Note the secondary S-wave arrivals
that have larger amplitudes than the first P waves, and connect at a
smaller
slope.
Locating Earthquakes
The principle use of seismograph networks is to locate
earthquakes.
Although it is possible to infer a general location for an event from
the
records of a single station, it is most accurate to use three or more
stations.
Locating the source of any earthquake is important, of course, in
assessing
the damage that the event may have caused, and in relating the
earthquake
to its geologic setting.
Given a single seismic station,
the seismogram records will yield a measurement
of the S-P time, and thus the distance between the station and the
event.
Multiply the seconds of S-P time by 8 km/s for the kilometers of
distance.
Drawing a circle on a map around the station's location, with a radius
equal to the distance, shows all possible locations for the event. With
the S-P time from a second station, the circle around that station will
narrow the possible locations down to two points. It is only with a
third
station's S-P time that you can draw a third circle that should
identify
which of the two previous possible points is the real one:
This example uses stations in Boston, Edinburgh, and Manaus. With
the distances shown, all three circles can intersect only at a single
point
on the Mid-Atlantic Ridge spreading center.