METHODOLOGY
Because the historical record of earthquakes in this region is
so brief and many faults have neither ruptured in this historic
period nor are paleoseismic data available, for most fault zones
we had to rely on set of empirical relationships between fundamental
earthquake parameters which are described below. Throughout the
text we will refer to a so-called standard methodology which
presupposes a characteristic earthquake model for a given fault
or segment of a fault [Schwartz and Coppersmith, 1984] and
applies the procedures and assumptions as described below.
The length of a potential earthquake source is an
important parameter for estimating the potential size of an earthquake.
Historical data on actual rupture length are most preferred, followed
by paleoseismic evidence. Most faults have neither, so current practice
relies strongly on a combination of analogy to similar faults or
by judgment based on available data of diverse character: e.g.,
major bends or discontinuities in surface trace or microseismicity
alignment are commonly chosen as segment boundaries. In northeastern
California proximity to active volcanic centers offers distinct
constraints on segment lengths. Tentative segmentation models adopted
here are only intended for hazard modeling purposes. The endpoints
should be treated as approximate in the seismic hazard analysis.
Future paleoseismologic investigation is still required in all cases
to test our currently preferred model. For fault location we primarily
used a digital version of Jennings [1992] state fault map,
but amended this map where greater accuracy was required (e.g.,
San Andreas, Hayward, Northern Calaveras, Concord and Green Valley
faults) or where mapping was incomplete for our purposes (e.g.,
blind thrust faults of the Great Valley).
Generally we assumed 12 km as a typical value of rupture
depth in Northern California used to calculate down-dip width. David
Oppenheimer and Ivan Wong reviewed the database and suggested revisions
based on USGS Calnet catalog and special investigations. Dip values
were taken from a variety of sources, both geologic and seismologic.
When reliable historical values of magnitude were
available, then they were used. Otherwise, we mostly relied on the
empirical relation of moment magnitude to rupture area (a=lw) of
Wells and Coppersmith [1994](W&C94):
Mw = 4.07 + 0.98 log a (km2)
The equation using area was used in preference to the length equation
because it is statistically more robust according to Wells and Coppersmith.
Another important reason to avoid the length equation is that a
great many of the events used to develop the equation have greater
rupture width than applies to northern California, thus these wider
ruptures have larger seismic moment than events of equal rupture
length in California. Figure
1 and Table 1
illustrate that historic earthquakes in northern California generally
agree better with the W&C94 area relation than with their length
relation. Exceptions will be discussed by individual fault zone.
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| Figure 1. Comparison of historically observed
moment magnitudes in northern California with the empirical
rupture area and length relations of Wells and Coppersmith [1994]
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We used reliable historical or paleoseismological
values of coseismic slip where available, otherwise, we derived
slip from magnitude generally using the relation of moment magnitude
to moment of Hanks and Kanamori [1979]:
Mw = (2/3)logMo (dyne-cm) _
10.7
Using the definition of seismic moment (Mo) and rigidity
(µ = 3*1011 dyne/cm2) gives average coseismic
slip:
d = Mo/( µa)
Only minimum values of geologic or long-term
slip rates are available for some larger faults in the region, because
they may not represent the entire breadth of the fault zone. Local
and regional geodetic strain rates and regional plate tectonic models
have been used to check and constrain geologic rates where needed.
Slip rate is often the most important indicator of a fault for earthquake
potential, because it is strongly related to recurrence time. For
this reason the database gives a range of slip rate that may be
valid as an important measure of reliability of the model.
Recurrence Time (t)
When reliable historical and paleoseismic values of
average recurrence time (t) for events were available, then they
were used. Otherwise, we continue to make use of the empirical relationships
above and the following equation:
t = d/r
where d is average coseismic slip (as above) and r is slip rate
(as above). When considerable aseismic slip or creep occurs on a
particular fault, then both the values of average slip and long-term
slip rate must reflect the fault behavior in the seismogenic zone
at depth. Coseismic surface slip can be much smaller than deep coseismic
slip on creeping faults [Oppenheimer and others, 1990; Lienkaemper
and others, 1991; Lienkaemper and Prescott, 1989]. Recurrence
is a critical parameter for the probabilistic aspect of the hazard
map. Sources with recurrence times of >20,000 yr will have little
impact on the final maps.
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