Ae. Clifton et al., Influence of rift obliquity on fault-population systematics: results of experimental clay models, J STRUC GEO, 22(10), 2000, pp. 1491-1509
We use clay models to simulate how fault population systematics vary as a f
unction of rift obliquity. Rift obliquity is related to the acute angle, al
pha, between the rift trend and the displacement direction, so that the val
ue of alpha is inverse to the degree of obliquity. The range of azimuths in
a fault population increases as rift obliquity increases (i.e. as alpha de
creases). The length of the longest faults, the sum of fault lengths, and t
he width of the deformed zone all increase as rift obliquity decreases (i.e
. as alpha increases). The majority of faults in our models are segmented a
nd have highly tortuous traces. Tortuosity is maximum when alpha = 30 degre
es as segments of widely varying azimuth link during fault growth. Signific
ant changes occur in the fault patterns between alpha = 30 degrees and alph
a = 45 degrees. At 1-30 degrees two fault populations of equal importance d
evelop in the center of the rift zone, one approximately rift-parallel and
the other displacement-normal. Between alpha = 30 degrees and 45 degrees. t
he number of faults more than doubles, and between alpha = 45 degrees and 6
0 degrees, summed fault length more than doubles. Fault patterns for all mo
dels are fractal, with fractal dimensions that increase with increasing alp
ha and that are comparable to those found in the field. Fault populations a
re not multi-fractal because the cumulative frequency distributions of faul
t lengths do not generally follow a power-law relationship. An exponential
distribution best describes the data for whole faults, with the characteris
tic length increasing with increasing alpha. Segment lengths also follow an
exponential distribution with characteristic length varying very little wi
th alpha. The fault patterns in our models resemble the spatial pattern of
brittle deformation observed at oblique mid-ocean ridge segments and are si
milar in geometry to those in oblique continental rift basins. At the rift
margins, tensional stresses are modulated and reoriented by a secondary str
ess field related to a change in boundary conditions, resulting in the form
ation of two distinct sub-populations of faults during oblique rifting. (C)
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