TY - JOUR
T1 - Power-law velocity distributions in fracture networks
T2 - Numerical evidence and implications for tracer transport
AU - Painter, Scott
AU - Cvetkovic, Vladimir
AU - Selroos, Jan Olof
N1 - Publisher Copyright:
© Copyright 2002 by the American Geophysical Union.
PY - 2002/7/15
Y1 - 2002/7/15
N2 - Velocity distributions in two- and three-dimensional networks of discrete fractures are studied through numerical simulations. The distribution of 1/v, where v is the velocity along particle trajectories, is closely approximated by a power law (Pareto) distribution over a wide range of velocities. For the conditions studied, the power law exponents are in the range 1.1-1.8, and generally increase with increasing fracture density. The same is true for the quantity 1/bv, which is related to retention properties of the rock; b is the fracture half-aperture. Using a stochastic Lagrangian methodology and statistical limit theorems applicable to power-law variables, it is shown that the distributions of residence times for conservative and reacting tracers are related to one-sided stable distributions. These results are incompatible with the classical advection dispersion equation and underscore the need for alternative modeling approaches.
AB - Velocity distributions in two- and three-dimensional networks of discrete fractures are studied through numerical simulations. The distribution of 1/v, where v is the velocity along particle trajectories, is closely approximated by a power law (Pareto) distribution over a wide range of velocities. For the conditions studied, the power law exponents are in the range 1.1-1.8, and generally increase with increasing fracture density. The same is true for the quantity 1/bv, which is related to retention properties of the rock; b is the fracture half-aperture. Using a stochastic Lagrangian methodology and statistical limit theorems applicable to power-law variables, it is shown that the distributions of residence times for conservative and reacting tracers are related to one-sided stable distributions. These results are incompatible with the classical advection dispersion equation and underscore the need for alternative modeling approaches.
UR - https://www.scopus.com/pages/publications/0346037238
U2 - 10.1029/2002GL014960
DO - 10.1029/2002GL014960
M3 - Article
AN - SCOPUS:0346037238
SN - 0094-8276
VL - 29
JO - Geophysical Research Letters
JF - Geophysical Research Letters
IS - 14
M1 - 1676
ER -