Article ID Journal Published Year Pages File Type
10121234 Physics of the Earth and Planetary Interiors 2005 6 Pages PDF
Abstract
The observed temporal series of the shocks per day can be considered as a sum of a deterministic contribution (the aftershock decay power law, n(t) = K·(t + c)−p + K1) and of a stochastic contribution (the random fluctuations around a mean value represented by the above mentioned power law). If the decay can be modeled as a non-stationary Poissonian process where the intensity function is equal to n(t) = K·(t + c)−p + K1, the number of aftershocks in a small time interval Δt is the mean value n(t)·Δt, with a standard deviation σ=n(t)⋅Δt.
Related Topics
Physical Sciences and Engineering Earth and Planetary Sciences Geophysics
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