2010
DOI: 10.1007/s10687-010-0119-1
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A class of non-Gaussian second order random fields

Abstract: Non-Gaussian stochastic fields are introduced by means of integrals with respect to independently scattered stochastic measures distributed according to generalized Laplace laws. In particular, we discuss stationary second order random fields that, as opposed to their Gaussian counterpart, have a possibility of accounting for asymmetry and heavier tails. Additionally to this greater flexibility the models discussed continue to share most spectral properties with Gaussian processes. Their statistical distributi… Show more

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Cited by 30 publications
(49 citation statements)
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“…The model coincides with the one that in the discretized version was given by (1). Dynamics is expressed by an arbitrary time varying velocity field that generates a flow given by ψ t,h (p) which is the location at time t + h of a point that at time t is at p. Such a flow is incorporated into a stochastic framework by means of the stochastic integral…”
Section: 3mentioning
confidence: 99%
See 1 more Smart Citation
“…The model coincides with the one that in the discretized version was given by (1). Dynamics is expressed by an arbitrary time varying velocity field that generates a flow given by ψ t,h (p) which is the location at time t + h of a point that at time t is at p. Such a flow is incorporated into a stochastic framework by means of the stochastic integral…”
Section: 3mentioning
confidence: 99%
“…The generality of the approach allows a natural extension for second order models that goes beyond Gaussian distribution but this is not explored here. Steps in this direction have been undertaken for the fields driven by Laplace motion in [1] and will be continued in future research.…”
Section: 3mentioning
confidence: 99%
“…The Laplace moving average field was introduced inÅberg and Podgórski (2011). It can be also constructed using Eq.…”
Section: Laplace Moving Average Model (Lma) X Lmamentioning
confidence: 99%
“…The significance of AL distributions, denoted by AL d ( , µ), is partially due to fact that these arise rather naturally as the only distributional limits for (appropriately normalized) random sums X (1) + · · · + X (N p )…”
Section: Introductionmentioning
confidence: 99%