anisotropyT2

Provides parametric functions that describe different types of planar deformation fields, including affine (rotation and stretching), and swirl-like deformation. For more details see Papalexiou et al.(2021) and references therein.

internal

Makes univariate, multivariate, or random fields simulations precise and simple. Just select the desired time series or random fields’ properties and it will do the rest. CoSMoS is based on the framework described in Papalexiou (2018, <doi:10.1016/j.advwatres.2018.02.013>), extended for random fields in Papalexiou and Serinaldi (2020, <doi:10.1029/2019WR026331>), and further advanced in Papalexiou et al. (2021, <doi:10.1029/2020WR029466>) to allow fine-scale space-time simulation of storms (or even cyclone-mimicking fields).

Kevin Shook

CoSMoS

Complete Stochastic Modelling Solution

Simon Michael Papalexiou

Francesco Serinaldi

Filip Strnad

Yannis Markonis

anisotropyT2 function

<dl><dt>id</dt>
<dd>anisotropy type id</dd>
<dt>arglist</dt>
<dd>list of additional arguments (vector of coordinates and parameters of the anisotropy transformations)</dd></dl>

Arguments

Anisotropy transformation — anisotropyT2

<dl>

<dt>id</dt>
<dd>anisotropy type id</dd>


<dt>arglist</dt>
<dd>list of additional arguments (vector of coordinates and parameters of the anisotropy transformations)</dd>

</dl>

anisotropyT2: Anisotropy transformation

Description

Usage

Arguments

References