fitactf

Fits the ACTF to the estimated (rho_x, rho_z) points using <code>nls</code>.

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

fitactf function

<dl><dt>actpnts</dt>
<dd>estimated ACT points (output of <code>actpnts</code>)</dd>
<dt>discrete</dt>
<dd>logical — is the marginal distribution discrete?</dd></dl>

Arguments

Fit the AutoCorrelation Transformation Function — fitactf

<dl>

<dt>actpnts</dt>
<dd>estimated ACT points (output of <code>actpnts</code>)</dd>


<dt>discrete</dt>
<dd>logical — is the marginal distribution discrete?</dd>

</dl>

fitactf: Fit the AutoCorrelation Transformation Function

Description

Usage

Value

Arguments

See Also

Examples