Mercurial > hg > ltpda
diff m-toolbox/html_help/help/ug/noisegen_content.html @ 0:f0afece42f48
Import.
author | Daniele Nicolodi <nicolodi@science.unitn.it> |
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date | Wed, 23 Nov 2011 19:22:13 +0100 |
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--- /dev/null Thu Jan 01 00:00:00 1970 +0000 +++ b/m-toolbox/html_help/help/ug/noisegen_content.html Wed Nov 23 19:22:13 2011 +0100 @@ -0,0 +1,26 @@ +<p> + +Generating non-white random noise means producing arbitrary long time series with a given spectral density. +Such time series are needed for example for the following purposes: +</p> +<p> + <ul> + <li> To generate test data sets for programs that compute spectral densities, </li> + <li> as inputs for various simulations.</li> + </ul> +</p> +<p> + One way of doing this is to apply digital filters (FIR or IIR) to white input noise.<br/> + This approach is effectively implemented for the generation of <a href="ndim_ng.html"> multichannel noise </a> + with a given cross spectral density. <br/> + Multichannel transfer functions are identified by an automatic fit procedure based + on a modified version of the vector-fitting algorithm + (see <a href="zdomainfit.html"> Z-Domain Fit </a> for further details on the algorithm). <br/> + Partial fraction expansion of multichannel transfer functions and the implementation of + <a href="sigproc_dfilt.html">filter</a> state initialization avoid the presence of unwanted 'warm-up period'. +</p> + +<p> + A different approach is implemented in LTPDA as <a href="franklin_ng.html">Franklin noise-generator</a>.<br/> + It produces spectral densities according to a given pole zero model (see <a href="pzmodel.html">Pole/Zero Modeling</a>) and does not require any warm-up period. <br/> +</p>