timprove MCMC description - cosmo - front and backend for Markov-Chain Monte Carlo inversion of cosmogenic nuclide concentrations
 (HTM) git clone git://src.adamsgaard.dk/cosmo
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 (DIR) commit 34d863dbc2986f2eff0ac8ff390333c91e8fa532
 (DIR) parent 6bbc2f1eca168add56b0057cd8692abdd08448bb
 (HTM) Author: Anders Damsgaard <anders.damsgaard@geo.au.dk>
       Date:   Fri, 27 Nov 2015 16:07:08 +0100
       
       improve MCMC description
       
       Diffstat:
         M pages/methods.html                  |      53 ++++++++++++++++++++++++++-----
       
       1 file changed, 45 insertions(+), 8 deletions(-)
       ---
 (DIR) diff --git a/pages/methods.html b/pages/methods.html
       t@@ -65,7 +65,28 @@
                            (&delta;<sup>18</sup>O<sub>threshold</sub>) is specified
                            with uniform probability across the linear
                            parameter interval. The user specifies the bounds
       -                    of the model parameters, which define the model space.
       +                    of the model parameters.
       +                    </p>
       +
       +                    <p>Given a single value of model parameters
       +                    (&epsilon;<sub>int</sub>, &epsilon;<sub>gla</sub>,
       +                    <i>t</i><sub>degla</sub>,
       +                    &delta;<sup>18</sup>O<sub>threshold</sub>), the TCN
       +                    concentration after the duration of e.g. the entire
       +                    Quaternary period in a sample can be computed. This
       +                    <i>forward model</i> describes a history of exhumation and
       +                    TCN production in a sample volume as it experiences the
       +                    variable physical environment of the Pleistocene.
       +                    </p>
       +
       +                    <p>When model parameters 
       +                    (&epsilon;<sub>int</sub>, &epsilon;<sub>gla</sub>,
       +                    <i>t</i><sub>degla</sub>,
       +                    &delta;<sup>18</sup>O<sub>threshold</sub>) are allowed to
       +                    vary within specified limits, they can be thought of as
       +                    orthogonal axes creating a coordinate system in higher-order
       +                    space. Every position in this model space is associated with
       +                    a certain set of model parameter values.
                            </p>
                        </div>
        
       t@@ -73,13 +94,29 @@
                            <h4 class="header blue-text light">
                                What is a MCMC walker?</h4>
                            <p>
       -                    forward responses are computed based on an initial set of
       -                    model parameters that is proposed using the
       -                    Metropolis-Hastings technique. A burn-in phase of 1000
       -                    iterations is first used to make a crude initial search of
       -                    the model space. This step is followed by a more detailed
       -                    and local search of the model space based on the best-fit
       -                    model parameters from the burn-in phase.
       +                    A MCMC walker is a numerical entity which sequentially
       +                    explores the model parameter space in order to obtain the
       +                    best result between a forward-model and an observational
       +                    dataset. During each iteration
       +                    the walker takes its current position in model space, plugs
       +                    the parameter value into the forward-model, and
       +                    evaluates if the output result matches the observational
       +                    record better or worse than the output at its previous
       +                    position in model space. If the new results better matches
       +                    the observed dataset, it continues walking along the same
       +                    path in model space with a small random perturbation.
       +                    </p>
       +
       +                    <p>
       +                    Starting at a random place inside the model space, a burn-in
       +                    phase of 1000 iterations is first used to make a crude
       +                    search of the entire model space.  
       +                    The burn-in phase is followed by a similar but more detailed
       +                    and local search of the model space, based on the best-fit
       +                    model parameters from the burn-in phase.  The weighted
       +                    least-squared misfit to observed TCN concentrations is used
       +                    to evaluate the likelyhood for the combinations of
       +                    model parameter values.
                            </p>
                        </div>