tadd mcmc methods - cosmo - front and backend for Markov-Chain Monte Carlo inversion of cosmogenic nuclide concentrations
 (HTM) git clone git://src.adamsgaard.dk/cosmo
 (DIR) Log
 (DIR) Files
 (DIR) Refs
 (DIR) README
 (DIR) LICENSE
       ---
 (DIR) commit 4769723624cf47e9a1c827ebe1388971f8616e2c
 (DIR) parent c61d24deab6ce81dcb4e8b538cab571d035beb2e
 (HTM) Author: Anders Damsgaard <anders.damsgaard@geo.au.dk>
       Date:   Fri, 27 Nov 2015 15:34:25 +0100
       
       add mcmc methods
       
       Diffstat:
         M pages/methods.html                  |      26 ++++++++++++++++++++++++--
       
       1 file changed, 24 insertions(+), 2 deletions(-)
       ---
 (DIR) diff --git a/pages/methods.html b/pages/methods.html
       t@@ -52,13 +52,35 @@
                        <div id="mcmc" class="section scrollspy">
                            <h3 class="header blue-text">
                                Markov-Chain Monte Carlo (MCMC) basics</h3>
       -                    <p>bla bla</p>
       +                    <p>The inversion problem of turning observed TCN
       +                    concentrations into erosion histories is handled using a
       +                    conventional Metropolis-Hastings MCMC approach where the
       +                    model parameters are constrained between fixed model
       +                    parameter bounds specified by the user. Erosion rates
       +                    (&epsilon;<sub>int</sub>, &epsilon;<sub>gla</sub>), which
       +                    may vary over several orders of magnitude, are specified
       +                    with uniform probability across the logarithmic parameter
       +                    interval. The temporal parameter (<i>t</i><sub>degla</sub>)
       +                    and climate record threshold value
       +                    (&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.
       +                    </p>
                        </div>
        
                        <div id="mcmcwalker" class="subsection scrollspy">
                            <h4 class="header blue-text light">
                                What is a MCMC walker?</h4>
       -                    <p>bla bla</p>
       +                    <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.
       +                    </p>
                        </div>
        
                        <div id="twostage" class="section scrollspy">