cosmo

Front and backend for Markov-Chain Monte Carlo inversion of cosmogenic nuclide concentrations
git clone git://src.adamsgaard.dk/cosmo
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commit 9abb8d8302f7752b7f803bacc0a0a68e3992ee00
parent a53b33ee8911d15bcfd27b48dad8944d0fd86baa
Author: Anders Damsgaard <anders.damsgaard@geo.au.dk>
Date:   Fri, 27 Nov 2015 16:48:47 +0100

change nesting and indentation

Diffstat:
Mpages/methods.html | 158++++++++++++++++++++++++++++++++++++++++---------------------------------------
1 file changed, 81 insertions(+), 77 deletions(-)

diff --git a/pages/methods.html b/pages/methods.html @@ -87,85 +87,89 @@ as it experiences the variable physical environment of the Quaternary.</p> - </div> - - <div id="twostage" class="subsection scrollspy"> - <h4 class="header blue-text light"> - Two-stage glacial-interglacial forward model</h4> - <p>The forward model builds on the assumption of a - "two-stage uniformitarianism", meaning that the processes - that operated during the Holocene also operated during - earlier interglacials with comparable intensity. Likewise, - the erosion rate during the past glacial periods is assumed - to be comparable.</p> - - <p>The model approach assumes that glacial periods were - characterized by 100% shielding and no exposure, which would - require more than 10 m of ice thickness for production due - to spallation (&gt;50 m for muons). Interglacial periods are - assumed to have been characterized by 100% exposure and zero - shielding. The production of TCNs takes place during the - interglacials, while erosion removes the land surface at - different rates during the glacials and interglacials.</p> - </div> - - <div id="mcmcwalker" class="subsection scrollspy"> - <h4 class="header blue-text light"> - What is a MCMC walker?</h4> - <p> - A MCMC walker is in this context a numerical entity which - sequentially explores the model parameter space in order to - obtain the closest match between the forward model and the - observational dataset of TCNs. 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 in the same - direction in model space. - </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. - The MCMC walker continues exploring the model space until it - is sufficiently satisfied with the best model parameter - estimate it has found. - </p> - - <p> - For a given observational data set more than one set of - model parameters may produce forward models which - sufficiently satisfy the MCMC walker. - In this case the solution is <i>non-unique</i>. Even worse, - a single MCMC walker may find an area in model space which - seemingly is in good correspondence with the observational - data set, but the walker is missing a much better set of - model parameters since they are located somewhere entirely - different in the model space. In order to mitigate these - issues, MCMC inversions are often performed using several - MCMC walkers. The starting point of each MCMC walker is - chosen at random, resulting in unique walks through the - model space. If a single walker is caught in an area of - non-ideal solutions, chances are that the other walkers will - find the area of better model parameters. - </p> + <div id="twostage" class="subsection scrollspy"> + <h4 class="header blue-text light"> + Two-stage glacial-interglacial forward model</h4> + <p>The forward model builds on the assumption of a + "two-stage uniformitarianism", meaning that the + processes that operated during the Holocene also + operated during earlier interglacials with comparable + intensity. Likewise, the erosion rate during the past + glacial periods is assumed to be comparable.</p> + + <p>The model approach assumes that glacial periods were + characterized by 100% shielding and no exposure, which + would require more than 10 m of ice thickness for + production due to spallation (&gt;50 m for muons). + Interglacial periods are assumed to have been + characterized by 100% exposure and zero shielding. The + production of TCNs takes place during the interglacials, + while erosion removes the land surface at different + rates during the glacials and interglacials.</p> + </div> - <p> - The computational time depends on the number of MCMC - walkers. When casually trying out the calculator we - recommend using low numbers of MCMC walkers (1 to 2) in - order to obtain fast results and reduce load on the server. - When attempting to produce high-quality and reliable - results, the number of walkers should be increased (3 to 4). - </p> + <div id="mcmcwalker" class="subsection scrollspy"> + <h4 class="header blue-text light"> + What is a MCMC walker?</h4> + <p> + A MCMC walker is in this context a numerical entity + which sequentially explores the model parameter space in + order to obtain the closest match between the forward + model and the observational dataset of TCNs. 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 in the same direction in model space. + </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. The MCMC walker continues + exploring the model space until it is sufficiently + satisfied with the best model parameter estimate it has + found. + </p> + + <p> + For a given observational data set more than one set of + model parameters may produce forward models which + sufficiently satisfy the MCMC walker. In this case the + solution is <i>non-unique</i>. Even worse, a single MCMC + walker may find an area in model space which seemingly + is in good correspondence with the observational data + set, but the walker is missing a much better set of + model parameters since they are located somewhere + entirely different in the model space. In order to + mitigate these issues, MCMC inversions are often + performed using several MCMC walkers. The starting + point of each MCMC walker is chosen at random, resulting + in unique walks through the model space. If a single + walker is caught in an area of non-ideal solutions, + chances are that the other walkers will find the area of + better model parameters. + </p> + + <p> + The computational time depends on the number of MCMC + walkers. When casually trying out the calculator we + recommend using low numbers of MCMC walkers (1 to 2) in + order to obtain fast results and reduce load on the + server. When attempting to produce high-quality and + reliable results, the number of walkers should be + increased (3 to 4). + </p> + </div> </div>