trestructure sentences - 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
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(DIR) commit 1d8bf4c603bb8c5c9084c8c7e3c82d0f6fe5a87d
(DIR) parent 92b401241f5faf7348a8517d6bd5d82bad18500e
(HTM) Author: Anders Damsgaard <anders.damsgaard@geo.au.dk>
Date: Fri, 27 Nov 2015 16:32:22 +0100
restructure sentences
Diffstat:
M pages/methods.html | 11 +++++------
1 file changed, 5 insertions(+), 6 deletions(-)
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(DIR) diff --git a/pages/methods.html b/pages/methods.html
t@@ -54,18 +54,17 @@
Markov-Chain Monte Carlo (MCMC) basics</h3>
<p>The inversion problem of turning observed TCN
concentrations into erosion histories is handled using a
- conventional Metropolis-Hastings MCMC approach where the
+ conventional Metropolis-Hastings MCMC approach. The
model parameters are constrained between fixed model
parameter bounds specified by the user. Erosion rates
(ε<sub>int</sub>, ε<sub>gla</sub>), which
- may vary over several orders of magnitude, are specified
+ may vary over several orders of magnitude, are tested
with uniform probability across the logarithmic parameter
interval. The temporal parameter (<i>t</i><sub>degla</sub>)
and climate record threshold value
- (δ<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.
+ (δ<sup>18</sup>O<sub>threshold</sub>) is tested with
+ uniform probability across the linear parameter interval.
+ The user specifies the bounds of the model parameters.
</p>
<p>When model parameters