trearrange card content - 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 cd16bf83c2780e10e95feaa249d2c9cd2ac5a70a
(DIR) parent 7a9890ce43337c2b72e1e458186f652573fe2a3d
(HTM) Author: Anders Damsgaard <anders.damsgaard@geo.au.dk>
Date: Mon, 9 Nov 2015 12:52:24 +0100
rearrange card content
Diffstat:
M index.php | 35 +++++++++++++++++++++++++++++++
1 file changed, 35 insertions(+), 0 deletions(-)
---
(DIR) diff --git a/index.php b/index.php
t@@ -108,6 +108,41 @@ if (isset($_GET['wait_id']) && !empty($_GET['wait_id'])) {
</div>
<div class="row">
+ <!--<div class="col s12 m8 offset-m2">-->
+ <div class="col s12 m10 offset-m1">
+ <div class="card">
+ <div class="card-content">
+ <span class="card-title blue-text text-darken-2">
+ <b>Model parameter values</b></span>
+ <img src="output/<?php
+ echo($_GET['results_id']); ?>_Walks-5.png">
+ <p>The histograms show the distribution of (a)
+ interglacial erosion rate, (b) glacial erosion rate, (c)
+ timing of last deglaciation, and (d)
+ d<sup>18</sup>O<sub>threshold</sub> levels that provide
+ the best fit to the supplied TCN concentrations. There is
+ one histogram per model parameter for each MCMC walker.
+ The <!--fraction indicates the number of simulations
+ included in--> vertical axis indicates the number of
+ simulations included in each bin out of the 10,000
+ simulations that followed the MCMC burn-in phase.</p>
+ </div>
+ <div class="card-action">
+ <a href="output/<?php
+ echo($_GET['results_id']); ?>_Walks-5.png"
+ target="_blank">Link to PNG</a>
+ <a href="output/<?php
+ echo($_GET['results_id']); ?>_Walks-5.pdf"
+ target="_blank">Link to PDF</a>
+ <a href="output/<?php
+ echo($_GET['results_id']); ?>_Walks-5.fig"
+ target="_blank">Link to FIG</a>
+ </div>
+ </div>
+ </div>
+ </div>
+
+ <div class="row">
<div class="col s12 m10 offset-m1">
<div class="card">
<div class="card-image">