tremove attempt - 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 79c30468f12e186dac1984ca4d3bab5140469549
(DIR) parent cd16bf83c2780e10e95feaa249d2c9cd2ac5a70a
(HTM) Author: Anders Damsgaard <anders.damsgaard@geo.au.dk>
Date: Mon, 9 Nov 2015 12:52:57 +0100
remove attempt
Diffstat:
M index.php | 35 -------------------------------
1 file changed, 0 insertions(+), 35 deletions(-)
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(DIR) diff --git a/index.php b/index.php
t@@ -108,41 +108,6 @@ 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">