commit 32cedb4ec127122f5dfa68992d4bbdd29e2755b2
parent 99f449ab587a54a5f26a827e2f62156f46175346
Author: Vincent Forest <vincent.forest@meso-star.com>
Date: Fri, 27 Nov 2020 11:11:14 +0100
Add flux maps to the high-tune overview page
Diffstat:
4 files changed, 50 insertions(+), 5 deletions(-)
diff --git a/high-tune/Makefile b/high-tune/Makefile
@@ -17,7 +17,17 @@ HTRDR-VERSION=0.6.1
HTRDR-STARTER-PACK-VERSION=0.6.0
SRC = high-tune.html.in high-tune.sh
-IMG = CLEMENT.jpg DZVAR.jpg DZVAR2.jpg L12km_BOMEX.jpg L25_Fire.jpg HRES_ARMCu.jpg CLEMENT_lw_9000_10000.jpg city.jpg
+IMG = \
+ city.jpg \
+ CLEMENT.jpg \
+ CLEMENT_lw_9000_10000.jpg \
+ downward_flux_500x500x2048_lw_4000_100000_425.156.jpg \
+ downward_flux_500x500x2048_sw_380_4000_879.349.jpg \
+ DZVAR2.jpg \
+ DZVAR.jpg \
+ HRES_ARMCu.jpg \
+ L12km_BOMEX.jpg \
+ L25_Fire.jpg
.PHONY: all clean default publish
default: all
diff --git a/high-tune/downward_flux_500x500x2048_lw_4000_100000_425.156.jpg b/high-tune/downward_flux_500x500x2048_lw_4000_100000_425.156.jpg
@@ -0,0 +1 @@
+#$# git-wad b18eb54be4c6d3558081cd01f5684383cb49c2fe7387e5e23bd651e7f10b6c07 192351
+\ No newline at end of file
diff --git a/high-tune/downward_flux_500x500x2048_sw_380_4000_879.349.jpg b/high-tune/downward_flux_500x500x2048_sw_380_4000_879.349.jpg
@@ -0,0 +1 @@
+#$# git-wad bb04ec3cf9146f8d10772bed664c981129c56a55bd5b3d215fddf84997d44cda 200302
+\ No newline at end of file
diff --git a/high-tune/high-tune.html.in b/high-tune/high-tune.html.in
@@ -95,7 +95,7 @@ run either directly or through a MPI process launcher like <code>mpirun</code>.
<img src="CLEMENT.jpg" alt="CLEMENT">
</a>
<div class="caption">
- Image rendered with htrdr of a 500<sup>3</sup> cloud field produced by the
+ Image rendered with htrdr of a 1000<sup>3</sup> cloud field produced by the
Meso-NH (<a
href="https://www.ann-geophys.net/16/90/1998/angeo-16-90-1998.html">Lafore et
al 1998</a>, <a href="https://www.geosci-model-dev.net/11/1929/2018/">Lac et
@@ -148,7 +148,7 @@ following research projects.</p>
<img src="CLEMENT_lw_9000_10000.jpg" alt="CLEMENT_lw">
</a>
<div class="caption">
- Infrared rendering in [9000, 10000] nanometers of the 500<sup>3</sup> cloud
+ Infrared rendering in [9, 10] micrometers of the 500<sup>3</sup> cloud
field of <a
href="https://rmets.onlinelibrary.wiley.com/doi/full/10.1002/qj.3614">Strauss
et al. (2019)</a>. The color map displays the brightness temperature in
@@ -177,6 +177,35 @@ href="https://imagemagick.org/script/display.php">display</a>.
<h2>Quick start</h2>
+<div class="img" style="width: 20em">
+ <div style="width: 46%; float: left; padding: 1%">
+ <a href="downward_flux_500x500x2048_sw_380_4000_879.349.jpg">
+ <img src="downward_flux_500x500x2048_sw_380_4000_879.349.jpg" alt="downward_flux_sw">
+ </a>
+ </div>
+
+ <div style="width: 46%; float: left; padding: 1%">
+ <a href="downward_flux_500x500x2048_lw_4000_100000_425.156.jpg">
+ <img src="downward_flux_500x500x2048_lw_4000_100000_425.156.jpg" alt="downward_flux_lw">
+ </a>
+ </div>
+ <div class="caption" style="clear: both">
+ Shortwave (left) and longwave (right) downward flux density maps in
+ W/m<sup>2</sup> computed at 1 meter height for the <a
+ href=starter-pack.html>DZVAR</a> cloud field. The shortwave and longwave
+ spectral integration ranges are [0.38, 4] micrometers and [4, 100]
+ micrometers, respectively. Their spatially-avaraged flux is
+ 879.349 W/m<sup>2</sup> in shortwave and 425.159 W/m<sup>2</sup> in
+ longwave. In both cases, the spatial position is the sub-solar point, meaning
+ that the sun is located at the zenith. In the shortwave map we observe the
+ contrast between the shadows of the clouds and fully illuminated areas. In
+ longwave, we can see the effect of clouds (higher values, due to the emission
+ by the base of the cloud at higher temperatures than for a clear-sky zone)
+ and also a "ripple" effect that is due to the spatial variations of water
+ vapor concentration, as provided by the LES simulation.
+ </div>
+</div>
+
<p>No pre-compiled version of <code>htrdr</code> is provided; it must be
compiled directly from its source tree. A simple way is to rely on the
<code>high_tune</code> branch of the <a
@@ -205,8 +234,10 @@ procedure is summed up to:
<pre class="code">
~ $ git clone -b High-Tune-${VERSION} \
- https://gitlab.com/meso-star/star-engine.git High-Tune-${VERSION}
-~ $ mkdir High-Tune-${VERSION}/build; cd High-Tune-${VERSION}/build
+ https://gitlab.com/meso-star/star-engine.git \
+ High-Tune-${VERSION}
+~ $ mkdir High-Tune-${VERSION}/build
+~ $ cd High-Tune-${VERSION}/build
~/High-Tune-${VERSION}/build $ cmake ../cmake
~/High-Tune-${VERSION}/build $ make
</pre>
