meso-web

Sources of the |Méso|Star> website
git clone git://git.meso-star.fr/meso-web.git
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commit a995a1c3a64ff3d02dbf3d1aeb6a08e90457edba
parent 2008410fc549a818d58027932eab2e0860624f2b
Author: Vincent Forest <vincent.forest@meso-star.com>
Date:   Tue, 31 Aug 2021 15:23:46 +0200

Small upd of the htrdr overview

Diffstat:
Mhtrdr/Makefile | 2++
Mhtrdr/htrdr.html.in | 20++++++++++----------
2 files changed, 12 insertions(+), 10 deletions(-)

diff --git a/htrdr/Makefile b/htrdr/Makefile @@ -25,6 +25,7 @@ HTML = \ htrdr-docs.html IMG = \ city.jpg \ + city_thin_lens.jpg \ CLEMENT.jpg \ CLEMENT_lw_9000_10000.jpg \ downward_flux_500x500x2048_lw_4000_100000_425.156.jpg \ @@ -33,6 +34,7 @@ IMG = \ dummy_medium_clipped.jpg \ DZVAR2.jpg \ DZVAR.jpg \ + DZVAR_ortho.jpg \ HRES_ARMCu.jpg \ L12km_BOMEX.jpg \ L25_Fire.jpg \ diff --git a/htrdr/htrdr.html.in b/htrdr/htrdr.html.in @@ -79,19 +79,19 @@ used for computing various quantities:</p> <ul> <li> -<p><b>Images</b> on a camera sensor, in a given field of view. For combustion - applications, only monochromatic images are supported. In atmospheres, both - visible and infrared images are possible: CIE colorimetry is used for visible - images, while and infrared image is in fact a brightness temperature map, - obtained from the incoming radiative flux over the required spectral - interval</p> + <p><b>Images</b> on a camera sensor, in a given field of view. For combustion + applications, only monochromatic images are supported. In atmospheres, + spectral integration is also possible, both for solar and thermal images: CIE + colorimetry is used for solar images, while thermal images are in fact + brightness temperature maps, obtained from the incoming radiative flux over a + specified spectral interval.</p> </li> <li> -<p><b>Flux density maps</b>, on a grid of sensors, integrated over an entire + <p><b>Flux density maps</b>, on a grid of sensors, integrated over an entire hemisphere. In the case of combustion chambers, only monochromatic flux maps - can be calculated, while spectrally integrated flux density maps (both on the - visible part of the spectrum and on the infrared) are possible for - atmospheric applications.</p> + can be calculated, while spectrally integrated flux density maps are also + possible for atmospheric application, both for solar and thermal + radiation.</p> </li> </ul>