Colour-changing dust cloud vortex

Colour-changing dust cloud vortex

01 February 2017 00:00 UTC–02 February 12:00 UTC

Colour-changing dust cloud vortex
Colour-changing dust cloud vortex

Dust in northern Iraq shows different colours before and after circulation.

Last Updated

09 August 2021

Published on

31 January 2017

By Vesa Nietosvaara, Jose Prieto and Jochen Kerkmann (EUMETSAT)

Dust presents different hues on satellite channel composites. The reasons are not yet clear.

Meteosat-8 Dust RGB, 2 Feb 07:00 UTC
Meteosat-8 Dust RGB, 2 Feb 07:00 UTC

The Meteosat-8 Dust composite with the ECMWF 10m-wind and mean sea level pressure overlaid, Figure 1 and infrared composite animation ,  01 February 2017 00:00 UTC–02 February 12:00 UTC indicate the presence of a weak circulation in the Middle East area, close to northern Iraq.

The wind associated with the cyclonic circulation on eastern Syria raises dust south of it, as shown in the infrared animation around 10:00 UTC on 1 February.

Over the northwestern part of Iraq, the dust joins the circulation along the south flank (red and pink on the left hand side of Figure 2), but it comes out mostly from the cyclone's west flank with a peach hue near Iraq's eastern border. An influence of the ground in the coloration is not evident. The time of the day plays no role, since the same hues show day and night.

Image comparison

Image from 2 Feb, 06:00 UTC compare1
compare2
 

Figure 2: Comparison of two different moments in the evolution of the dust area.

Both Meteosat-8 and -10 see the same colours, so the viewing angle through a thicker humidity layer is not a sufficient explanation. Differences are only around 1 K between the measurements by the two satellites, so slant effects are not impacting colour hue either.

Orange (or peach) colour results from higher green, which is a larger positive Brightness Temperature Difference (BTD) between channels at 10.8µm and 8.7µm. In cloud free areas bigger BTD comes from higher water vapour, whereas in cloudy areas this BTD is affected by 1) dust height, 2) dust concentration and 3) dust properties, mainly particle size.

If the reason for peach hues in this case would be dust particle size, one could imagine coalescence in the upward circulation, followed by drying up close to the circulation boundaries and the creation of dry bigger dust particles, producing the peach tone. That is suggested by the fact that volcano eruptions (made of big particles) show often in peach in the window infrared composite.

Figure 3 is analysis for all pixels inside the red square on the left Meteosat-10 IR composite image. The graph on the right hand side compares 10.8 µm–8.7 µm differences (vertical axis) and values at 12 µm (horizontal). The peach coloured pixels (exit of a conveyor belt) show a BTD 10.8 µm–8.7 µm which is around one kelvin higher than the magenta-red pixels at the southern part of the conveyor belt. Height or size effect?

   Figure 3: Meteosat-10 IR composite, 2 February 00:00 UTC and BTD graph.
   Figure 3: Meteosat-10 IR composite, 2 February 00:00 UTC and BTD graph.
 

This Meteosat-10 Dust RGB with ECMWF 2 m temperature lines , shows similar temperatures close to the ground in both pink and peach areas of dust contamination.

Any alternative suggestions for an explanation of this colour shift are welcome, please email our Helpdesk.


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