Tuesday, September 16, 2014

ASTER high resolution imagery of the Holuhraun fissure, near Bardarbunga, Sept 16 2014, 12:32 UTC

The ASTER sensor captured the thermal signals from the fissure activity at 12:32 UTC, today, September 16, 2014. The data was from the Bands 3N, 2 and 1, so at 0.8, 0.66 and 0.55 microns respectively. Below is an RGB of these channels overlayed in Google Earth.


RGB of ASTER Channels 3N, 2, 1. 30 m resolution. Sept 16 2014, 12:32 UTC


Zoomed in on the active region. RGB of ASTER Channels 3N, 2, 1. 30 m resolution. Sept 16 2014, 12:32 UTC

Examining the hottest portion of the region, likely the active fissure, this is 630 m long.  There are two other points that show significant thermal signatures. Seem zoomed in view below. These are 400 m approx from the fissure, 160 m apart.


Zoomed in on the additional active locations. RGB of ASTER Channels 3N, 2, 1. 30 m resolution. Sept 16 2014, 12:32 UTC.

Displaying the 3N channel, 0.8 microns, only, we are able to see the portion that is the most thermal active. We can enhance the 3N data to see the full flow off to the northeast of the most active feature,


Zoomed in on the active region. Black and White of ASTER Channel 3N. 30 m resolution. Sept 16 2014, 12:32 UTC


Zoomed in on the active region. Enhanced Black and White of ASTER Channel 3N. 30 m resolution. Sept 16 2014, 12:32 UTC

For more information on the real-time activity, see the Icelandic Met. Office [http://en.vedur.is/] and for a volcanic ash advisories see the London VAAC [http://www.metoffice.gov.uk/aviation/vaac/].

This is my interpretation of the ASTER data. Thanks to the NASA LP DAAC for access to this data.



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