NEW Merapi Volcano Imaging

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NEW Merapi Volcano Imaging
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From: Michael Ramsey <mramsey+@xxxxxxxx>

The ASTER sensor has continued observing the increasing volcanic activity
at Merapi Volcano, Indonesia. A night time shortwave infrared (SWIR) and 
thermal infrared (TIR) set of images were captured at 15:10 UTC time on 
the 14th of May. Compared to previous ASTER images, the data show a much 
more significant thermal anomaly including saturation in the TIR wavelengths
and detectable emissions down to 1.65 microns (ASTER band 4). Also present
is an elongated thermal anomaly (max of ~ 40 C) extending to the SW of 
the summit 1.7 km, presumably from the start of larger pyroclastic flows. 

The maximum surface temperature measured at the summit dome is now 442 C
over 3 SWIR pixels (30 m). This is a significant increase from a max of 
213 C detected just two days prior. The presence of the PF deposit and 
the marked increase in temperatures at the summit is evidence that dome 
collapse has and is continuing to occur, giving rise to the PF and 
exposing much higher temperatures over portions of the dome that have 
broken away. 

Two new images have been posted at the IVIS website and are located here:
http://ivis.eps.pitt.edu/data/merapi/

SWIR and TIR derived temperatures have been contoured and placed on the 
daytime VNIR image from 12 May. For comparison, note the differences in 
the following images:
http://ivis.eps.pitt.edu/data/merapi/12May06.pdf
http://ivis.eps.pitt.edu/data/merapi/051406_TC.pdf

ASTER will continue to observe the crisis in Indonesia. The next daytime 
images are scheduled for 19 May and 21 May, with a full VNIR-SWIR-TIR 
pass scheduled for 28 May.

For more information on ASTER, please see the NASA website here:
http://asterweb.jpl.nasa.gov/


-- Mike

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