The formation of
hot spots in dynamically compressed, plastic-bonded
explosives is known to be the primary mechanism by which these materials
ignite and initiate, but hot spots are small, fleeting, and hard to
observe. Using a microscope equipped with laser-launched, miniflyer
plates, we have studied hot spots in small grains of cyclotetramethylene-tetranitramine
(HMX) embedded in a polyurethane binder, shocked to about 20 GPa.
A nanosecond video with 4 μm spatial resolution is used to observe
hot spot formation and growth, while nanosecond optical pyrometry
measured temperature. Using individual ∼200 μm nominally
single crystals of HMX (HMX-SC), we observed hot spots forming preferentially
on corners or edges. These hot spots are about 4000 K. When there
are multiple hot spots, the flame propagated along crystal edges,
and the crystal is mostly combusted after about 300 ns. Using polycrystalline
grains (HMX-PC), 6000 K hot spots are created near internal defects
or crystal junctions. However, the thermal mass of the material at
6000 K is quite small, so after those hot spots cool down, the HMX
combustion is similar to the single crystals. Comparing a HMX-based
polymer-bonded explosive (PBX) to the individual polymer-bonded HMX-SC
and HMX-PC grains shows that the myriad hot spots in the PBX are hotter
than HMX-SC and colder than HMX-PC, but they persist for a longer
time in PBX than in the individual grains.
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