A coal sample was prepared from a Western Australia sub-bituminous
coal via density separation (1.4–1.6 g/cm3) and
size separation (63–90 μm). The mineral matter in the
coal is of included nature, of which ∼90% are fine mineral
particles <10 μm. The raw coal was then washed by dilute
acid to prepare an acid-washed coal from which char sample was generated
in a quartz drop-tube/fixed-bed reactor at 1000 °C under argon
atmosphere. The acid-washed coal and char samples were then combusted
in a drop-tube furnace at 1400 °C in air. The PM10 samples collected (mostly PM1–10) contains mainly
refractory species including Si, Al, Fe, Mg, and Ca and account for
∼19.4% of the total ash collected in both the low-pressure
impactor and the cyclone. This suggests important roles of the abundant
fine included mineral particles originally present in coal. The significant
roles of fine included mineral particles in PM1–10 emission during acid-washed coal and char combustion are also clearly
evidenced with the presence of abundant individual but partially molten
quartz ash particles in the PM1–10 range. PM0.1 contains dominantly volatile elements (e.g., Na, K, P,
S, and Cl) and refractory elements (Fe and Si), while PM0.1–1 are mainly composed of Al, Fe, and Si. The significant roles of
fine included kaolinite and/or Al-silicates particles in the emission
of PM0.1–1 from char combustion are also observed.
The results suggest that liberation and transformation of fine included
mineral particles in coal/char during combustion is a key mechanism
responsible for PM10 formation and/or emission. Experimental
evidence further suggests that the fine included minerals within a
burning coal particle clearly experience coalescence to form large
agglomerated ash particles.