Figures & data
FIG. 2 Measured gas temperature evolution with time along the lower part of the heated tube, refractory section, and chimney. The sampling points used for studying the particle formation process are marked.
![FIG. 2 Measured gas temperature evolution with time along the lower part of the heated tube, refractory section, and chimney. The sampling points used for studying the particle formation process are marked.](/cms/asset/5b1077d7-67f5-40e1-b9e0-9345c6e37a44/uast_a_9705903_o_f0002g.gif)
FIG. 4 Measured and predicted pressure and static temperature evolution with length along the AQPS probe.
![FIG. 4 Measured and predicted pressure and static temperature evolution with length along the AQPS probe.](/cms/asset/05e607bd-060c-4dac-8947-5f41b506282e/uast_a_9705903_o_f0004g.gif)
TABLE 1 Proximate and ultimate ASTM analysis and inorganic matter composition of the sieved orujillo
FIG. 5 Particle size distribution of the final emissions. Note the difference between the scales for both modes. (dLog10Dp equals 0.0664 for the laser diffractometer and ∼0.31 for the BLPI).
![FIG. 5 Particle size distribution of the final emissions. Note the difference between the scales for both modes. (dLog10Dp equals 0.0664 for the laser diffractometer and ∼0.31 for the BLPI).](/cms/asset/1a1c2e2c-aa81-4d8d-8a70-3dc3b7768497/uast_a_9705903_o_f0005g.gif)
FIG. 6 DMA-derived PSD distribution (mass basis) compared with the BLPI result. Both series have been normalized by their peak height.
![FIG. 6 DMA-derived PSD distribution (mass basis) compared with the BLPI result. Both series have been normalized by their peak height.](/cms/asset/194d7912-62e2-466f-b708-0611c088aac7/uast_a_9705903_o_f0006g.gif)
FIG. 7 Chemical composition (in a mass basis) of deposits on BLPI stages 1 through 6, and 8 and 9, compared with the mineral matter composition of the original fuel.
![FIG. 7 Chemical composition (in a mass basis) of deposits on BLPI stages 1 through 6, and 8 and 9, compared with the mineral matter composition of the original fuel.](/cms/asset/ae252090-b1fa-4036-83d2-2fe33f592b47/uast_a_9705903_o_f0007g.gif)
FIG. 8 X-ray diffractogram of a sample from stage 4 of the BLPI (dp = 100 nm). The aluminum substrate peaks are identified.
![FIG. 8 X-ray diffractogram of a sample from stage 4 of the BLPI (dp = 100 nm). The aluminum substrate peaks are identified.](/cms/asset/db4283f4-78ea-4343-8864-fd99335dde26/uast_a_9705903_o_f0008g.gif)
FIG. 11 TEM pictures of samples collected in the EFR using the AQPS probe at (a) 1300°C, (b) 900°C, and (c) 560°C. (Continued)
![FIG. 11 TEM pictures of samples collected in the EFR using the AQPS probe at (a) 1300°C, (b) 900°C, and (c) 560°C. (Continued)](/cms/asset/4b4959d6-b7ca-4898-b739-73b4a3bb3047/uast_a_9705903_o_f0011ag.gif)
![FIG. 11 TEM pictures of samples collected in the EFR using the AQPS probe at (a) 1300°C, (b) 900°C, and (c) 560°C. (Continued)](/cms/asset/d54bcdd9-afd7-4937-a5e4-f90629b7e731/uast_a_9705903_o_f0011bg.gif)
![FIG. 11 TEM pictures of samples collected in the EFR using the AQPS probe at (a) 1300°C, (b) 900°C, and (c) 560°C. (Continued)](/cms/asset/8af31404-e768-4c95-a6b3-021ab64a1429/uast_a_9705903_o_f0011cg.gif)
FIG. 12 TEM-XEDS spectra of samples collected at 900°C and 560°C. Both curves have been normalized by their K (Kα) peak height. The small peaks to the left of P are spurious due to the measurement technique.
![FIG. 12 TEM-XEDS spectra of samples collected at 900°C and 560°C. Both curves have been normalized by their K (Kα) peak height. The small peaks to the left of P are spurious due to the measurement technique.](/cms/asset/b3610c73-ca48-4bd5-a24e-ce931db11ab6/uast_a_9705903_o_f0012g.gif)