Figures & data
FIG. 1 The burner and the experimental setup used to sample soot particles in the ethylene diffusion flame.
![FIG. 1 The burner and the experimental setup used to sample soot particles in the ethylene diffusion flame.](/cms/asset/bc246b90-8ff1-496a-994f-05591bdbb262/uast_a_507228_o_f0001g.gif)
TABLE 1 Gaussian fit parameters for the four sampling protocols TPP, TPS, IPS, and NFS, with standard deviation in parentheses
FIG. 2 TEM micrographs of samples collected by TPP, TPS, IPS, and NFS and stored in a N2 atmosphere in the dark.
![FIG. 2 TEM micrographs of samples collected by TPP, TPS, IPS, and NFS and stored in a N2 atmosphere in the dark.](/cms/asset/6b5fb0f0-63b1-4755-938b-b8a8668a002d/uast_a_507228_o_f0002g.gif)
FIG. 3 Probability density function of the gyration diameter obtained for the four sampling protocols (Number of aggregates analyzed: 211 for TPP, 141 for TPS, 202 for IPS, and 225 for NFS).
![FIG. 3 Probability density function of the gyration diameter obtained for the four sampling protocols (Number of aggregates analyzed: 211 for TPP, 141 for TPS, 202 for IPS, and 225 for NFS).](/cms/asset/8999c9d4-0dcb-4d13-b544-a9ad97ce0cae/uast_a_507228_o_f0003g.gif)
FIG. 4 The number of primary particles in the aggregates as a function of the ratio between gyration and primary particle diameters.
![FIG. 4 The number of primary particles in the aggregates as a function of the ratio between gyration and primary particle diameters.](/cms/asset/f071de3e-06c9-407c-85d7-70284f58cda0/uast_a_507228_o_f0004g.jpg)