3.1. Elemental Composition
The elemental composition of the ashes was analysed using X-Ray Fluorescence spectrometry (XRF). Samples of LCA collected from PSA and PSB were analysed alongside CFA samples collected from PSD power station. In all the analysed samples the major elements (as oxides in weight %) were SiO
2 and Al
2O
3. The minor oxides detected in the samples (both LCA & CFA) in the order of their respective relative abundances were; CaO > Fe
2O
3 > TiO
2 > P
2O
5 > K
2O > Na
2O. The typical elemental composition of the LCA samples collected from PSA power station is presented in
Figure 2.
Overall, there was minimal variation in both the major and minor elements with time, and this observation was consistent in all the other tested samples. SiO2 and Al2O3 were the predominant elements, with a total percentage composition of > 70 % at any given time throughout the sampling.
There were slight variations in the elemental composition over the sampling period for both the PSD (CFA) samples and the other LCA samples. These outcomes were expected due to the low proportion of inorganic elements that volatilise during the combustion of South African feed coals [
20]. Collins at al., reported on the elemental composition of a blend of South African coal ashes and the wt. % ranges were; CaO (1.5 – 13), Fe
2O
3 (2.0 – 5.7), TiO
2 (1.3 – 1.8), P
2O
5 (0.1 -0.3), K
2O (1.1 – 16.1) and Na
2O (0 – 0.1) [
21]. In other related studies on the elemental composition of South African coal ashes (Van Dyk et al., and Matjie et al, are consistent with the observations made in this study [
22,
23]. Averages of the elemental composition wt. % of the tested ashes are presented in
Table 3.
Thus, according to the ASTM C618 specification, the LCA and the CFA are compliant with pozzolanic material class F, siliceous ash; (sum of SiO
2, Al
2O
3, and Fe
2O
3 should be > 70 %). There are very slight variations in the composition of the LCA over time, for instance the sample collected from PSA power station; the average percentages were 87.59, 88.51, and 88.28 % for daily, weekly, and monthly variations respectively. These slight variations are attributed to the fact that coal is inherently heterogeneous and even though the coal might have been coming from the same mine variations would be expected. The exact composition of the LCA is influenced by several factors namely; raw coal source, particle size, type of coal burner, and the operating conditions of the burner, which differ with each power station, thus the differences in the elemental composition of ashes from different stations [
24]. Rafieizonooz et al., reported on the composition of Malaysian CBA and CFA and the total wt. % of SiO
2 + Al
2O
3 + Fe
2O
3 was 83.24 % and 78.82 % respectively [
25]. Other previous studies on CFA and CBA elemental composition reported comparable outcomes for the CBA and CFA elemental composition [
11,
26,
27]. In some of the studies, the CaO wt. % composition was lower than that of Fe
2O
3, contrary to the observation made in this study, for instance, Rafieizonooz et al., reported the CaO and Fe
2O
3 in Malaysian CBA to be 8.7 % and 19.84 % respectively, while Sanjith et al., reported the CaO and Fe
2O
3 in Indian CBA to be 7.44 % and 4.29 % respectively [
25,
29]. The ratio of CaO : Fe
2O
3 may also be influenced by the fact that some of the power stations especially in Europe, America, and Asia use washed coal for power generation. Coal washing reduces the amount of pyrite in the coal and hence the amount of Fe
2O
3 produced in the resultant ash. It should be noted that Eskom, the South African power utility uses feed coals that typically consist of a fraction of washed coal and a high-ash discard. In some instances, unwashed run-of-mine coal or de-stoned coal can be part of the mix [
29]. Despite this, variations of LCA composition are to be expected since the composition is largely influenced by the source and nature of the incinerated coal.
3.2. Mineral Composition
Peaks due to mullite, quartz, sillimanite, and haematite were clearly visible in the XRD patterns obtained for both the CFA and LCA samples tested. These mineral phases are characteristic of class F material [
30]. Both diffractograms presented in
Figure 3(a) and (b) were characterised by a broad hump centred at 26.5° 2θ which attests to the presence of amorphous material in the tested samples [
31]. In some samples, minor fractions of leucite, magnetite, dolomite, and limenite were detected. In the tested samples there was minimal variation in the mineral phases with time, in all the samples analysed. The silica and aluminosilicate, mineral phases formed are governed by 3 major factors, namely: (i) how reducing or oxidising is the environment in which they are formed, (ii) the presence of rare elements. In power stations and boilers where the atmosphere is reducing there is a tendency towards the formation of quartz, magnetite, and mullite. Furthermore, the distribution of these mineral phases ought to change with temperature changes [
32,
33].
Generally, the mineral matter that makes up coal consists of pyrite (cubic FeS
2), kaolinite (Al
2Si
2O
5(OH)
4), and calcite (CaCO
3). Other common minerals include marcasite (orthorhombic FeS
2), chalcopyrite (CuFeS
2), arsenopyrite (FeAsS), stibnite (Sb
2S
3), gypsum (CaSO
4·2H
2O), quartz (SiO
2), dolomite (CaMg(CO
3)
2), apatite (Ca
5(PO
4)
3F) and mica. Thus, the quartz in the diffractogram of both the CFA and the LCA is due to its natural occurrence in coal [
34]. Pure quartz particles can enter the gasifiers and boilers and resist phase transformation even at temperatures of ± 1200 °C [
35]. Phase transformation of kaolinite (naturally occurring in coal) at these temperatures is responsible for the formation of mullite. It is also possible for mullite to crystallise from molten solution due to the reactions of kaolinite with fluxing minerals (i.e. dolomite, calcite, and pyrite) [
20]. Another mineral phase which was detected in both the tested CFA and LCA was sillimanite, which is one of the polymorphs of Al
2SiO
5. At temperatures above 1200 °C, sillimanite is transformed into mullite, with complete mullitisation occurring at the temperature range 1500 °C - 1600 °C [
36,
37]. The mullite formation occurs in accordance with the reaction: (3Al
2O
3 + 2SiO
2 → 3Al
2O
3·2SiO
2, ΔG = −24.06 kJ/mol, 1200 °C).
Some minor minerals were detected in the CFA sample such as lime, clinopyroxene, and magnesioferrite. The presence of lime is due to the high-temperature decomposition of calcite (and maybe gypsum) present in coal [
34]. Magnesioferrite is produced when ankerite Ca(Fe
2+,Mg)(CO
3)
2 (one of the dominant carbonate minerals in coal) is heated to temperatures of about 1000 °C. The breakdown of ankerite also results in the formation of periclase and calcite ([
38,
39]. Clinopyroxene is formed by the reactions between SiO
2, Al
2O
3, Fe
2O
3, and CaO at temperatures below 1200 °C. The ratio of CaO : Fe
2O
3 may influence the formation of the mineral phase, and higher ratios favour the formation of clinopyroxene [
40]. Typical plots for the variation of major mineral phases over a period of 24 hours are presented in
Figure 4(a) PSB power station LCA samples (b) PSD power station CFA samples.
Throughout the 24-hour sampling period, the PSB (LCA) samples had mullite as the most abundant mineral phase. Hematite was relatively low in all the tested samples ranging from 1.7 to 5.7 wt. % over the sampling times. Sillimanite was generally low apart from the sample taken at 10:00 where there was 35.1 wt. % alongside a reduced amount of 45.9 wt. % of mullite. This may be attributed to the temperature swings that occur in some regions of the boiler. Temperatures below 1200 °C are associated with the presence of mullite and sillimanite will appear as the temperature goes above 1200 °C. Further evidence to indicate that the boiler temperature at the time of sampling was lower than 1200 °C, is the existence of aragonite which thermally decomposes at 1000 °C. The mineral composition of aragonite is not presented in
Figure 4(a) but was detected in the tested sample. It also has to be noted that the presence of aragonite suppresses the formation of mullite by reducing the ash fusion temperature, thus the lower wt. % of mullite detected in the sample [
41]. The same sample also had the highest wt. % of quartz, and this could be attributed to the decomposition of muscovite which occurs at temperatures around 850 °C (muscovite is formed from the initial kaolinite present in coal). Furthermore, the ashing temperature for coals is 815 °C and at this point, the ash composition is dominated by simple oxides and quartz levels are at their maximum [
42].
The mineral composition analysis of PSD Power Station coal fly ash indicated that sillimanite, quartz, and hematite minerals were present in all sampled time intervals. Interestingly, mullite was present for most of the sampling intervals except for those in which sillimanite was > 50 % (i.e., time – 12:00 and 13:00). This again can be attributed to the temperature dependence of the sillimanite-mullite phased transformation. Low levels of hematite, lime, and magnesite were detected in the sample. Generally, the major mineral phases and their relative abundances in the tested samples were comparable and the variation of these mineral phases were largely due to the temperature variation of the boilers, in addition to the heterogeneity of the coal itself. The averages of the mineral composition of the ash samples collected from the four power stations are presented in
Table 4.
A comprehensive analysis of the variability of the PSC and PSA power stations ash types was carried out over much longer periods; firstly, over 5 weeks taking samples every week, and secondly over a period of 4 months. The weekly samples were collected in June/July and the monthly samples were collected in June, July, August, and September of 2022. The mineral variations are presented in
Figure 5 and
Figure 6.
Generally, the order of mineral relative abundance followed the order mullite > quartz > sillimanite > hematite. In some samples, magnesite and lime were detected. The trends for both the weekly and monthly variations are also comparable. The temperature variation and coal inhomogeneity can be ascribed to be the chief governing factors in determining the variation of these major ash minerals. This is in addition to the fact that the chemistry and mineralogical composition of the incinerated coals at the different power stations would differ. A summary of the variations of these minerals in the tested samples is presented in
Table 5.
The wt. % mean values for mineral phases for weekly and monthly data sets were comparable for each respective LCA sample. The highest standard deviation recorded was 5.19 for mullite in the PSA (LCA) samples with hematite having a low standard deviation of < 2 in all samples over the weekly and monthly variation analysis. In a study on the mineralogy of Brazilian coal ashes, Silva et al., analysed 7 samples of CFA and CBA and the mineral phase wt. % range in CFA was; quartz (17.02 – 44.55 %), and mullite (60 – 69.7 %) [
43]. With the CBA samples, the ranges were; quartz (31.44 – 41.89 %), mullite (55.56 – 69.82 %), and hematite (0 – 0.3 %). Generally, the mineralogy of the tested samples is consistent with numerous other studies on CBA and CFA [
44,
45,
46].
3.3. Particle Size Distribution
The particle size distribution of the coal ashes collected from four different power stations was analysed and
Figure 8 shows the PSD (CFA) and PSB (LCA), Dv(10), Dv(50), and Dv(90) plotted against time for the samples collected over 24 hours. The PSD (CFA) had a consistent particle size distribution over the sampling period. The LCA sample showed some slight variation, and the same was observed with the other two LCA samples (PSA and PSC).
As expected, the CFA had a lower particle size distribution, in comparison to the LCA sample, the mean Dv(50) values were 24.15 µm and 30.62 µm for the CFA and LCA respectively while the mean specific area was 864.44 m²/kg and 532.04 m²/kg. Guan et al., reported on the particle size distribution of LCA samples collected from 4 power stations in China and the Dv(50) values ranged from 9.28 – 28.47 µm [
47]. In the same report, a sample of CFA was also analysed and the Dv(50) value was 19.07 µm. These values are also consistent with those reported by Kim & Do, on the analysis of Korean CFA and CBA [
48]. The variation of the particle size distribution of LCA over 5 weeks and over 4 months was done with the PSA and PSC samples and is presented in
Figure 8. The particle size distribution curves show that all samples had good continuity and minimal variations over the respective sampling periods. There however was some noticeable variation in the weekly samples collected from PSA, but each of the samples exhibited good continuity. Rafieizonooz et al., reported the particle size distribution of Malaysian CFA and CBA, and the CFA particle size range was 0.5 µm – 250 µm, while the CBA range was 7.5 µm – 1320 µm [
25]. The data obtained in this study is within the ranges reported. Similar profiles for CBA particle size distribution were obtained by [
47,
49,
50].
The particle size analysis for both the CFA and LCA samples revealed that the grains are predominantly made up of clay, silt and sand sized particles. The average daily, weekly and monthly uniformity coefficient (Cu) and coefficient of curvature (Cc) for the coal ash samples are presented in
Table 6. The (C
u) and (C
c) were computed using expression (i) and (ii) respectively.

The PSD coal fly ash, the PSC and PSA coal legacy ash samples fell within the sand-well graded class (Cu > 6 and 1 < Cc < 3), with only the PSB coal legacy ash samples falling in the gravel-well graded class (Cu > 4 and 1 < Cc < 3). The ash classes remained consistent over the sampling periods, daily, weekly and monthly despite the changes in burner temperatures and other combustion conditions. The Cu and Cc data for LCA obtained in this study is consistent with data reported in related studies on Malaysian CBA which was classified as sand-well graded [
51,
52]. In another related study by Asvesta et al, in which CBA samples from 4 different Greek powers stations were analysed, 3 of the samples had grain size classification consistent with that of the PSB samples [
53].
3.4. Acid-Base Accounting
The acid-base accounting was done based on the static test results as presented by Sobek et al., Lawrence, R.W. & Wang, and Morin & Hutt, [
17,
19,
54]. The classification is based on the net neutralising potential (NNP), and this classification, an NNP value of 0 with a paste pH of 4 is classified as acid generating. The x-y scatter plots of the NNP vs paste pH for daily, weekly, and monthly samples are presented in
Figure 9. Sulphur quantification can also be regarded as a form of predicting acid-forming behaviour in solid particulate matter. In the tested samples the highest total sulphur wt. % recorded was 0.32 % for PSD (CFA) sample. The other three groups of LCA samples had a total sulphur concentration of < 0.2 %. The low total sulphur levels signify low acid-forming potential. It was also expected that the CFA would have a higher total sulphur content compared to the LCA samples, since CFA interacts with the produced SO
x in the flu gas stream which does not occur with the CBA which makes part of the LCA. The SO
x- sulphur can then adsorb to the fly ash particles and be retained on the surface while part of it may end up reacting with metal oxides to form various sulphite or sulphate end products [
55]. The reasonable levels of aluminosilicates and carbonates against a low concentration of total sulphur in the ash samples guarantee an excellent potential for acid neutralisation [
56]. It should also be noted that total sulphur analysis does not necessarily indicate the amount of reactive sulphur.
Based on the static test results Sobek et al., classification, all the samples tested for daily, weekly, and monthly analysis were in the non-acid generating class [
17].
Figure 9(a) shows data collected from the 24-hour sampling, and it can be seen that the CFA sample from PSD showed the most non-acid-forming behaviour. From the elemental composition data presented in
Table 2, it can be seen that the total wt. % composition of the PSD (CFA) in terms of SiO
2, Al
2O
3, and Fe
2O
3 was the lowest, however the wt. % composition of the other metal oxides such as CaO, MgO, Na
2O, and K
2O were relatively high in the CFA samples. These metal oxides are responsible for the neutralising behaviour of coal ashes [
34]. The higher concentration of these oxides was able to mask the acid-generating behaviour induced by the presence of sulphur compounds in the ash. Another contributing factor is that during the oxidation of reactive sulphur and carbonate dissolution, iron oxy-hydroxides may precipitate at the surface of these sulphides and carbonates rendering them captive [
57]. On comparing the respective LCA samples, the same can be said about the neutralising behaviour of the PSA ash compared to that of the PSC ash. During the 3 sampling phases, the PSA ash exhibited better acid neutralising behaviour relative to the PSC ash. This again can be ascribed to the relatively higher wt. % of the oxides; CaO, MgO, Na
2O and K
2O.
Sample uniformity is also essential in minimising variations in chemical and physical behaviour. The elemental, mineral as well as particle size distribution of the CFA was mostly consistent in all the samples and the x-y scatter plot (NNP vs pH) in
Figure 9 (a), shows a high degree of clustering with the PSD (CFA) sample. On the contrary, there was noticeable dispersion in the LCA samples and this can be ascribed to the respective variations in elemental, mineralogical, morphology, and particle size distribution, in combination with the coal inhomogeneity. A summary of the NNP and pH of the PSC and PSA (LCA) samples is presented in
Table 7.