7.1. Calibration Results
The particle size data (
Table 1) clearly indicated that sinter fines had the largest average particle size (
Dav) and subsequently the lowest bed density. The ores had a much smaller
Dav, with the magnetite concentrate and the hematite ore having average diameters of 0.16 mm and 0.22 mm, respectively. Image analysis also showed the uniformity of the particles, with the magnetite concentrate having the most uniform particle size and the hematite ore the least, with a range in particle sizes from 0.067 mm to 8.63 mm. The variation in the size of the lump sinter (
Table 1) was due to the pseudo random process determined by the distribution of the bonding phase in the sintering process [
59]. From XRD analysis (
Tables S1 and S2), the phases present in the sinter and bed materials ranged from simple oxides such as hematite to more complex multi-element phases like SFCA. The heat capacity results for the lump sinter samples had a 3.5% deviation across the five samples, with an average value of 863.6, 892.1 and 919.9 J/kg K at 500, 550 and 600 °C, respectively (
Figure 5). Lai et al. [
50] calculated the heat capacity of sinter to be 860–980 J/kg K in the temperature range of 200–380 °C, whereas [
28] used a value of 920 J/kg·K and a sinter inlet temperature of 550 °C in their simulation, which is very similar to the 600 °C but deviates quite significantly from the 500 °C (
Figure 5).
Comparing the heat capacity of the bed materials (
Figure 6) at a standard temperature of 100 °C, the hematite–goethite ore was found to have the highest heat capacity, followed by the hematite ore, the sinter fines and the magnetite concentrate. The oxidation state of iron along with the bound water content had the largest impact on the heat capacity because of their increased interaction with infrared radiation compared to the gangue elements. Magnetite has a higher heat capacity than hematite, but the hydrogen bonding between the hydroxyl groups (FeOOH) in goethite increased its heat capacity (
Table 3).
The polar bonds contained within the bed materials vibrated, stretched and twisted when they absorbed infrared radiation (
Figure 7). Collected FTIR spectra showed peaks representing goethite, hematite, silicon and calcium oxides. The specific peak information is shown in
Table S3. Hydrated iron oxides contain a mixture of the polar O-H and Fe-O bonds [
60,
61,
62], resulting in a strong absorption, as shown in
Figure 7, whereas magnetite only contains Fe-O, reducing the absorption potential. As expected, the hematite–goethite ore had a higher absorption peak compared to the magnetite concentrate. The breaking of O-H and Ca-O bonds in the high-temperature sintering process reduces the absorption potential, but the formation of silico ferrites of calcium and aluminium has been shown to have a positive effect [
42], restoring the infrared absorption capability of sinter.
7.3. Temperature Results
The magnetite concentrate was an evenly distributed powder with a
Dav = 0.16 mm (
Table 1). At 500 °C, the magnetite concentrate reached an average peak temperature of 74 and 68 °C for the bottom and top layers at a rate of 0.13 and 0.17 °C/s, respectively (
Figure 9). The resultant cooling rate was 4.29 and 4.53 times lower than the heating rate for the bottom and top layers. Increasing the temperature to 550 °C increased the maximum temperature by only 7 °C for the bottom layer, but the top layer increased by 17 °C to 85 °C. The heating rate for both layers also increased, but the heating ratio (heating rate/cooling rate) increased for the bottom layer but decreased for the top layer. Lastly, at 600 °C, the peak temperature was 93 and 97 °C, and the heating ratio was 5.37 and 3.73.
The hematite ore,
Dav = 0.22 mm, was primarily made up of hematite, with small quantities of other elements (
Table 1). At 500 °C, the heating rate for the bottom and top layers was 0.09 °C/s, reaching peak temperatures of 72 and 83 °C (
Figure 9). Increasing the lump sample temperature to 550 °C resulted in peak temperatures rising to 77 and 91 °C. The resulting heating ratios for the bottom and top layers were 4.93 and 3.2. At 600 °C, the peak temperatures rose to 80 and 96 °C in the bottom and top layers. There was also an inversion in the heating ratio to 3.89 and 4.14.
The last ore, the hematite–goethite ore, was a mixture of hematite and goethite,
Dav = 0.27 mm (
Table 1). At 500 °C, it reached an average peak temperature of 63 and 64 °C for the bottom and top layers at a rate of 0.09 °C/s (
Figure 9). The resultant cooling rate was 2.16 and 2.40 times lower than the heating rate for the bottom and top layers. Increasing the temperature to 550 °C increased the maximum temperature by only 5 °C for the bottom layer, but the top layer increased by 28 °C to 92 °C. Lastly, at 600 °C, the peak temperature was 70 and 86 °C, and the heating ratio was 3.44 and 3.26.
The sinter fines were a complex mixture of iron oxides and SFCA structures, with the largest average particle size at 2.65 mm (
Table 1). At 500 °C, the heating rates were 0.09 and 0.06 °C/s, reaching peak temperatures of 66 and 83 °C (
Figure 9). Increasing the lump sample temperature to 550 °C resulted in peak temperatures rising to 73 and 93 °C. The resulting heating ratio for the bottom and top layers was 4.75 and 3.56. At 600 °C, the peak temperature rose to 74 and 104 °C in the bottom and top layers.
7.5. Heat Flow Tracking
Once in the reactor, the thermal energy was transferred from the lump sinter through the bed via radiation and conduction, forming a heat front that was analysed using image analysis from the thermal camera data. Mathematical models [
43,
63] have previously been used to predict the effect of different heat transfer modes on the effective thermal conductivity (ETC) of solid beds. The models predicted that an increase in particle size, and therefore voidage, would lead to a reduced effective thermal conductivity because of the low thermal conductivity of air, although the use of high-emissivity materials, such as iron oxide, could counteract this by means of an increased photon count moving through the voids (
Figure 1).
Radiation from a material is controlled by its emissivity, surface area and temperature, as described in the Stefan–Boltzman equation, Equation (9).
As emissivity and temperature increase, more energy is emitted as infrared radiation, with flux (
Q) increasing by the fourth power of absolute temperature. In
Figure 7, the polar bonds within the bed materials were identified using Fourier transform infrared spectroscopy: Fe-O, O-H, Ca-O and Si-O, whereas the air contained in the pores is 78% N
2, which is a poor absorber of infrared radiation. Conductive processes are controlled by the thermal conductivity (k), thermal diffusivity (D) and heat capacity (C
p). Thermal conductivity describes the rate of heat flow across a temperature gradient, where a high k can move heat quickly and a low k is a barrier to heat flow. Diffusivity describes the temperature change during conduction, where a high D shows that heat is dissipated and has a lower rate of temperature increase. Finally, a high heat capacity describes the energy input required to increase the temperature by one °C.
The bed materials have a thermal conductivity of 1.5–5.98 W/mK and thermal diffusivities of 2.2 × 10
−6–5.8 × 10
−6 m
2/s, whereas air has a thermal conductivity of 0.024 W/mK and a thermal diffusivity of 1.9 × 10
−5 m
2/s.
Figure 11 shows how energy moves from sinter, through a pore and into the bed material, taking into account the infrared and conductive properties of each material.
Figure 12 shows how energy is transferred through direct conduction from the lump sinter to the bed material; the thermal conductivity of both materials is similar, allowing temperature to flow quickly across the boundary. Preferential conduction through the bed materials causes conduction around pores, creating tendrils in the image analysis. The emissivity of the bed materials is also high (
Table 5), allowing the bed materials to radiate through pores and heat neighbouring bed materials. The difference in thermal properties of lump sinter, air and the bed materials show how isolated hotspots in the image analysis (
Figure 13) from the bed material heats faster than the air in the pore.
Figure 13 shows how the bed materials pack based on particle morphologies in the scanning electron microscope images (
Figure 2).
The maximum recorded temperature was found to correlate well with the heat capacity of the bed materials; a lower heat capacity resulted in faster conduction (
Figure S3). Numerical models predicted that an increase in voidage would result in a more resistive bed and therefore a lower heating rate, which was seen in both layers but to a lesser extent in the top. Because of the high emissivity of the bed materials (
Table 5), a high proportion of the heat could be transferred through radiation through a very porous bed.
Figure 14 shows the results of the image analysis of how the heat movement through the bed differed in each bed material. Panel A depicted the smooth flow of heat from the lump sinter through the top layer of the magnetite concentrate,
Dav = 0.16 mm. The steadily increasing distribution of the areas (
Figure 15) further indicated that heat was transferred smoothly through direct conduction. Additionally, the presence of very few heat spots due to the high bed density, 999.3 kg/m
3, leads to very few voids through which energy could be transferred by radiation. These image-based results correlate with the BET and SEM analysis (
Table 2 and
Figure 2), where beds with higher surface areas but moderate pore volumes (e.g., hematite–goethite) showed distributed and persistent heat fronts, while the sinter fines, with both high voidage and pore volume, exhibited delayed heat propagation and more fragmented thermal fronts. The magnetite concentrate had the highest thresholded area after 2 min, which correlates with its high thermal conductivity (
Table 4).
Conversely, bed materials the hematite ore and hematite–goethite ore had a slightly larger
Dav = 0.22 and 0.27 mm but a wider particle distribution, thus forming a less dense bed with a higher proportion of voids (
Figure 1). The thermal conductivity of the hematite ore was lower compared to the other ores, thus reducing the ratio of conduction to radiation. The images in panels B and C showed slower and more uneven heat flow, as pores impeded the energy flow and areas of small particles acted as conducting bridges to larger particles. This process is visualised in
Figure 15, where the hematite ore has a slower increase in area than the magnetite concentrate and an increased breaking of the heat front. The hematite–goethite ore had a high initial area that steadily decreased but recovered to a similar final area to the hematite ore. The decreasing area could be explained by an initial heating of the small particles, which then transferred to the wider bed. Lastly, the sinter fines,
Dav = 2.65,
ρ = 791.9 kg/m
3, had a very high proportion of voids within the bed (
Figure 1).
Figure 14 shows that individual particles in contact with the lump sinter increased in temperature via conduction before then radiating their energy through the pores, a large number of hot spots (
Figure 14), transferring energy from particle to particle while slowly heating the air increasing the total area and reducing the number of spots as the temperature becomes more homogeneous. The heating rate data (
Figure 9) shows that the magnetite concentrate had a consistently high heating rate, while the sinter fines had a consistently low value. The magnetite concentrates and the hematite ore varied throughout the tests due to the more inconsistent packing arrangements caused by the wider particle size distribution seen in the optical and SEM images (
Figure 1 and
Figure 2). For the most efficient heat transfer, a smaller particle size reduced pore volume and increased the contact area between the bed material and lump sinter, facilitating rapid conductive heat transfer. The BET and surface area (
Table 2) and pore volume data confirm these findings. Materials with higher surface area had a stronger interaction with radiative heat transfer because of higher IR-active surface exposure, but excessive pore volume introduced insulating voids, lowering conduction efficiency. For example, the hematite–goethite ore had a high surface area but moderate pore volume, balancing radiative absorption and conductive heat transfer. Analysing the 600 °C runs resulted in a similar heat flow pattern for each bed material with a faster rate, which correlates with the heating rate data.
Figures S4–S7 present the difference in the heat flow between the 550 °C runs and the 500 °C and 600 °C runs for the hematite ore and the hematite–goethite ore, respectively. As the temperature increased to 600 °C, the flow became more stable, showing fewer hotspots and a smoother increase in area over the first 2 min. While the increase in the quantity of biofuel being used to make the sinter had a negative effect on its heat capacity (
Figure 5), it was found that the rate limiting step was the absorption of energy by the bed material.
Figure S8 shows that the increase in the percentage of ecoke in the sinter mixture had little to no correlation with the average peak temperatures for all the bed materials, indicating that the choice of bed material had a greater impact. This further validates the use of hybrid biofuel as an effective sustainable replacement for coke breeze.
The area under the temperature curve (
Figure 16) was a secondary indicator of the effectiveness of the bed material at absorbing and, more importantly, retaining energy. The magnetite concentrate and the hematite–goethite ore were the most consistent at absorbing energy over the entire range of temperatures, whereas the hematite ore and the sinter fines fluctuated more because of their wider size distribution. In most cases, the top layer had a larger area due to the higher maximum temperatures reached because of the higher contact area with the lump sinter, although the slower cooling rate of the bottom layer increased the area reducing the difference. Overall, the hematite–goethite ore had the lowest area, and the hematite ore and the magnetite concentrate had the largest. In the energy balance, the heat capacity of both the sinter and the bed material were considered, meaning that the magnetite concentrate became much more like the sinter fines and the hematite ore to the hematite–goethite ore.
The high heat capacity of the hydrated goethite ore (
Figure 6) combined with the higher temperature efficiency of the magnetite concentrate (
Figure 10) would form an optimised chemistry for absorbing thermal energy. Image analysis identified the pores created by the wide size distribution of the goethite ore slowed the rate of heat transfer because of the reduced thermal conductivity of air. Therefore, the secondary addition of magnetite concentrate into a goethite bed would reduce the volume of insulating air within the bed, increasing the rate of heat transfer and overall efficiency. Together, the data show that the chemistry of the hematite–goethite ore, i.e., quantity of FeOOH, and the particle size distribution of the magnetite concentrate would, if combined, create a very effective bed material for absorbing excess thermal energy from iron ore sinter. The absorption of energy by the bed material before sintering will result in a lower quantity of energy required to melt the raw mixture, reducing the required fuel rate. Using the calorific content of the fuel mixture, measured by bomb calorimetry [
64], the theoretical percentage fuel saving for each bed material was calculated. Unsurprisingly, the hematite ore had the highest fuel saving, with 0.16 kg of fuel saved per 0.885 kg used in the sinter pot. Scaled up, this is a saving of 9.4 kg per tonne of fuel (
Figure S9). Despite having the lowest transfer efficiency, the sinter fines still had a potential saving of 1.1 kg/tonne. In comparison to moving grates and vertical tanks, this new method directly transfers heat into the sinter bed instead of using an intermediate transfer fluid, thus reducing the effect of transfer loss. During the experiment, cooling rates of 1.3–4.2 °C/min were achieved, which is the ideal range for efficient formation of SFCA [
18]. The most efficient bed material, the hematite–goethite ore, absorbed 2.36 kJ of energy over 328 s from 10 g of sinter. Scaled up to a rate of 9300 tonne/h of sinter, this results in a heat utilisation of 2.194 × 10
9 kJ/h. Studies on the moving grate style air cooled simulations by Zhang et al. [
65] had a waste heat utilization of 2.55 × 10
8 kJ/h, and simulations by Liu et al. [
28] were at 1.90 × 10
8 kJ/h. However, the vertical tank arrangement had a heat utilisation of 1.49 × 10
8 kJ/h [
37], showing little improvement compared to the moving grate process. Lastly, the solid–solid process model by Felinks et al. [
39] had predicted recoveries of 70% over multiple steps and 50% over two steps, similar to the efficiency data in
Figure 10. Based on a CO
2 emission factor of 2.86 kg CO
2/kg of coke, the projected fuel saving of 9.4 kg/tonne corresponds to ~27 kg CO
2 saved per tonne of sinter.