3.1. Sintering Process Parameters
The chemical composition of the sinter is shown in
Table 6.
Table 6 shows that the iron content of the sinter after sintering reached more than 50%, which meets the requirements of the ore used in the blast furnace.
Figure 2 depicts the sintering process parameters of acid, self-fluxing, and high-basicity PVTM sinters. The results show a large gap between them regarding the flame front speed. The flame front speed of a natural acid sinter (R = 0.33) is only 6.91 mm/min, the rate of an acid sinter (R = 0.50) jumps to 12.26 mm/min, the self-fluxing PVTM sinter (R = 1.10) is 14.44 mm/min, and the highest high-basicity PVTM sinter (R = 2.60) is 19.7 mm/min. This may be attributed to the permeability of the sintering mixture caused by the gaps in the granulation. The PVTM ore has a coarse granularity, a small surface area (shown in
Figure 3), and a poor pelletizing property. The quicklime was slaked into the hydrated lime Ca(OH)
2 where it came in contact with the sinter mixture mixing and the granulation stage. The granulation was improved by the bonding effect of Ca(OH)
2 [
17,
18]. The temperature of the sinter mixture was increased by the exothermic reactions of hydration, which can ease moisture condensation in the bottom layer of the sinter bed. This decreases the resistance in sintering and improves the permeability. Thus, the more quicklime added, the faster the rate becomes. The weight loss with the high-basicity PVTM sinter was the largest at 15.05%. This is probably due to the highest basicity adjustment by the quicklime. This suggests that as more quicklime is added, the larger the weight loss becomes.
The differences between acid, self-fluxing, and high-basicity PVTM sinters in yields >5 mm are seen in
Figure 2. The yield of the acid PVTM sinter (R = 0.50) was the highest (83.1%), and the second highest was the self-fluxing sinter (R = 1.10) with a value of 82.90%. The high-basicity sinter had the lowest value at 78.02%. This might be caused by the acid sinter becoming bonded with the silicate, which needs a large mount of heat to form the liquid phase, while the coke content is constant and the heat released by the 3.2% coke combustion is not enough to provide a sufficient liquid phase in the natural acid sinter (R = 0.33). Thus, the yield is lower than that in the acid sinter (R = 0.50). Moreover, the bigger weight loss may cause more pores in the self-fluxing PVTM sinter, which would reduce the yield. Besides, the high-basicity PVTM sinter is mainly bonded by silico-ferrite of calcium and aluminum (SFCA) but, due to the precipitation of perovskite (CaO·TiO
2) and the biggest weight loss, the yield (>5 mm) is the lowest.
Figure 2 depicts the productivity of the PVTM sinters. The flame front speed of the natural acid sinter (R = 0.33) was the lowest, it had the longest t, and a lower y (
Figure 2). Therefore, the natural acid had the lowest P (0.481 t/(m
2·h)). The flame front speed for the acid sinter (R = 0.50) had a large rise, followed by a large decrease in t, and had the highest y. The acid sinter increased the
P to 0.883 (t/(m
2·h)). The P had a further increase in the self-fluxing PVTM sinter because the flame front speed further increased while the sintering time had almost no decline. The high-basicity PVTM sinter had the highest
P, the fastest flame front speed, and the smallest t. Additionally, the lowest y had little effect on the final result, as it was slightly smaller than that in the acid or the self-fluxing PVTM sinters.
3.3. Microstructure and Mineralogy
The microstructures of acid (R = 0.33; R = 0.50), self-fluxing (R = 1.10), and high-basicity (R = 2.60) PVTM sinters are shown in
Figure 5. The magnetite and hematite of the vanadium and the titanium sinters were different from the ordinary sinter. The magnetite was a magnetite–ferrotitanium solid solution. The hematite was a titanium–ilmenite solid solution. The mineral content of acid (R = 0.33; R = 0.50), self-fluxing (R = 1.10) and high-basicity (R = 2.60) PVTM sinters is shown in
Figure 6.
The main minerals in the acid PVTM sinter were magnetite, hematite, silicate, and pseudobrookite. Approximately 70% of the magnetite in the raw material was oxidized to the hematite. The hematite and the magnetite were mostly self-shaped or semi-self-shaped zonal crystals, where the crystal was the main bond between the natural basicity PVTM sinter. The silicates were primarily olivine and vitreous that formed a smooth and uniform spongy structure. The microstructure of the acid (R = 0.33, 0.50) PVTM sinters was dense and uniform (
Figure 5a,b). There was a small amount in the form of magnetite bonded by silicate that was confirmed by EDS (
Figure 7). The structure of the sinter was compact with good intensity. The flame front speed was low due to the time required to oxidize the large amount of magnetite.
The primary minerals found in the self-fluxing PVTM sinter were magnetite, hematite, silicate, pseudobrookite, titanium eclogite, perovskite, and SFCA. The crystal effect of the hematite and magnetite were weakened, as most of their particles were filled and cemented during the silicate phase. Small amounts of SFCA and perovskite appeared in the sinter. The calcium iron ore was dispersed between the magnetite and hematite granules in a granular or dendrite form during the sintering process, which weakened the interaction between the two (
Figure 5c). The main bonding mode of the self-fluxing PVTM sinter was a silicate bond.
The primary minerals in the high-basicity PVTM sinter were magnetite, hematite, silicate, perovskite, and SFCA (
Figure 5d). The content of the magnetite, SFCA, and perovskite was increased in the sinter, and the content of the hematite was decreased. The silicates were primarily dicalcium silicate, and olivine. The high-basicity (R = 2.60) PVTM sinter was mostly bonded by SFCA to form a molten microstructure (
Figure 8). A small amount of secondary hematite appeared, where there was also a bit of dicalcium silicate, fayalite, and perovskite precipitation around the SFCA. The distribution of the silicate liquid phase in the sinter was unevenly distributed, and the sinter formed an inhomogeneous porous, thin-walled structure due to the increase in perovskite. This affected the intensity of the sinter, although the silicate liquid phase was not obviously increased.
To further explore the impact of the basicity on the mineral composition, a thermodynamics analysis on the reaction of the CaO and some oxides (Fe
2O
3, SiO
2, TiO
2) was conducted [
19]. The CaO mainly had the following reactions during the sintering process (
Figure 9a),
The order of the thermodynamic trend for the formation of the new minerals shown by the reaction between CaO and the above oxides was: 2CaO·SiO2; 3CaO·SiO2; CaO·TiO2; 2CaO·Fe2O3; 2CaO·Fe2O. During the actual sintering process of the PVTM magnetite concentrate, there was a large contact area between the CaO and the iron oxide due to the SiO2. There were good dynamic conditions for the reaction, and it was beneficial in the formation of SFCA and the formation of the liquid phase. Perovskite was more likely to form than SFCA, which was confirmed by the experimental results of the relationship between the mineral composition and the basicity. To ensure the formation of SFCA when producing a high-basicity sinter, perovskite production must be suppressed. This can be accomplished by reducing the content of TiO2 in the concentrate.
Perovskite can be formed in many ways. The thermodynamic analysis showed that CaO-TiO
2, CaO-FeO·TiO
2, CaO-2FeO·TiO
2, CaO·Fe
2O
3-TiO
2, CaO·Fe
2O
3-FeO·TiO
2, CaO·Fe
2O
3-2FeO·TiO
2 could produce perovskite (
Figure 9b). During the actual process, the formation of perovskite is determined by the dynamic conditions of the reaction. The above reactions can be classified as solid–solid and liquid–solid reactions, and a liquid–liquid reaction also was possible. Although perovskite can be formed through the solid–solid reaction, the speed is very slow. Occurring at high temperatures (1320–1420 °C), the solid–phase reaction between CaO and TiO
2 was accelerated, and perovskite was formed in the sinter. During the cooling process, the perovskite phase first precipitated, which differed from the perovskite generated in a solid-phase reaction. TiO
2 existed primarily in FeO·TiO
2 and 2FeO·TiO
2 from within the PVTM magnetite concentrate. Their melting points were 1360 °C. and 1470 °C. CaO could react with Fe
2O
3 to form SFCA at a low melting point, so it was possible to have a liquid–solid reaction (reactions (8) and (9)) and a liquid–liquid reaction (reactions (15) and (16)). This generated perovskite with a high stability and a high melting point that precipitated from the liquid phase. The calcium ferric decomposed and was restored where more CaO and TiO
2 minerals were used to generate perovskite when the temperatures were high, and the atmosphere was reduced. This suggests that if sintering with a low-temperature oxidation, the formation of perovskite could be reduced and the formation of SFCA could be enhanced to improve the sintering properties by increasing basicity.
3.4. Metallurgical Performance
Figure 10 illustrates the metallurgical performances of the acid, self-fluxing, and high-basicity PVTM sinters. The acid sinter was dependent on the bonding of the silicate, and the natural acid PVTM sinter (R = 0.33) had the lowest TI (62.93%). The bonding of the self-fluxing sinter was different from that of the acid sinter, where the uneven distribution of liquid arose from poor granulation. The acid PVTM sinter (R = 0.50) had the highest TI (63.69%), due to the uniform microstructure, the sufficient liquid, and lack of perovskite. The self-fluxing PVTM sinter had the lowest TI (60.91%). This may have been caused by the inhomogeneous microstructure, where additional glass and pores occurred as the flame front speed increased with insufficient liquid crystallization. Although no SFCA was present, perovskite would result in the lowered TI. The high-basicity PVTM sinter had a higher TI (63.51%), because it was bonded by SFCA, which had a high strength. The TI had a slightly smaller value than the acid PVTM sinter (R = 0.50), due to the amount of precipitation by the perovskite.
The RDI
+3.15 of acid was R = 0.33, 0.50 with a high-basicity of R = 2.60. The PVTM sinter was higher than 70%, which meets the requirements for a BF, except the self-fluxing RDI
+3.15 that had a value of 50.81%. The acid PVTM sinter had a high RDI
+3.15 value. This may be attributed to the bonding phases, which were primarily silicate as fayalite with a high FeO. A 1% increase in FeO improved the RDI by 4 points [
20]. There was little hematite present, which was the main reason the sinter had a reduced degradation during the phase transformation of Fe
2O
3 → Fe
3O
4. This was associated with a volume increase of 10%, which led to degeneration during the reduction process at 450–500 °C [
12,
21,
22]. Another cause for the high RDI
+3.15 value could be the uniform microstructure, sufficient liquid, few pores, and lack of perovskite. Additional pores appeared when the maximum weight loss was achieved, the secondary hematite from SFCA decomposed, and the phase transformation of dicalcium silicate (C
2S) (β-C
2S → γ-C
2S) occurred. These factors combined to cause the RDI
+3.15 value to be lower than the acid PVTM sinter, even though it was bonded by a high strength SFCA. The self-fluxing PVTM sinter had the lowest RDI
+3.15 value, which was likely due to the uneven bonding phase, the presence of perovskite, the pores, and the lack of a high-strength SFCA. Additionally,
Figure 11 shows that the vanadium and titanium sintered ore had a good reduction performance and, with the soda ore basicity increased, its reduction performance improved.
Figure 11a shows the softening start temperature (T
10), softening temperature (T
40), and softening zone (T
40–T
10) of the acid, self-fluxing, and high-basicity PVTM sinters. The results show that T
40 and T
10 are also on the rise with the increase in the basicity of the sinter. The reason is the iron olivine is gradually converted to calcic olivine, and the softening temperature of the sinter is promoted. Accompanying the increase in the basicity, hematite, magnetite, and calcium ferrite restore faster, so it causes the speed of the softening temperature to increase faster. The softening zones of the self-fluxing sinter and high-basicity sinter (T
40–T
10) are obviously showing a narrowing trend.
Figure 11b shows the melting start temperature (T
S), melting-dripping end temperature (T
D), and melting-dripping zone (T
D–T
S) of acid, self-melting, and high-basicity PVTM sinters. The T
S value of the acid sinter is low, and the content of the T
D is high, which leads to the widest point of (T
D–T
S). This is due to the higher content of SiO
2 compared to the content of CaO. During the reduction process it mainly forms low melting materials such as iron silicate, and the acid slag that it produces has a high viscosity, and poor liquidity, which causes the slag iron only to drop off in high temperatures, leading (T
D–T
S) to increase. The Ts of the melting sinter is increased, mainly because the reduction degree rises with the additional basicity, and the FeO in the slag decreases accordingly, causing the melting point of the slag to rise, and the (T
D–T
S) to narrow. Regarding a high basicity sinter, when the ratio of the alkaline oxide in the slag and acid oxides is more than that in the silicate, to continue to improve the CaO in the molten pool with the temperature not high enough, it cannot melt or separate as a solid precipitation of compounds (2CaO·SiO
2) with a high melting point. Additionally, it increases the viscosity of the molten slag, which is not conducive to drip, so there is a trend for (T
D–T
S) to widen.
Figure 11c is the softening–melting zone of the acid, self-fluxing, and high-basicity PVTM sinters. Acid sinter, due to the low softening start temperature, will form the slag earlier with a higher distilling temperature, which causes a wider softening–melting zone; therefore, it will cause a bad blast furnace permeability, impeding gas from flowing through smoothly, and is unfavorable to burden descent. While the basicity of the self-fluxing sinter increases, the sinter softening start temperature begins to increase, and the softening-melting zone starts to decrease in a good trend but, in a basicity of 2.6, the sinter’s dripping start temperature is too high, which is not conducive to the operation of the blast furnace.
Figure 12 shows the gas permeability index of acid, self-fluxing, and high-basicity PVTM sinters. The gas permeability index, namely the S value, was calculated according to the parameters during reduction and smelting with the equation
, which is referred to in previous studies [
23]. ∆Ps is the external static load when the temperature reaches the melting start temperature and ∆P is the external static load at a different time.
Figure 12 shows that the Sn value of the acid sinter and the high-basicity sinter is larger, and the characteristic value of the self-fluxing sinter is the lowest. The acid sinter and high-basicity sinter do not have good permeability, and they are not good to be used in the operation of the blast furnace due to their high characteristic values.
3.5. Comprehensive Index
Acid, self-fluxing, and high-basicity PVTM sinters are evaluated by the comprehensive index method, and the higher comprehensive index value calculated, the better are the PVTM sinter performances being evaluated. Here, the comprehensive index method is the same as the method in reference [
12], and the chosen indexes and the significance coefficient is the same as that in PANGGANG; the indexes chosen are productivity, TI, and RDI
+3.15. The total significance coefficient is 100, and the significance coefficients of the productivity, TI, and RDI
+3.15 levels are 40, 30, and 30, respectively.
The method is as follows. To facilitate the comparison and analysis, the comprehensive index of the (R = 0.33, chosen as the better fit) first group is set as a reference and quantified to 100.
Defining:
where
Fi is the comprehensive index,
fi is the composite index, and
F1 = 100 (
Fi =
fi −
f1 + 100)
where
ωj is the unit range coefficient, and
fi ≥ 0 (
i = 1,2,…,
n)
where
Wj is the significance coefficient and
and
Rj are the range.
where z
i1 is the productivity, z
i2 is the TI, and z
i3 is the RDI
+3.15.
The calculation process and the results of the comprehensive index are shown in
Table 7.
Table 7 shows the self-fluxing PVTM sinter performance is the worst, then the natural acid PVTM sinter (R = 0.33). The high-basicity PVTM sinter performance is the best, with the highest comprehensive index value, then the acid PVTM sinter (R = 0.50). The burden structural model of the blast furnace smelting a vanadium and titanium burden should adopt a ‘high-basicity PVTM sinter + acid V-Ti pellet’, and when the production capacity of the acid pellet is short, an acid PVTM sinter (R = 0.50) could be produced using a surplus sinter plant to replace a part of the acid pellet added to the blast furnace. The novel burden structural model was a ‘high-basicity PVTM sinter (R = 2.60) + acid V-Ti pellet + acid V-Ti sinter (R = 0.50)’ used in a BF smelting V-Ti burden, which will require further research into the softening–melting behaviors as it is used in the blast furnace.