3.1. Optical Characteristics of Fe3O4, ATO and Fe3O4/ATO Hybrid Nanofluid
The optical properties of nanofluids are critical factors influencing their photothermal conversion efficiency.
Figure 4 presents the optical absorbance and transmittance spectra for 0.1 wt% Fe
3O
4, ATO, and Fe
3O
4/ATO nanofluids. As depicted in
Figure 4(a), Fe
3O
4 and ATO nanofluids exhibit distinct absorption characteristics within the wavelength range of 400 to 1200 nm. The ATO nanofluid shows a peak absorbance near 1100 nm, but overall, it demonstrates a lower optical absorbance compared to the Fe
3O
4 nanofluid. In contrast, the Fe
3O
4 nanofluid displays strong absorbance between 800 and 1100 nm, with a marked reduction in absorbance at wavelengths below 600 nm. This reduction can be attributed to the significant scattering reflection that occurs in the ultraviolet region for Fe
3O
4 nanofluids.
Figure 4(b) illustrates this scattering phenomenon, where the Fe
3O
4 nanofluid exhibits increased reflectance at wavelengths shorter than 600 nm, with reflectance intensity increasing as the wavelength decreases. On the other hand, the ATO nanofluid maintains a reflectance below 0.1 in the same wavelength range, indicating minimal scattering. These findings suggest that, although Fe
3O
4 nanofluids possess superior optical absorption properties, their high reflectance at shorter wavelengths can hinder their performance. Therefore, the combination of ATO and Fe
3O
4 in a hybrid nanofluid presents an opportunity to enhance overall optical absorption by leveraging the complementary properties of both materials.
Figure 5 shows the solar-weighted absorption coefficients of the Fe
3O
4/ATO hybrid nanofluids (NFs). For the Fe
3O
4 nanofluid, the solar-weighted absorption coefficient exhibited a modest increase from 0.854 to 0.883 as the optical path length increased from 0.01 m to 0.06 m. In comparison, the ATO nanofluid displayed a more pronounced increase, with the solar-weighted absorption coefficient rising from 0.529 to 0.876 over the same range. This indicates that, although the Fe
3O
4 nanofluid has superior optical absorbance, the improvement in photothermal conversion performance with increasing optical path length is limited due to scattering reflection.
The Fe3O4/ATO hybrid nanofluids demonstrated enhanced solar-weighted absorption coefficients relative to both Fe3O4 and ATO nanofluids. At an optical path length of 0.01 m, the solar-weighted absorption coefficient of the Fe3O4/ATO hybrid nanofluid (where =0.8) was 0.861, indicating a slight improvement over the coefficients of 0.854 for the 0.1 wt% Fe3O4 NF and 0.529 for the 0.1 wt% ATO NF. However, at an optical path length of 0.06 m, the solar-weighted absorption coefficient of the Fe3O4/ATO hybrid nanofluid (where =0.2) increased from 0.748 to 0.938. As the optical path length extended from 0.01 m to 0.06 m, the optimal for maximizing the solar-weighted absorption coefficient gradually decreased. These findings suggest that, with an increase in optical path length, enhancing optical absorbance and suppressing scattering reflection are crucial for the performance of Fe3O4/ATO hybrid nanofluids.
3.2. Photothermal Conversion Performance of Fe3O4/ATO Hybrid Nanofluid
The photothermal conversion performance of nanofluids is a critical parameter that directly influences the solar radiation harvesting efficiency of direct absorption solar collectors. This performance is affected by several factors, including the optical absorbance of the nanofluid, the fluid temperature, and the optical path length of the containment vessel.
Figure 6 presents the temperature variation of 0.1 wt% Fe
3O
4/ATO nanofluids over time under solar radiation exposure. The results indicate that the temperature of the 0.1 wt% Fe
3O
4/ATO nanofluids increases progressively with prolonged exposure to solar radiation, demonstrating the effective conversion and storage of solar energy into thermal energy. Over an exposure period of 9000 sec, the nanofluid with
=0.2 exhibited the highest temperature increase, reaching 12.2°C. In contrast, the nanofluid with
=0.6 showed the lowest temperature increase of 11.7°C, a result that is comparable to the temperature increase observed for the ATO nanofluid.
Figure 7 depicts the energy conversion efficiency of water and nanofluids (0.1 wt% Fe
3O
4 NF, 0.1 wt% ATO NF, and 0.1 wt% Fe
3O
4/ATO NFs) during solar exposure. The 0.1 wt% Fe
3O
4/ATO nanofluids exhibited photothermal conversion efficiencies that were either comparable to or greater than those of the 0.1 wt% Fe
3O
4 and 0.1 wt% ATO nanofluids. Among the mixtures, the Fe
3O
4/ATO hybrid nanofluid with
=0.2 achieved the highest collection efficiency, reaching 76.8%. As the solar exposure duration increased from 300 to 9000 sec, a decrease in collection efficiency and an increase in thermal losses were observed across all fluids, with nanofluids showing higher thermal losses compared to water. Notably, the Fe
3O
4/ATO hybrid nanofluid with
=0.2 not only enhanced collection efficiency but also reduced thermal losses. Its thermal loss rate increased from 13.2% to 64.7% as exposure time extended from 300 to 9000 seconds, which is lower than the thermal loss rates observed for the single-component nanofluids: 16.2–65.7% for the 0.1 wt% Fe
3O
4 nanofluid and 15–64.9% for the 0.1 wt% ATO nanofluid. However, increasing the proportion of Fe
3O
4 nanoparticles in the Fe
3O
4/ATO nanofluid led to a rise in thermal loss, indicating a potentially adverse effect. This behavior suggests that three-dimensional absorption of solar energy within the receiver contributed to a reduction in heat loss to the surroundings.
Figure 8 shows the temperature increase and local collection efficiency of the nanofluids after 9000 seconds of solar exposure. The temperature distribution within the receiver is primarily influenced by the solar energy absorption characteristics of the nanofluids. Both water and nanofluids exhibited higher energy storage in the upper section of the receiver, attributed to the concentration of absorbed thermal energy in this region. The average temperature increases and receiving efficiency for water were observed to be 8.16°C (
=10.3
,
=8.4
,
=7
) and 17.5% (
=7.02%,
=5.73%,
=4.77%), respectively. The single-component nanofluids, specifically 0.1 wt% Fe
3O
4 and 0.1 wt% ATO, demonstrated enhanced solar energy absorption capabilities compared to water, resulting in elevated temperature increases and receiving efficiencies. The 0.1 wt% Fe
3O
4 nanofluid achieved an average temperature increase of 11.8°C (
=15.8
,
=11.7
,
=9.1
) and a receiving efficiency of 25% (
=10.8%,
=8%,
=6.2%), indicating that the primary absorption of solar radiation occurred predominantly in the upper region. In contrast, the 0.1 wt% ATO nanofluid exhibited an average temperature increase of 11.7°C (
=15.1
,
=11.8
,
=9.5
) and a receiving efficiency of 24.82% (
=10.2%,
=8.05%,
=6.48%), demonstrating its capacity to absorb solar energy more evenly across the receiver, including the lower regions.
The 0.1 wt% Fe3O4/ATO hybrid nanofluid showed a further improvement in collection efficiency over the single-component nanofluids. Notably, the 0.1 wt% Fe3O4/ATO hybrid nanofluid with =0.2 recorded the highest performance, with an average temperature increase of 12.2°C (=16.5, =16.5, =13.4) and a receiving efficiency of 26.6% (=11.3%, =11.3%, =9.14%). This enhancement is attributed to the combined presence of Fe3O4 and ATO nanoparticles, which effectively broadens the solar energy absorption spectrum, thereby facilitating more efficient solar energy capture compared to single-component nanofluids. The 0.1 wt% Fe3O4/ATO hybrid nanofluid demonstrated superior solar energy absorption performance, particularly in the upper and middle sections of the receiver.
Interestingly, the Fe3O4/ATO hybrid nanofluid with =0.2, despite having a relatively lower absorption rate for solar energy at wavelengths above 800 nm, exhibited the most efficient photothermal conversion. This outcome is likely due to its lower reflectance at 400 nm and the optical path length of the receiver, which was adequate for optimal solar absorption. These results indicate that for the efficient performance of direct absorption solar collectors (DASCs), it is crucial to optimize both the optical properties of the nanofluids and the design parameters of the receiver
Figure 9 shows the photothermal conversion efficiency and the solar-weighted absorption coefficient of 0.1 wt% Fe
3O
4/ATO hybrid nanofluids as a function of
at an optical path length of 0.04 m. The photothermal conversion efficiency of the 0.1 wt% Fe
3O
4/ATO hybrid nanofluid reached its peak value of 0.932 at
=0.2. Beyond this ratio, a decline in photothermal conversion efficiency was observed. This trend is consistent with the behavior of the solar-weighted absorption coefficient, which also attained its maximum value of 0.918 at
=0.2 and subsequently decreased.
To enhance photothermal conversion performance using hybrid nanofluids, it is crucial to achieve a complementary interaction between the optical properties of the coexisting nanoparticles. While Fe3O4 nanofluids exhibit high scattering reflection in the ultraviolet and near-infrared regions, the coexistence of Fe3O4 and ATO nanoparticles in the base fluid reduces scattering reflection, thereby allowing for increased optical absorption and, consequently, higher photothermal conversion efficiency. Therefore, by carefully designing the of the hybrid nanofluid in consideration of the optical path length of the direct absorption solar collector, the optimal performance of the system can be achieved.