Assessment of Antarctic SIC products based on MODIS data
Through the preprocessing of 36 MODIS images and the inversion of SIC, the data albedo, ice-water binarization map, and MODIS 25km\(\:\times\:\)25km spatial resolution SIC were obtained. By comparing the bias, mean absolute deviation (MAD), root mean square deviation (RMSD), and correlation coefficient (R) (see Table 1) between the SIC inverted from MODIS and the SIC products released by various organizations, the consistency between different SIC products and high-resolution optical remote sensing data-derived SIC was verified and analyzed. AMSR2/NT2, SSMIS/CDR, and MWRI/NT2 show high correlation coefficients with the verification data SIC, at 0.92, 0.91, and 0.94, respectively.
The bias analysis indicates that the bias of MWRI/NT2 is the smallest, at just 0.23%, while the bias of SSMIS/NT is the largest, at -9.63%. Because the NT algorithm has a low recognition capacity for new ice and melt ponds, there is a significant bias compared to the SIC inverted from MODIS.
The analysis of MAD and RMSD shows that the MAD and RMSD of SSMIS/NT are the largest, at 11.20% and 15.35%, respectively, while those of MWRI/NT2 are the smallest, at 3.68% and 9.52%.
In summary, MWRI/NT2 has the highest correlation coefficient, the lowest MAD, and the lowest RMSD among the six SIC products, achieving the highest consistency with the SIC inverted from MODIS. Therefore, the MWRI/NT2 SIC product was used for subsequent research analysis. The NT2 algorithm reduces the effect of sea ice surface changes using the polarization ratio, making it more effective than the NT algorithm. The MWRI/NT2 product can detect finer-scale SIC changes than the 25km\(\:\times\:\)25km spatial resolution SIC products. The influencing factors include variations in sensors used for obtaining brightness temperature data, differences in satellite observation times, algorithmic differences, variations in spatial resolution, differences in post-processing methods, and sensitivity to climate and environmental factors.
Table 1
Bias, MAD, RMSD and correlation coefficients between six sic products and the SIC of MODIS.
Products | Bias | MAD | RMSD | R |
SSMIS/NT | -9.63 | 11.20 | 15.35 | 0.66 |
SSMIS/BT | -2.85 | 6.36 | 14.68 | 0.86 |
SSMIS/CDR | -1.64 | 5.10 | 11.53 | 0.91 |
AMSR2/NT2 | 1.84 | 3.69 | 10.75 | 0.92 |
AMSR2/ASI | -7.02 | 8.68 | 15.41 | 0.88 |
MWRI/NT2 | 0.23 | 3.68 | 9.52 | 0.94 |
Seasonal sea ice changes
Summer changes
Over the past 13 years, the summer SIC in the Weddell Sea has shown an overall decreasing trend, with a decline rate of -8.9 ± 2.1×103km2yr−1 (Table A8). A strong inverse relationship exists between SST and SIC (r=-0.62, p < 0.01) (Table A9), which leads to a reduce of SIC with high SST (Fig. 1(a) and (b)). Due to the substantial increase in SST north of 70°S and the decrease south of 70°S (eastern Antarctic Peninsula), both thermal and pressure differences between low and high latitudes have resulted in the strengthening of the westerly belt33,34. As shown in Fig. 1(c), the wind speed and zonal wind between 60°S and 70°S significantly increase, indicating the strengthening of the westerlies. The intensification of the westerlies promotes the northward transport of colder surface waters through Ekman transport. This phenomenon leads to Ekman suction, enhancing the mid-layer water transport from mid-latitudes to high latitudes. Furthermore, a weakening of the westerlies leads to a reduction in the Weddell Gyre circulation, which in turn causes an upwelling of the thermocline, resulting in an increase in surface water temperatures and a subsequent reduction in sea ice33. Additionally, correlation analysis results demonstrate that both wind speed and zonal wind have an inverse relationship with SIC (zonal wind: r=-0.42, p < 0.05; wind speed: r=-0.62, p < 0.01) (Table A9). Changes in wind speed can affect the intensity of sea ice advection, which subsequently influences both increase and decrease of sea ice. As shown in Fig. 1(d), wind speed increases between 60°S and 70°S, promotes sea ice advection towards the northeastern Weddell Sea and reduces the SIC. Therefore, both SST and wind speed have a significant inverse relationship with SIC, which together affect the changes of sea ice during summer24.
Autumn changes
In autumn, the SIC in the northern and northeastern regions of the Weddell Sea decreases significantly, with a decline rate of -10.7 ± 2.3×103km2 year-1 (Table A8), marking it as the season with the most severe sea ice loss in the Weddell Sea. There is an inverse relationship between the trend in SST and SIC, indicated by a correlation of -0.66 (p < 0.01) (Table A9, Fig. 2(a) and (b)). The westerly winds strengthen in the northwestern and northeastern Weddell Sea (Fig. 2(c)). Correlation analysis shows that in autumn, there is a strong negative relationship between both wind speed and zonal wind and the SIC (zonal wind: r=-0.60, p < 0.01; wind speed: r=-0.77, p < 0.01) (Table A9). (1) Northwestern region: This intensified circulation causes the thermocline to rise, subsequently leading to the northward migration of warm water into the Weddell Sea. Additionally, the enhanced Ekman transport increases the movement of cold surface water from high to low latitudes, triggering the Ekman suction phenomenon, which facilitates the influx of warm low-latitude water into the Weddell Sea. The rise in wind speed enhances the movement of sea ice, leading to its northwestward drift. These three factors collectively promote the melting of sea ice. (2) Northeastern region: In the northeastern Weddell Sea, changes in the wind speed and zonal wind are minimal24. A decrease in both the wind speed and zonal wind is observed in some areas, where sea ice experience loss (Fig. 2(c) and (d)). Therefore, we divided the Weddell Sea at the − 20°W meridian into eastern and western sections and separately analyzed the correlations of the SIC with the SST, wind speed and zonal wind. The results show that in the eastern Weddell Sea, the SST, wind speed and zonal wind all exhibit an inverse relationship with the SIC (Eastern SST: r = -0.62, p < 0.01; Eastern zonal wind: r = -0.70, p < 0.01; Eastern wind speed: r = -0.77, p < 0.01). In the western Weddell Sea, the correlation coefficients of the SIC with the SST, wind speed and zonal wind are − 0.68, -0.39 and − 0.40, respectively (Table A9). Therefore, in the northeastern Weddell Sea, the primary cause of changes in SIC is variations in SST, while the impacts of the wind speed and zonal wind on SIC are minor.
In summary, in the northwestern Weddell Sea during the autumn, the reduction in the SIC is primarily due to rising SST and the intensification of zonal and meridional winds. In the northeastern Weddell Sea, the dominant factor influencing the decrease in the SIC is the SST.
Winter changes
In winter, the trend in SIC changes in the Weddell Sea is minimal, with a notable reduction primarily near 60°S, especially at the northern tip of the Antarctic Peninsula (Fig. 3(a)). The rate of sea ice loss is -1.3 ± 0.5×103km2yr−1 (Table A8). Similar to autumn, the correlation between the SIC and SST, wind speed and zonal wind is different in the eastern and western Weddell Sea. (1) In the northwestern Weddell Sea, at the northern tip of the Antarctic Peninsula, the correlation coefficients between the SIC and the SST, zonal wind, and wind speed are − 0.57, -0.35, and − 0.53, respectively (Table A9). The correlation analysis results indicate that as the trend in changes in the SIC weakens, the correlation also diminishes. The findings from the correlation analysis suggest indicate that changes in the SIC are primarily influenced by variations in sea surface temperature and wind speed. The strengthening of westerly and northwesterly winds in this region (Fig. 3(c) and (d)) enhances both sea ice advection and Ekman suction. This, in turn, facilitates the influx of warm water from lower latitudes. As a result of this warm water intrusion, sea surface temperatures at the northern tip of the Antarctic Peninsula exhibit an upward trend (Fig. 3(b)). Consequently, the SIC at the northern tip of the Antarctic Peninsula significantly decreases. (2) In the northeastern Weddell Sea, SST has a strong negative correlation with SIC, as shown by a correlation coefficient of -0.71 (p < 0.01) (Table A9), and shows no significant correlation with the wind speed and zonal wind. Therefore, the decrease in the SIC in this region is primarily due to the increase in SST.
Spring changes
During spring, SIC in most areas of the Weddell Sea shows a declining trend, with the northwest experiencing the most pronounced decrease. The rate of sea ice decline is -6.2 ± 1.9×10³ km²yr⁻¹ (Table A8) (Fig. 4(a)). The SIC displays strong negative correlations with the SST, wind speed, and zonal wind, exhibiting correlation coefficients of -0.65, -0.71, and − 0.74, respectively (Table A9). The SST shows an upward trend in the northern Weddell Sea (Fig. 4(b)), resulting in higher seawater temperatures and hastening the dissolution of sea ice. During spring, the strengthening of westerly winds (Fig. 4(c)) enhances Ekman transport, which drives the movement of colder polar surface water toward lower latitudes. This intensified Ekman transport also increases Ekman suction, leading to the influx of warm water into the Weddell Sea. Additionally, the strengthening of westerly winds contribute to the intensification of the Weddell Gyre, which in turn promotes increased vertical mixing and the upward movement of warmer water from the thermocline35. The declining trend in SIC in the eastern Weddell Sea is driven by the substantial strengthening of westerly and northwesterly winds, which promotes sea ice advection and causes the ice to drift eastward (Fig. 4 (c) and (d)). The pronounced declining trend in SIC at the northern tip of the Antarctic Peninsula is caused by intensified sea ice advection, a result of the increased wind speeds due to westerly winds from the Bellingshausen Sea being blocked by the Antarctic Peninsula. This phenomenon is also observed in the summer, autumn and winter. The SST along the eastern flank of the Antarctic Peninsula is showing a declining trend, while the western side exhibits an increasing trend. The Antarctic Peninsula acts as a barrier, preventing the transfer of temperature and wind between its eastern and western sides1,36. As can be seen from Fig. 4, as the SST in the west of the Antarctic Peninsula increases, the SIC decreases significantly. Due to the Antarctic Peninsula's resistance to heat transfer, the SST in the east of Antarctic Peninsula changes very little, resulting in almost no change in SIC24.
Long-term sea ice changes
From 2011 through 2023, the SIE in the Weddell Sea exhibited significant seasonal variations and interannual fluctuations. In 2014, the SIE reached its maximum extent of 4.08×106km2, declining to its minimum extent of 3.17×106km2 by 2023 (Fig. 5). Overall, the SIE shows a decreasing pattern, characterized by an average yearly reduction rate of -6.6 ± 1.3×103 km²yr− 1 (Table A8).
Seasonal analysis indicates that the most significant declining trend occurs in autumn, with a rate of -10.7 ± 2.3×10³ km² yr⁻¹, while the smallest decline is observed in winter, at -1.3 ± 0.5×10³ km² yr⁻¹ (Table A8). According to statistical analysis, there is a significant negative correlation between SIE and SST across seasons (r=-0.81, p < 0.01) (Table A2), with the negative correlation occurring in summer (r=-0.89, p < 0.01) (Table A3). Changes in SST are the primary factors affecting the expansion and retreat of sea ice37. The largest SIE in 2014 corresponded to the lowest SST of -0.21°C, while the smallest SIE in 2023 corresponded to the highest SST of 0.25°C (Fig. 6). This finding is consistent with existing research, which indicates that increases in SIE correspond with decreases in SST38.
The NHF represents the net exchange of heat between a system, such as the ocean, and its surrounding environment. A positive NHF indeed means that the ocean is losing heat to the atmosphere. Conversely, a negative NHF indicates that the ocean is gaining heat from the atmosphere. The NHF is crucial for driving atmospheric circulation, affecting ocean temperatures and influencing the formation and melting of sea ice. Statistical analysis reveals that the relationship between the NHF and SIE varies by season. In spring and summer, a substantial positive relationship is observed between NHF and SIE, with correlations of r = 0.72 (p < 0.01) for spring and r = 0.3 (p < 0.1) for summer. Conversely, in autumn and winter, the relationship becomes negative, with correlations of r=-0.65 (p < 0.01) for autumn and r=-0.52 (p < 0.01) for winter (Tables A3-A6, Fig. 6).
Over the past 13 years, the sea ice cover in the Weddell Sea has undergone significant changes, which are closely related to the continuing ocean-atmosphere interactions. To deepen the understanding of these processes, a correlation analysis was conducted on Weddell Sea sea ice with various climate variability patterns (Fig. 5, Table A2). The SAM refers to the climate variations caused by the northward or southward shifts of the westerly wind belt or low-pressure systems surrounding Antarctica39,40, directly reflecting variations in the atmospheric pressure patterns around Antarctica. It significantly influences the SST and the strength of the westerly winds in the Weddell Sea. Although annually there is no significant correlation between the SIE and the SAM, seasonally, the SIE correlates positively with the SAM in summer (r = 0.29, p < 0.1), and negatively in winter (r=-0.28, p < 0.1) (Tables A2-A6, Fig. 6). The expansion and contraction of sea ice are driven by the positive phase of the SAM, which leads to changes in the westerlies and alters the pressure differences between the Antarctic low pressure belt and the subtropical high pressure belt34,41,42.
The IOD is associated with variations in the differences between the SST and sub-surface ocean temperatures in the eastern and western regions of the Indian Ocean. The IOD demonstrates significant negative correlations with the SIE during summer (r=-0.62, p < 0.01) and autumn (r=-0.33, p < 0.1), and a significant positive correlation in spring (r = 0.31, p < 0.1) (Tables A2-A6, Fig. 6). This may be attributed to the proximity of the Indian Ocean to the eastern Weddell Sea, where changes in the SST of the western Indian Ocean and variations in the IOD facilitate changes in the Southern Hemisphere westerlies, easily influencing sea ice changes in the eastern Weddell Sea. The results of this study indicate that there is no significant correlation between the ENSO and AMM with SIE throughout the year (Tables A2-A6, Fig. 6).
High sea ice minus low sea ice
In order to investigate how ocean-atmosphere heat exchange influences sea ice changes, we conducted a principal component analysis on the SIE. Based on the results, years with a standard deviation greater than 1 were classified as high sea ice years, while those with a standard deviation less than − 1 were defined as low sea ice years (Table A1). We determined the mean values for the SIC, NHF, and SST during periods of high and low sea ice, and derived a composite difference by subtracting the average values of low ice years from those of high ice years. Using this composite difference, we investigated the composite variation patterns of the SIC, NHF and SST (Fig. 7).
In summer, the positive anomalies in the SIC were observed in the Weddell Sea, particularly along the western and eastern coastal areas. At the same time, most regions experienced the positive anomalies in the NHF and negative anomalies in the SST (Fig. 7(a), (b) and (c)). Correlation analysis shows that in summer, the SIC is positively correlated with the NHF, with a coefficient of 0.30 (p < 0.1), and negatively correlated with the SST, with a coefficient of -0.32 (p < 0.1) (Table A3). Consequently, the positive NHF anomalies and negative SST anomalies that occur in summer collectively promote the formation of sea ice.
In autumn, the positive SIC anomalies in the mid-sections of the Weddell Sea are accompanied predominantly by the negative NHF anomalies (Fig. 7(d) and (e)). This could result from the heat gathered over the summer dissipating into the atmosphere during the autumn43. The SST predominantly exhibits negative anomalies (Fig. 7(f)). Consequently, the increase in the SIC during autumn is associated with the combined effects of NHF (correlation coefficient of -0.65, p < 0.01) and SST (correlation coefficient of -0.71, p < 0.01). (Fig. 7(d)–(f) and Table A4).
In winter, the significant positive anomalies in the SIC occur near 60°S in the northern sector of the Weddell Sea, while both the NHF and SST exhibit negative anomalies in the same area (Fig. 7(h) and (i)). In winter, positive anomalies in SIC are linked to negative anomalies in NHF, with a correlation of -0.51 (p < 0.01), and SST, with a correlation of -0.71 (p < 0.01) (Table A5).
In spring, the positive SIC anomalies persist across most areas of the Weddell Sea (Fig. 7(h)). The positive NHF anomalies dominate in most regions south of 60°S, while the SST primarily exhibits negative anomalies (Fig. 7(k) and (l)). This indicates that the rise in sea ice correlates with positive anomalies in NHF and negative anomalies in SST, respectively. In spring, the SIC anomalies shows a strong positive correlation with the NHF anomalies (r = 0.71, p < 0.01) and a strong negative correlation with the SST anomalies (r=-0.70, p < 0.01) (Table A6).
Correlation analysis between the NHF and SST shows that their relationship varies with the seasons. During summer and spring, the NHF and SST exhibit significant negative correlations, with coefficients of -0.32 (p < 0.1) and − 0.90 (p < 0.01), respectively. This may be due to the higher solar radiation in these seasons, which enhances the release of the LH and sensible heat flux (SH), thereby increasing NHF from the ocean to the atmosphere during years with high sea ice. During autumn and winter, NHF and SST exhibit significant positive correlations, with coefficients of 0.62 (p < 0.01) and 0.29 (p < 0.1), respectively (Tables A3-A6). In summer and autumn, the SST decreases significantly, while the decrease is less pronounced in winter and spring. This may be attributed to the reduced solar radiation received by the Weddell Sea in winter and spring, leading to increased upward radiation from open seawaters in subsequent seasons44. Consequently, the relationships and variations between the NHF and SST are not constant but may change over time and with the seasons.
Spatial and Temporal Analysis of Environmental Factors Influencing SIC
The GTWR accounts for spatial and temporal heterogeneity in modeling, allowing various environmental factors to have unique impacts on SIC at different geographic locations and time points31,32. Initially, correlation analysis and multicollinearity tests were conducted to screen the environmental factors, including 10m zonal wind, 10m meridional wind, 10m wind speed, mean sea-level pressure (MSL), SST, LH, SH, and NR flux (NR), derived from the ERA5 reanalysis dataset. The results of the correlation analysis indicate a high degree of correlation between SST and other environmental factors, particularly with MSL and LH (Table A7). The results of the multicollinearity test show that the variance inflation factor (VIF) for SST is 27.4 (Table 3). The VIF is a statistical measure used to assess the degree of multicollinearity, indicating how the interrelationships among independent variables affect the precision and stability of a linear regression model45,46,47. Typically, the VIF of less than 10 is considered acceptable for multicollinearity. Since the VIF for SST exceeds 10, it was excluded from the analysis. We then employed 10m zonal wind, 10m meridional wind, 10m wind speed, MSL, LH, SH, and NR as independent variables, with SIC as the dependent variable, to construct the GTWR model, quantifying the effects of these factors on SIC.
The statistical results of the regression coefficients for each environmental variable in the GTWR model are presented in the Table 2. The regression coefficients shown are standardized coefficients, where a larger absolute value indicates a greater impact on SIC48. The LH exhibits the most significant impact on SIC, with a median value of 1.44. This is followed by 10m zonal wind, 10m meridional wind, MSL, SH, and NR. The influence of 10m wind speed is the least, with a median value of 0.09.
Table 2
Statistics of regression coefficients of environmental factors in GTWR model
| Mean | First quartile | Second quartile* | Third quartile |
10m u-component of wind | 0.49 | 0.07 | 0.29 | 0.65 |
10m v-component of wind | 0.41 | 0.08 | 0.28 | 0.60 |
Mean sea level pressure | 0.48 | 0.08 | 0.29 | 0.69 |
10m wind speed | 0.13 | 0.02 | 0.09 | 0.18 |
Latent heat flux | 2.04 | 0.36 | 1.44 | 3.01 |
Net thermal radiation | 0.37 | 0.07 | 0.24 | 0.53 |
Sensible heat flux | 0.76 | 0.15 | 0.52 | 1.11 |
Table 3
Statistics of regression coefficients of environmental factors in GTWR model
Environmental factor | Collinearity statistics |
Allowance | VIF |
10m u-component of wind | 0.159 | 6.302 |
10m v-component of wind | 0.417 | 2.397 |
Mean sea level pressure | 0.194 | 5.145 |
Sea surface temperature | 0.063 | 25.323 |
10m wind speed | 0.138 | 7.225 |
Latent heat flux | 0.133 | 7.791 |
Net thermal radiation | 0.376 | 2.662 |
Sensible heat flux | 0.311 | 3.218 |
Figure 8 shows the change in the regression coefficients of zonal wind on SIC. In most regions, the zonal wind promotes sea ice growth. This is because the strengthening of the zonal wind leads to an accelerated Ekman transport, which moves colder surface water northward49. This cold water transport lowers the sea surface temperature in the northern areas, facilitating sea ice formation. Particularly under the influence of the Weddell Gyre, the enhanced zonal wind may push cold water northward while reducing heat exchange between the atmosphere and the ocean, thereby stabilizing sea ice50,51. In contrast, at the northern tip of the Antarctic Peninsula, zonal wind suppresses sea ice growth, and in 2013, the extent of this suppression expanded. This is due to the significant impact of the Antarctic Peninsula’s topography on local wind fields. The peninsula’s terrain may amplify wind speeds in certain areas, increasing ocean surface turbulence and enhancing vertical mixing of the water column52. This mixing can bring warmer deep water to the surface, inhibiting sea ice formation.
Figure A1 illustrates the variation in the regression coefficients of meridional wind on SIC. It can be observed that, in most regions, meridional wind promotes sea ice growth. This is because the strengthening of meridional wind transports cold air from the Antarctic continent to the Weddell Sea, lowering sea surface temperatures and reducing sea ice melt, which in turn facilitates the formation and expansion of sea ice53. Under the influence of the Ekman effect, meridional wind induces a shift in water flow at the ocean surface. Southerly winds typically push sea ice northward, while northerly winds tend to push warmer surface waters southward54. This transport mechanism helps establish cold water bands in the Weddell Sea, creating favorable conditions for sea ice expansion. However, in the central Weddell Sea, meridional wind suppresses SIC growth in certain areas. This suppression is likely due to strong southerly winds altering sea ice distribution by pushing it northward, leading to reduced sea ice coverage in the central Weddell Sea. Additionally, changes in northerly winds may enhance Ekman suction of deeper warm waters, bringing them to the surface, further inhibiting sea ice growth.
Figure A2 shows the variation in regression coefficients of MSL on SIC from 2011 to 2023. It is evident that MSL inhibits sea ice growth in the northern Weddell Sea while promoting it along the southern coastal regions of the Weddell Sea. In the northern Weddell Sea, higher MSL is typically associated with anticyclonic weather systems. These high-pressure systems often bring clear skies, increasing solar radiation, which raises surface temperatures and thus inhibits sea ice formation4. Additionally, high-pressure systems generally result in weaker winds, potentially reducing the transport of cold air from the Antarctic continent, further suppressing sea ice growth. In contrast, along the southern coastal regions of the Weddell Sea, lower MSL is typically linked to cyclonic systems, which often bring stronger winds, particularly facilitating the transport of cold air from the Antarctic continent to the ocean. This situation is conducive to sea ice growth. Furthermore, lower pressure may enhance Ekman transport effects along the coast, pushing colder surface water upward, which helps maintain or increase sea ice coverage. However, the impact of these factors has shown a declining trend over the years. This may be due to changes in climate patterns in the Antarctic region as global warming progresses. Changes in heat exchange between the atmosphere and ocean, accelerated ice sheet melting, and alterations in atmospheric circulation may all contribute to weakening the direct influence of MSL on sea ice growth55. Over time, these changes have likely reduced the impact of pressure systems on sea ice dynamics.
Figure A3 shows the variation in regression coefficients of wind speed on SIC. It can be observed that the impact of wind speed on SIC does not display a clear spatial pattern. This lack of pattern may be due to the inherently low influence of wind speed on SIC. Additionally, in the ERA5 dataset, wind speed is not a vector variable, meaning it lacks directional information. However, in the Weddell Sea, wind direction is particularly important for influencing sea ice dynamics.
Figure A4 shows the variation in regression coefficients of LH on SIC from 2011 to 2023. It is evident that LH promotes sea ice growth in most regions. This is because LH involves the condensation of water vapor in the air, a process that releases heat56. Typically, in the Weddell Sea, when atmospheric water vapor encounters the colder sea surface, condensation occurs. The LH released during this condensation is absorbed by the surrounding air, raising the air temperature, which in turn triggers further condensation of water vapor57. This process leads to surface cooling, thereby promoting sea ice formation, as the formation of sea ice requires sea water temperatures to be close to the freezing point.
Figure A5 shows the variation in regression coefficients of NR on SIC. It can be observed that the impact of NR on SIC does not display a clear pattern. This lack of consistency is due to the fact that the balance of NR is influenced by factors such as cloud cover, ice surface reflectivity, atmospheric composition, and surface characteristics. These factors make the effect of NR on sea ice complex and difficult to predict.
In the western and eastern Weddell Sea, SH promotes sea ice growth by cooling the ice surface (Figure A6). However, in the central Weddell Sea, the phenomenon of SH inhibiting sea ice growth may be closely related to the region's unique atmospheric and oceanic conditions. In the central area, northerly winds and ocean currents may transport relatively warm air and water to this region. SH transfers heat from the atmosphere to the ice surface, leading to ice melt or inhibiting new ice formation58. This localized transport of warm air and water causes the effect of SH in the central region to differ significantly from that in the western and eastern regions, thereby suppressing sea ice growth.