The Saharan Air Layer (SAL) is a mass of very dry, dusty air that originates over the Sahara Desert during the late spring, summer, and early fall, forming a layer approximately 2 to 2.5 miles thick that begins about 1 mile above the surface and travels westward across the tropical North Atlantic Ocean roughly every three to five days.[1] This phenomenon is driven by the African Easterly Jet, which propels the air mass at speeds of 25 to 55 miles per hour between 6,500 and 14,500 feet in altitude, peaking in activity from late June to mid-August.[1] Characterized by extreme dryness—containing about 50% less moisture than the typical tropical atmosphere—the SAL also features elevated temperatures and high concentrations of mineral dust particles, primarily in sizes ranging from 0.25 to 4 micrometers, which scatter sunlight and alter atmospheric radiation balance.[1][2]The SAL's transport mechanisms involve trade winds and African easterly waves, carrying plumes that can span vast areas, such as the size of the contiguous United States during intense outbreaks, and extend from near the surface up to 5–6 kilometers in altitude.[3][1] These plumes increase air temperatures by 1–2 Kelvin around 2 kilometers altitude while enhancing atmospheric stability below that level, which inhibits vertical motion and convection in the underlying marine boundary layer.[3]Dust within the SAL reduces incoming shortwave radiation at the ocean surface by up to 45 W/m² while increasing longwave radiation by about 20 W/m², resulting in a net radiative cooling of 20–30 W/m² that cools sea surface temperatures by up to 0.5 Kelvin under the plume and influences heat fluxes.[2]One of the most significant impacts of the SAL is its suppression of tropical cyclone formation and intensification in the Atlantic basin, achieved through increased vertical wind shear, mid-level dryness that promotes downdrafts, and overall atmospheric stabilization that limits moisture convergence.[1][4] Dust-induced cooling further reduces enthalpy fluxes beneath the plume, weakening potential storms.[2] Beyond hurricanes, the SAL affects regional climate by modifying air-sea interactions, such as reducing latent and sensible heat fluxes beneath the plume while enhancing them to the south, and altering precipitation patterns over West Africa and the North Atlantic.[2] When plumes reach the Caribbean and southeastern United States, they degrade air quality, exacerbate respiratory issues for vulnerable populations, and create hazy skies with enhanced sunsets, though the dust also plays a role in fertilizing distant ecosystems like the Amazon rainforest.[1][5] NOAA tracks the SAL using satellites such as GOES and Suomi-NPP, employing visible, infrared, and water vapor imagery to monitor its extent, intensity, and trajectory in real time.[4]
Physical Characteristics
Composition and Structure
The Saharan Air Layer (SAL) is defined as a hot, dry, and dust-laden mass of air originating from the Sahara Desert, typically extending from about 1.5 to 5.5 km above sea level with a vertical thickness of 2 to 4 km.[6][7] This layer forms a distinct atmospheric feature that overlies the cooler, more humid marine boundary layer in the tropical North Atlantic. Annually, it facilitates the transport of about 182 million tons of dust from Saharan Africa across the Atlantic, with 40 to 130 million tons reaching the Americas, primarily through easterly trade winds.[5][8]Structurally, the SAL constitutes a well-mixed, dry adiabatic layer characterized by an inversion at its base, which caps the underlying moist marine air and isolates the layer from the upper tropospheric flow above.[9][7] This inversion arises from the sharp temperature gradient where warm Saharan air overlies cooler oceanic air, maintaining stability and limiting vertical exchange.[9] The well-mixed nature of the layer results from intense solar heating over the desert surface, which drives deep convection and homogenizes the air mass, including its dust content, throughout its depth.[10][11]The dust within the SAL primarily consists of silicate minerals derived from Saharan soils, such as clays and quartz, with particle sizes ranging from 0.1 to 10 microns.[12][13] These fine particles are efficiently integrated into the air mass during mobilization, influencing the layer's radiative properties by absorbing and scattering solar radiation, which in turn affects visibility and atmospheric heating.[14] The dust-laden composition enhances the SAL's role in suppressing convection in underlying tropical systems through increased stability and reduced moisture availability.[15]
Temperature and Humidity Profiles
The Saharan Air Layer (SAL) exhibits a distinct temperature profile characterized by elevated warmth in the mid-troposphere, typically 5–10°C warmer than surrounding air masses, primarily due to large-scale subsidence within the subtropical high-pressure system and the absorption of solar radiation by embedded dust particles.[16] This warming is most pronounced at the layer's base around 850 hPa, creating a strong inversion that separates the SAL from the cooler marine boundary layer below.Relative humidity within the SAL is extremely low, often below 20%, in stark contrast to the moist boundary layer underneath, where humidity can exceed 70%. This aridity results from intense surface heating over the Sahara that desiccates the air without subsequent moistening, establishing a sharp vertical gradient at the inversion base that enhances atmospheric stability. The low humidity in the SAL contributes to the suppression of tropical cyclone development by entraining dry air into convective systems, though this effect is detailed further in related meteorological impacts.[16]The layer's stability is governed by a dry adiabatic lapse rate of approximately 9.8°C/km, reflecting its well-mixed nature and promoting internal vertical mixing while inhibiting deep convection through the capping inversion. Radiative processes amplify this profile, as dust particles absorb incoming shortwave radiation to further warm the mid-levels internally, while simultaneously reflecting sunlight back to space, which cools the underlying surface.[16]Vertically, the SAL spans 2–4 km in thickness under typical conditions, with its base near 1.5–2 km above the surface and the top extending to about 5–6 km; during intense dust outbreaks, it can reach higher altitudes. These variations influence the layer's overall thermodynamic influence across the Atlantic.
Formation and Sources
Seasonal Formation Process
The Saharan Air Layer (SAL) forms primarily during late spring, around May, as intense solar heating begins to intensify over the Sahara Desert, reaching its peak intensity from June to August before declining in early fall, typically September to October. This seasonal cycle is closely linked to the development and strengthening of the North African heat low, a semi-permanent low-pressure system driven by extreme surface temperatures that enhances regional convection and atmospheric instability.[6][17]The initial development of the SAL begins with intense surface heating over the arid Sahara, which triggers strong daytime convection and the growth of a deep, well-mixed boundary layer. This convective mixing dries the lower troposphere and elevates warm air, often reaching heights of 3–5 km by late afternoon, creating a stable, elevated layer characterized by low relative humidity (typically below 30%) and high temperatures. Dustentrainment occurs during this process as surface particles are lifted into the mixing layer, though the primary structure forms independently of dust loading.[10][18]Subsidence from the overlying subtropical high-pressure system plays a critical role in reinforcing the SAL's dryness and warmth, capping the mixed layer and forming the prominent trade wind inversion at its base, usually around 850 hPa. This descending air suppresses vertical motion, maintaining the layer's thermodynamic stability as it extends westward. The concept of the SAL as a distinct atmospheric feature was first hypothesized in 1972 by researchers Toby N. Carlson and Joseph M. Prospero, who identified it through analysis of large-scale Saharan air outbreaks and their interaction with African easterly flows.[19][20]During monsoon transitions, the SAL extends southward into the Sahel region, where interactions with the advancing West African monsoon flow contribute to greater layer depth by incorporating drier Saharan air into the transitional boundary layer. This extension modulates the depth and stability of the SAL, particularly as the Intertropical Convergence Zone shifts northward, influencing the overall vertical structure before the layer's seasonal decline.[17]
Dust Mobilization Mechanisms
The primary sources of dust for the Saharan Air Layer (SAL) are erodible basins in the Sahara Desert, including the Bodélé Depression in Chad, the Hoggar and Tibesti Mountains in Algeria and Libya, and other regions such as the Tidihelt Depression in central Algeria.[21][22] These areas provide fine silicate particles from ancient lake beds, desiccated soils, and weathered rock, with the Bodélé Depression a major source, contributing approximately 10–20% of Saharan mineral aerosol emissions based on recent multi-model estimates.[21][23][22]Dust mobilization begins at the surface through aerodynamic lifting when wind speeds exceed threshold velocities of around 6-8 m/s for fine particles, facilitated by the arid climate and sparse vegetation cover across the Sahara, where normalized difference vegetation index (NDVI) values often remain below 0.18, suppressing stabilization of soils.[24][25] Key lifting mechanisms include haboob thunderstorms and associated cold pool outflows from mesoscale convective systems, which generate intense gust fronts with winds up to 20-30 m/s, elevating dust to altitudes of 5-6 km in a matter of hours.[22][26] These outflows, often nocturnal, dominate summertime emissions, accounting for over 80% of dust pixels in satellite observations and forming arc-shaped plumes that rapidly entrain particles.[22]Sustained suspension is provided by low-level jets (LLJs), such as the Bodélé LLJ, which accelerate surface winds to 10-15 m/s or higher through channeling between topographic features like the Tibesti Mountains and Ennedi ridge, with breakdown events post-sunrise further intensifying near-surface turbulence.[21][22] The West African Easterly Jet, operating at low to mid-levels, contributes to broader shear and momentum transfer that maintains dust aloft during outbreaks.[27] Once lifted, dust particles are entrained into the dry adiabatic layer forming the SAL base through vertical turbulent mixing driven by wind shear and convective instability, allowing a substantial portion—estimated at 20-40% in modeling studies—to integrate into the elevated SAL structure rather than depositing locally.[28][29]Major dust outbreaks occur frequently during the summer season (June–August), with events emerging roughly every 3 to 5 days, each mobilizing 10–50 million tons of material, with cold pool-driven events peaking in frequency and intensity during this period due to enhanced convection over the Sahel.[22][30][6] Recent analyses as of 2024 show an increasing trend in dust outbreak frequency and intensity, attributed to climate change.[31] These episodic releases, combined with diurnal LLJ cycles, ensure high dust yields from sparsely vegetated, hyper-arid surfaces where evaporation rates exceed 2,000 mm/year and soil moisture is minimal, promoting easy particle detachment.[21][24]
Transport Across the Atlantic
Pathways and Trajectories
The Saharan Air Layer (SAL) is primarily transported westward across the Atlantic Ocean by mid-tropospheric easterly winds, including the African Easterly Jet and associated anticyclonic circulations, at altitudes ranging from 1.5 to 4.5 km above the surface.[6] These winds propel the layer, which typically takes 5 to 10 days to cross the Atlantic basin, with plumes originating from dust sources in the Sahara and Sahel regions of North Africa.[32] The SAL's trajectory is characterized by two main branches: a northern branch that influences the Canary Islands and occasionally extends to southern Europe via northerly pathways over the Mediterranean, and a southern branch that directs dust toward the Caribbean, Central America, and the southeastern United States.[33]Individual SAL events form expansive plumes spanning 2,000 to 5,000 km in width, advected at horizontal speeds of approximately 10 to 25 m/s, though gusts within the layer can reach up to 25 m/s.[6] A significant fraction of Saharan dust is transported via these transatlantic pathways, depositing around 50 to 70 million tons annually in regions such as the Caribbean and Amazon Basin.[32] En route, the layer experiences slight descent due to its stable, dry structure, but it may ascend locally over warmer ocean surfaces, maintaining its elevated position through much of the journey.[6]Arrival patterns vary by branch, with the southern trajectory peaking in April to June as dust events more frequently follow southward paths toward the Americas, while the northern branch intensifies in July to September, aligning with the height of the Atlantic hurricane season for some events but delivering to higher latitudes.[33] These seasonal dynamics reflect the modulation of trade wind strength and the positioning of subtropical high-pressure systems, which steer the SAL's overall westward progression.[34] Notable recent events include intense transport during July-August 2024 and frequent plumes in the first half of 2025, such as a prominent one in June 2025 observed from space.[35][36][37]
Influencing Meteorological Factors
The transport of the Saharan Air Layer (SAL) across the Atlantic is primarily driven by the West African Easterly Jet (WA EJ), a mid-level wind feature that accelerates the layer's westward progression and sustains dust suspension within it. The WA EJ typically exhibits wind speeds of 10–17 m/s, occasionally reaching up to 25 m/s, centered at approximately 3 km altitude near the 700 hPa pressure level. This jet enhances the SAL's stability and speed, facilitating its advection over thousands of kilometers while contributing to increased vertical wind shear in the region.[6]The North Atlantic Subtropical High (NASH), an anticyclonic circulation system, plays a crucial role in steering the SAL southward and westward during its transatlantic journey. The position and intensity of the NASHridge determine the latitude and trajectory of the dust plume, often directing it toward the Caribbean and southeastern United States when the high is positioned favorably in the mid-latitudes.[38] Variations in the NASH's strength can alter the SAL's path, with stronger highs promoting more direct westward flow and extended reach.Interactions between the SAL and the Intertropical Convergence Zone (ITCZ) significantly influence moisture dynamics during transport, as the dry, stable SAL air can override or deflect the ITCZ's ascending branch. This overriding reduces upward motion and convective activity within the ITCZ, thereby limiting moisture influx into the mid-troposphere and maintaining the SAL's aridity.[39] Such interactions often occur along the SAL's southern boundary, where dust-laden air modulates precipitation patterns over the tropical Atlantic.Oceanic influences, particularly sea surface temperatures (SSTs), modulate the SAL's vertical structure by affecting descent or ascent processes at its base. Warmer SSTs in the tropical Atlantic can enhance surface evaporation and low-level convergence, potentially eroding the SAL's dry base through increased moistureentrainment and destabilization.[40] This erosion is more pronounced over regions with SST anomalies exceeding 28°C, where upward heat fluxes weaken the temperature inversion capping the layer.[41]Variability in SAL transport is notably influenced by phases of the El Niño-Southern Oscillation (ENSO), with La Niña conditions typically strengthening the WA EJ and enhancing dust mobilization and export. During La Niña years, cooler equatorial Pacific SSTs promote a more robust easterly flow over West Africa, leading to increased SAL intensity and frequency compared to El Niño periods.[42] This ENSO modulation can result in up to 20% higher dust concentrations in the tropical North Atlantic during La Niña events, amplifying the layer's overall impact.
Meteorological and Climatic Impacts
Suppression of Tropical Cyclones
The Saharan Air Layer (SAL) plays a significant role in suppressing the development and intensification of tropical cyclones in the Atlantic basin by introducing environmental conditions that disrupt the thermodynamic and dynamic processes essential for storm growth. The SAL's dry air, enhanced vertical wind shear, and increased atmospheric stability collectively inhibit convection and structural organization within nascent or existing cyclones. Observational studies have documented these effects through satellite imagery, aircraft reconnaissance, and radiosonde data, highlighting the SAL's influence on approximately 65% of Atlantic tropical cyclones that originate from African easterly waves.[43]One primary mechanism is the intrusion of extremely dry air from the SAL into tropical cyclone circulations, where relative humidity levels are often below 20% in the mid-levels (600-850 hPa), compared to 25-45% lower than the surrounding moist tropical air. This dry air entrainment promotes mid-level evaporative cooling, which generates downdrafts that suppress updrafts and reduce convective available potential energy (CAPE), thereby weakening the storm's core convection and inhibiting intensification. For instance, during Hurricane Danielle in 1998, SAL dry air extended over 5,000 km across the Atlantic, leading to suppressed convection and failure to intensify beyond tropical storm strength. Similarly, in Hurricane Georges (1998) and Joyce (2000), the entrainment of SAL air caused notable convective suppression and structural degradation.[43]The SAL also generates vertical wind shear through its embedded mid-level easterly jet, with winds typically ranging from 10-17 m/s and occasionally reaching 25 m/s, resulting in shear magnitudes of 20-30 m/s that disrupt the alignment of the low- and upper-level vortex centers. This shear tears apart the eyewall formation and promotes asymmetric convection, further hindering intensification; storms interacting with the SAL experience shear increases of 20-30 m/s, often leading to weakening. Additionally, the SAL's warm temperature inversion (5-10°C warmer than surrounding air at 800-900 hPa) caps vertical motion, stabilizing the mid-troposphere and preventing the deep moist ascent required for rapid intensification by limiting the release of latent heat. Thermodynamically, this inversion enhances static stability, reducing the potential for organized deep convection essential to cyclone growth.[43]Observational evidence indicates that tropical cyclones embedded within the SAL intensify at substantially lower rates than those outside it, with case studies showing suppressed development in SAL-affected systems; for example, Hurricane Debby (2000) exhibited stalled intensification due to SAL intrusion, contrasting with non-SAL storms that achieved hurricane status more readily. Broader analyses reveal that SAL-embedded disturbances are less likely to develop into major hurricanes, contributing to interannual variability in Atlantic activity. This suppression is linked to the African monsoon through a feedback mechanism: stronger monsoonal rainfall weakens the SAL by increasing regional humidity and reducing dust mobilization, correlating with higher hurricane peak intensities (r = 0.82 for Sahel rainfall and intensity), while drought conditions enhance SAL strength, dry air, and shear, reducing activity (r = -0.77 for shear). Thus, the SAL serves as a climatic bridge between Sahelian precipitation and Atlantic cyclone suppression.[43][44]
Effects on Regional Weather and Air Quality
The Saharan Air Layer (SAL) significantly disrupts regional weather patterns, particularly through the generation of calima events in the Canary Islands and similar dust incursions in the Caribbean. These events involve dense dust clouds that drastically reduce visibility, often to less than 1 km, leading to hazardous driving conditions, school closures, and temporary halts in outdoor activities. In severe cases, such as the January 2002 calima in the Canary Islands, visibility at Tenerife's Santa Cruz airport dropped below 50 meters, forcing its complete closure and stranding thousands of travelers.[45] Similar disruptions occur in the Caribbean, where SAL dust layers create hazy skies and reduced visibility, exacerbating local weather instability during the summer months.SAL dust plumes also degrade air quality in downwind regions, notably the southeastern United States, by elevating particulate matter concentrations. Fine dust particles, including PM10 and PM2.5, can push air quality indices into unhealthy or hazardous categories, prompting health advisories for vulnerable populations. The 2020 "Godzilla" dust event, one of the most intense on record, transported massive plumes across the Atlantic, resulting in hazardous air quality along the Gulf Coast from Texas to Florida, with PM2.5 levels exceeding safe thresholds and causing widespread hazy conditions.[46] The mineral composition of the dust, rich in iron and silicates, contributes to these persistent aerosol burdens that linger in the atmosphere for days.Through direct radiative forcing, the SAL reflects incoming solar radiation, leading to surface cooling over the tropical North Atlantic, with sea surface temperatures reduced by approximately 0.5–1°C during peak events.[47] This cooling alters local atmospheric stability and can suppress precipitation patterns, such as contributing to drier conditions in the Sahel region by modifying the radiative balance and convective activity. The dust's scattering and absorptionproperties diminish shortwave radiation reaching the ocean by up to 190 W/m², influencing air-sea interactions and potentially shifting rainfall distributions in affected areas.[48]Ecologically, SAL dust deposition provides essential nutrients to remote ecosystems, fertilizing Amazonian soils with about 22,000 tons of phosphorus annually, which supports forest productivity and offsets nutrient losses from rainfall.[5] In the Atlantic Ocean, the iron-rich dust stimulates phytoplankton growth and algal blooms, enhancing marine primary production. However, excessive deposition can introduce stressors to marine environments, such as contributing to coral diseases and degradation through pathogen transport, alongside factors like warming waters that cause bleaching, though the dust's alkaline nature generally buffers ocean acidification rather than exacerbating it.[49]Public health impacts from SAL exposure are pronounced, with dust particles penetrating respiratory systems and triggering inflammation that exacerbates asthma, pneumonia, and allergic responses in downwind populations. Studies link these events to increased emergency department visits for respiratory issues and elevated risks of cardiovascular diseases, including heart failure, due to oxidative stress from inhaled particulates. Annually, Saharan dust affects air quality and health for millions in regions spanning the Caribbean, southern Europe, and the Americas, with Caribbean communities experiencing some of the world's highest asthma rates partly attributable to recurrent plumes.[50]
Observation and Research
Detection Methods
Satellite observations play a crucial role in detecting and monitoring the Saharan Air Layer (SAL) by identifying dust plumes and associated atmospheric anomalies across large scales. Geostationary Operational Environmental Satellite (GOES) imagery utilizes infrared channels, particularly the 10.7–12 μm bands, to detect silicate dust-induced temperature anomalies and dry air signatures within the SAL, enabling real-time visualization of layer extent and movement. Moderate Resolution Imaging Spectroradiometer (MODIS) on NASA's Aqua and Terra satellites measures aerosol optical depth (AOD), with values exceeding 0.5 indicating significant dust concentrations typical of SAL plumes over the Atlantic.[51] These visible and infrared techniques provide broad coverage for initial plume identification, often complemented by multispectral analysis to distinguish dust from other aerosols.[52]Radiosonde profiles offer direct in situ measurements to confirm SAL presence through vertical soundings of temperature and humidity. These balloon-borne instruments detect characteristic temperature inversions and sharp humidity decreases between approximately 700 hPa and 500 hPa, marking the dry, stable core of the SAL above the marine boundary layer.[53] Such profiles reveal relative humidity dropping to below 20% in the layer, contrasting with moister conditions below and above, and are routinely launched from island stations like the Canary Islands or Barbados to validate satellite detections.[54]Lidar and radar systems provide detailed vertical profiling of the SAL's dust layers. The Cloud-Aerosol Lidar with Orthogonal Polarization (CALIPSO) satellite employs spaceborne lidar to quantify aerosol backscatter and depolarization ratios, delineating the SAL's elevated structure typically between 1.5 and 5 km altitude with high vertical resolution.[55] Ground-based lidars, such as those at the Canary Islands observatories, complement this by measuring extinction coefficients and layer boundaries during transatlantic transport events. These active remote sensing tools excel in resolving the SAL's internal dust distribution and interactions with clouds, offering data for both research and operational use.[7]The National Oceanic and Atmospheric Administration (NOAA) produces operational SAL tracking maps by assimilating satellite-derived AOD and other observations into numerical models like the Global Forecast System (GFS). This approach, implemented since 2005 following Joint Hurricane Test projects, generates forecast products for SAL position and intensity, aiding hurricane season monitoring in the Atlantic basin.[6]Recent advancements incorporate artificial intelligence to enhance satellite-based SAL plume prediction. Machine learning models, such as DustNet, leverage neural networks trained on historical satellite imagery and reanalysis data to forecast aerosol optical depth from Saharan dust up to 24 hours ahead with superior accuracy over traditional physics-based methods at most grid points.[56] Techniques like convolutional neural networks applied to geostationary satellite data reconstruct cloud-obscured plumes, improving detection reliability and extending predictive lead times to 7–10 days when integrated with ensemble models.[57] These AI-driven tools, developed in 2024–2025, facilitate earlier warnings for dust impacts on weather and air quality.[58]
Historical Development and Key Studies
The Saharan Air Layer (SAL) was first characterized in the late 1960s through observations during the Barbados Oceanographic and Meteorological Experiment (BOMEX), with Toby N. Carlson and Joseph M. Prospero providing the definitive description in their 1972 study based on radiosonde data that revealed a dry, warm, dust-laden layer elevated over the tropical North Atlantic.[59] This work linked the SAL to large-scale Saharan air outbreaks, establishing its role in transporting African dust westward and influencing Atlantic weather patterns, building on earlier hints from dust detections in the Caribbean during the 1950s and 1960s.[59]Research in the 1980s and 1990s advanced understanding of the SAL's dynamical effects, with V. M. Karyampudi and T. N. Carlson's 1988 numerical simulations demonstrating how the layer's vertical wind shear and stability could suppress easterly wave disturbances while also potentially enhancing barotropic instability in some scenarios. Building on this, Karyampudi and H. F. Pierce's 2002 analysis quantified the SAL's synoptic-scale influence on tropical cyclogenesis over the eastern Atlantic, showing it could either inhibit or promote cyclone formation depending on wave-SAL interactions. A pivotal advancement came in 2004 with Jason P. Dunion and Christopher S. Velden's study, which used satellite and radiosonde data to illustrate the SAL's multifaceted suppression of Atlantic hurricanes through dry air entrainment, increased vertical shear (contributing substantially to mid-level wind differences), and enhanced atmospheric stability.[60]Contemporary research through 2025 has expanded on these foundations, emphasizing the SAL's broader climatic role. A 2024 Stanford-led study employed machine learning models on 19 years of satellite and meteorological data to reveal how Saharan dust within the SAL regulates tropical cyclone rainfall, suppressing it over the open Atlantic by blocking solar energy while potentially intensifying it near landfall through altered cloud processes.[61] Recent NOAA-supported investigations, including 2025 modeling of future dust scenarios, have highlighted SAL-climate feedbacks tied to the African monsoon, where reduced Sahel precipitation and a weaker easterly jet under warming conditions amplify dust emissions, creating positive loops that alter regional circulation and Atlantic variability.[62]Despite progress, key research gaps persist, including limited post-2022 analyses of the SAL's ecological impacts, such as nutrient deposition effects on marine and terrestrial ecosystems in the Americas.[30] Emerging AI-driven monitoring tools, like neural networks for dust plume prediction, show promise but require validation across diverse conditions. Links between the SAL and ENSO remain incompletely understood, with preliminary evidence suggesting El Niño phases may modulate dusttransport via altered trade winds, warranting targeted studies. Future directions prioritize improved Earth system models to capture dust-climate interactions, including radiative forcing and monsoon feedbacks, alongside investigations into understudied nutrient deposition consequences for global biogeochemical cycles.[63][62]