Articles | Volume 22, issue 8
Atmos. Chem. Phys., 22, 5253–5263, 2022
https://doi.org/10.5194/acp-22-5253-2022
Atmos. Chem. Phys., 22, 5253–5263, 2022
https://doi.org/10.5194/acp-22-5253-2022
Research article
21 Apr 2022
Research article | 21 Apr 2022

Causal influences of El Niño–Southern Oscillation on global dust activities

Causal influences of El Niño–Southern Oscillation on global dust activities
Thanh Le and Deg-Hyo Bae Thanh Le and Deg-Hyo Bae
  • Department of Civil and Environmental Engineering, Sejong University, 05006 Seoul, Republic of Korea

Correspondence: Deg-Hyo Bae (dhbae@sejong.ac.kr) and Thanh Le (levinhthanh.lvt@gmail.com)

Abstract

The dust cycle is an important element of the Earth system, and further understanding of the main drivers of dust emission, transport, and deposition is necessary. The El Niño–Southern Oscillation (ENSO) is the main source of interannual climate variability and is likely to influence the dust cycle on a global scale. However, the causal influences of ENSO on dust activities across the globe remain unclear. Here we investigate the response of dust activities to ENSO using output from Coupled Modeling Intercomparison Project Phase 6 (CMIP6) historical simulations during the 1850–2014 period. The analyses consider the confounding impacts of the Southern Annular Mode, the Indian Ocean Dipole, and the North Atlantic Oscillation. Our results show that ENSO is an important driver of dry and wet dust deposition over the Pacific, Indian, and Southern oceans and parts of the Atlantic Ocean during 1850–2014. Over continents, ENSO signature is found in America, Australia, parts of Asia, and Africa. Further, ENSO displays significant impacts on dust aerosol optical depth over oceans, implying the controls of ENSO on the transport of atmospheric dust. Nevertheless, the results indicate that ENSO is unlikely to exhibit causal impacts on regional dust emissions of major dust sources. While we find high consensus across CMIP6 models in simulating the impacts of ENSO on dust deposition and transport, there is little agreement between models for the ENSO causal impacts on dust emission. Overall, the results emphasize the important role of ENSO in global dust activities.

1 Introduction

The dust cycle is an important component of the Earth system (Bullard et al., 2016; Carslaw et al., 2010; Jickells et al., 2005; Knippertz and Todd, 2012). Dust may alter the balance of the radiative forcing of the climate system (Carslaw et al., 2010; Schulz et al., 2012; Xu et al., 2017), and changes in dust transport and distribution may have impacts on regional climate (Creamean et al., 2013; Evan et al., 2011; Kok et al., 2018; Li et al., 2019; Rotstayn et al., 2011; Scott et al., 2018; Yang et al., 2017). Dust deposition is a source of nutrients (e.g., dust iron, phosphorus, and nitrogen) for land and ocean ecosystems (Bao et al., 2017; Fan et al., 2006; Jickells et al., 2005; Jiménez et al., 2018; Kanakidou et al., 2018; Schulz et al., 2012; Tagliabue et al., 2010). In particular, long-range transport of mineral dust may alter the global biogeochemical cycles and regional soil composition (D'Odorico et al., 2013; Duan et al., 2021; Perry et al., 1997; Prospero and Mayol-Bracero, 2013). On the other hand, dust transports may cause pollution and have significant impacts on human health (Li et al., 2021; de Longueville et al., 2013; Shahsavani et al., 2020; Tong et al., 2017; Yang et al., 2017) and environments (Guo et al., 2017; Li et al., 2019; Perry et al., 1997; Xu et al., 2017; Zhang et al., 2018).

Dust emission, transport, and deposition are driven by vegetation cover, soil moisture, precipitation, and wind speed (Carslaw et al., 2010; Kanakidou et al., 2018; Kok et al., 2021; Pi et al., 2019; Thornhill et al., 2021). Hence, ENSO impacts on these variables (Cai et al., 2021; Le et al., 2022; Le and Bae, 2020; Yeh et al., 2018) are likely to result in ENSO-induced changes in dust activities. For instance, ENSO is shown to have influences on dust activities over Australia (Marx et al., 2009), the Sahara and Amazon basin (Boy and Wilcke, 2008), regions from the Arabian Peninsula to Central Asia (Huang et al., 2021), South America (Shao et al., 2013), and East Asia (Jeong et al., 2018). Nevertheless, ENSO influences on the dust cycle remain elusive. In particular, little effort has been made to evaluate the causal effects of ENSO on dust activities on a global scale.

While there are limited observational records of past dust deposition over oceans (van der Does et al., 2020), Earth system models contribute crucial datasets to examine the influences of ENSO on global dust activities. Recently, there has been improvement in understanding the global dust cycle (Kok et al., 2021) and simulating dust aerosol in Earth system models (Collins et al., 2017; Mulcahy et al., 2020; Thornhill et al., 2021; Zhao et al., 2022). In particular, Coupled Modeling Intercomparison Project Phase 6 (CMIP6) models (Eyring et al., 2016) are provided with a better description of the aerosol model and the atmospheric chemistry model and allow for a clearer understanding of ENSO impacts on dust activities.

In this work, we investigate the causal effects of ENSO on global dust activities. We consider the confounding influences of other main climate modes (i.e., the Indian Ocean Dipole (IOD), the Southern Annular Mode (SAM), and the North Atlantic Oscillation (NAO)). Further understanding of the linkages between ENSO and dust cycles at a global scale may contribute to the predictions of future dust events and their impacts under a changing environment.

2 Data and methods

2.1 Datasets

We employed monthly data of the following variables: dry deposition rate of dust (i.e., dry deposition due to gravitational settling, impact scavenging, and turbulent deposition – dry dust), wet deposition rate of dust (i.e., the surface deposition rate of dust due to wet processes – wet dust), dust optical thickness at 550 nm (i.e., total atmospheric aerosol optical depth due to dust at a wavelength of 550 nm – od550dust), and emission rate of dust (emidust). Dry dust and wet dust are important variables of dust deposition flux at land and ocean surface (Schulz et al., 2012), while od550dust represents the properties, transport, and distribution of dust in the atmosphere (Bullard et al., 2016; Collins et al., 2017). Dust emission is dependent on wind speed (or wind stress), land vegetation (e.g., leaf area index), and soil moisture (or soil type) (Kok et al., 2021). We used monthly sea surface temperature (SST) and sea level pressure (SLP) to calculate the time series of the main modes of climate variability (see also Sect. 2.2 Methods and Sect. S1 in the Supplement). These datasets were taken from the historical experiment (Eyring et al., 2016) covering the period 1850–2014. Tables S1 and S2 in the Supplement list the 12 CMIP6 models (with accessible dust-related data) utilized in the present work. We limited our study to all the models having both dry dust and wet dust data (i.e., there is total of 12 models with accessible dry dust and wet dust data as described in Table S2). Dust deposition on land and ocean surface is an important metric to assess the impacts of dust activities on ecosystems and environment (Bao et al., 2017; Fan et al., 2006; Jickells et al., 2005; Jiménez et al., 2018; Kanakidou et al., 2018; Schulz et al., 2012). Additional data of od550dust and emidust supplied by these 12 models provide further understanding of ENSO impacts on dust activities.

2.2 Methods

Following the methodology utilized in recent works (Le et al., 2021; Le and Bae, 2020), we evaluate the null hypothesis of no Granger causality between ENSO and dust activities (i.e., dust deposition rate, dust optical thickness, and emission rate of dust) by using a multivariate predictive model (see Sect. S1). We use the following multivariate predictive model (Mosedale et al., 2006; Stern and Kaufmann, 2013) to estimate the causal links between ENSO and dust deposition:

(1) X t = i = 1 p α i X t - i + i = 1 p β i Y t - i + j = 1 m i = 1 p δ j , i Z j , t - i + ε t ,

where Xt is the annual mean (or seasonal mean) dust deposition for year t, Yt is the ENSO index, and Zj,t is the confounding factor j for year t. In the predictive model presented in Eq. (1), while assessing the effect of Y on X (i.e., the contribution of the term i=1pβiYt-i in predicting X), the possible influence of past X events is considered by adding the term i=1pαiXt-i. Thus, the causal influence of Y on X, if detected, is robust, and the impact of past X events is accounted for in the analyses. Here, m is the number of confounding factors and p ≥1 is the order of the multivariate predictive model. The optimal order p is computed by minimizing the Schwarz criterion or the Bayesian information criterion (Schwarz, 1978). The optimal orders may be different for each model.

Here we take into account the impacts of confounding factors and therefore provide further information of the real-world teleconnections. In the analyses, we use three different confounding factors; hence, m is equal to 3. The noise residuals εt and the regression coefficients αi, βi, and δj,i are computed by using the multiple linear regression analysis of the least-squares method. We detrend and normalize all the climate indices.

In the analyses, we investigated the confounding effects of other main climate modes (i.e., the SAM (e.g., Cai et al., 2011), the IOD (Saji et al., 1999; Webster et al., 1999), and the NAO (Hurrell et al., 2003)) on the links of ENSO and dust activities. The climate modes SAM, IOD, and NAO are important sources of global climate variability (Hurrell et al., 2003; Luo et al., 2012; Roxy et al., 2015). For instance, the NAO is the prominent mode of atmospheric circulation variability over the North Atlantic and surrounding regions (Delworth et al., 2016; Hurrell et al., 2003), and variations in NAO are crucial for the environment and society (Hurrell et al., 2003). The IOD affects climate extremes over the Indian Ocean and surrounding areas (Abram et al., 2008; Kripalani et al., 2009; Kripalani and Kulkarni, 1997) and might cause severe economic consequences (Ummenhofer et al., 2009). The SAM is the major mode of atmospheric circulation variability in the Southern Hemisphere (Cai et al., 2011; Raphael and Holland, 2006). In addition, changes in these modes may affect the variations in ENSO (Abram et al., 2020; Cai et al., 2011, 2019; Le et al., 2020; Le and Bae, 2019). Nevertheless, it is likely that these factors may alter the influence of ENSO on dust activities. Further information on the methods is explained in Sect. S1.

3 Results

3.1 ENSO impacts on dust deposition, transport, and emission

Figure 1 denotes the causal influences of ENSO on the annual mean deposition rate of dry dust (a) and west dust (b) over the 1850–2014 period of the historical experiment. The results in Fig. 1 are described as the ensemble mean of 12 models (see Tables S1 and S2). We show that ENSO plays an important role in dust deposition over the Pacific, Indian, and Southern oceans; parts of the Atlantic Ocean; and the surrounding continents. In particular, ENSO exhibits a signature on both dry and wet dust deposition processes over the subarctic North Pacific, parts of the southern Arctic Ocean, and Antarctica. In these areas, the p value is lower than 0.33 (and 0.1), suggesting that ENSO is unlikely (and very unlikely) to exhibit no causal effects on dust deposition.

https://acp.copernicus.org/articles/22/5253/2022/acp-22-5253-2022-f01

Figure 1Multi-model mean probability map for the absence of Granger causality from ENSO to annual mean deposition rate of dry dust (a) and wet dust (b) over the period 1850–2014 of the historical experiment. Stippling indicates that no less than 70 % of all models show agreement on the mean probability of total models at a given grid point. The agreement of an individual model is specified when the difference between the multi-model mean probability and the selected model's probability is less than 1 standard deviation of the multi-model mean probability. The cyan and yellow contour lines specify p value = 0.33 and 0.1, respectively. Brown shades imply a low probability for no Granger causality. ENSO: El Niño–Southern Oscillation.

Further analyses reveal that ENSO displays significant impacts on aerosol optical depth over oceans, implying the controls of ENSO on the transport of atmospheric dust (Fig. 2a). Figure 2b shows the scale of ENSO causal impacts on global dust activities. In Fig. 2b, the areas influenced by ENSO are computed as the areas limited by the cyan contour line as shown in Figs. 1 and 2a (i.e., p value is lower than 0.33 or ENSO is unlikely to exhibit no causal effects on dust activities over these regions). Over oceans, the areas affected by ENSO are estimated at approximately 17.6 %, 32.3 %, and 20.7 % of total Earth surface (i.e., 24.9 %, 45.6 %, and 29.2 % of total ocean areas) for deposition of dry dust, dust aerosol optical depth, and deposition of wet dust, respectively (Fig. 2b). The land areas affected by ENSO are estimated at approximately 5.1 %, 7.5 %, and 6.8 % of the total Earth surface (i.e., 17.5 %, 25.7 %, and 23.3 % of total land areas) for deposition of dry dust, dust aerosol optical depth, and deposition of wet dust, respectively (Fig. 2b).

https://acp.copernicus.org/articles/22/5253/2022/acp-22-5253-2022-f02

Figure 2(a) As in Fig. 1, except for the probability for the absence of Granger causality from ENSO to annual mean dust aerosol optical depth over the period 1850–2014 for the historical experiment. (b) Fraction of total Earth surface over land and ocean with probability for no Granger causality from ENSO to dust deposition and dust aerosol optical depth smaller than 0.33 (i.e., p value <0.33). Fraction areas affected by ENSO on dry dust, dust aerosol optical depth, and wet dust are displayed in blue, red, and yellow bars, respectively. ENSO: El Niño–Southern Oscillation.

The causal effects of ENSO on seasonal mean dry dust deposition are shown in Fig. S1 in the Supplement. The largest impacts of winter (DJF) ENSO are observed in the following spring (MAM), with approximately 3.4 % of total Earth surface over land (i.e., 11.6 % of total land areas) and approximately 16 % of total Earth surface over the ocean (i.e., 22.6 % of total ocean areas) being affected (Fig. S2). The impacts of ENSO on dry dust deposition gradually decrease in the following summer, fall, and winter (Figs. S1 and S2). In particular, the influences of ENSO on winter dry dust deposition are mainly limited in Antarctica (approximately 0.5 % of total Earth surface or 1.7 % of total land areas) and the tropical Pacific (approximately 0.7 % of total Earth surface or 1 % of total ocean areas).

The results in Fig. 3 demonstrate that ENSO is less likely (i.e., p value >0.33) to exhibit causal impacts on regional dust emissions of major dust sources (e.g., over northern Africa, the Middle East, and central Asia).

https://acp.copernicus.org/articles/22/5253/2022/acp-22-5253-2022-f03

Figure 3As in Fig. 1, except for the probability of the absence of Granger causality from ENSO and annual mean dust emission over the period 1850–2014 for the historical experiment. ENSO: El Niño–Southern Oscillation.

3.2 Models' consensus of ENSO effects on dust activities

High consensus across models is noted for the large causal effects of ENSO on global dust deposition (Fig. 1) and transport (Fig. 2a). However, there is little consensus across models for the impacts of ENSO on dust emissions (i.e., a limited area in central Australia, Fig. 3).

Figure 4 shows the findings of 12 different models (see Tables S1 and S2) for the causal effects of ENSO on dry dust over the 1850–2014 period of the historical experiment. The results for wet dust are shown in Fig. S3. The response of dry dust deposition is underestimated in the models CanESM5, CNRM_ESM2_1, and INM-CM4-8 compared to the models' mean (Fig. 1a). Over Europe and northern Africa, the model MIROC-ES2L exhibits a clearer response of dry dust deposition to ENSO compared to other models. Most models suggest a strong response of dry dust deposition to ENSO over the tropical Pacific.

https://acp.copernicus.org/articles/22/5253/2022/acp-22-5253-2022-f04

Figure 4As in Fig. 1, except for the probability of the absence of Granger causality from ENSO and annual mean dry dust deposition over the period 1850–2014 for the historical simulation of 12 different models (see Tables S1 and S2). ENSO: El Niño–Southern Oscillation.

Figure 5 shows the results of nine individual models (see Table S2) for the causal influences of ENSO on dust aerosol optical depth over the 1850–2014 period. Consistent with Fig. 4, the response of dust aerosol optical depth to ENSO is weaker in the models CanESM5 and INM-CM4-8 compared to others. The results described in Figs. 4 and 5 indicate that the models agree well on the causal signatures of ENSO on the spatiotemporal evolution of dust.

https://acp.copernicus.org/articles/22/5253/2022/acp-22-5253-2022-f05

Figure 5As in Fig. 1, except for the probability for the absence of Granger causality from ENSO to annual mean dust aerosol optical depth over the period 1850–2014 for the historical simulation of nine different models (see Table S2). ENSO: El Niño–Southern Oscillation.

Figure 6 shows the response of dust emissions to ENSO in 11 different models (see Table S2). ENSO may initiate dust activities in limited regions over Australia (CESM2, CESM2_WACCM, INM-CM4-8, INM-CM5-0, MIROC6 and UKESM1_0_LL), southern Africa (CESM2, CESM2_WACCM, INM-CM4-8, MIROC6 and UKESM1_0_LL), southern South America (UKESM1_0_LL), and southwestern North America (INM-CM4-8, INM-CM5-0, and UKESM1_0_LL). Several models (i.e., INM-CM5-0, UKESM1_0_LL) exhibit stronger ENSO signals on dust emissions compared to other models. The response of dust emissions to ENSO is much less apparent in the models CESM2_FV2 and CESM2_WACCM_FV2. As most models do not include high-latitude dust sources (Kok et al., 2021), the impacts of ENSO on dust emissions of high latitude are not visible.

https://acp.copernicus.org/articles/22/5253/2022/acp-22-5253-2022-f06

Figure 6As in Fig. 1, except for the probability of the absence of Granger causality from ENSO and annual mean dust emission over the period 1850–2014 for the historical simulation of 11 different models (see Table S2). ENSO: El Niño–Southern Oscillation.

4 Discussion

Based on the trace of dust deposition as shown in Fig. 1, ENSO-induced dust deposition in the North Pacific likely originates from major dust source regions over central and eastern Asia, consistent with previous work (Jickells et al., 2005). Dust deposited in the tropical Pacific might come from multiple dust sources over Australia, southwestern North America, or even South America. Figure 1 suggests that dust supply to the southern Indian Ocean might originate from a small dust source over South Africa, while dust deposition over the tropical Atlantic is associated with the major dust source of West Africa, potentially contributing to variations in the Atlantic Meridional Mode (Evan et al., 2011). As dust particles might be carried by winds between different regions (Guo et al., 2017; Yang et al., 2017), the influences of ENSO on global atmospheric circulation and rainfall (Yeh et al., 2018) lead to ENSO-induced changes in spatial pattern of dust deposition. For example, ENSO impacts on winds and precipitation over the tropical Pacific (Dai and Wigley, 2000; Le and Bae, 2020) contribute to the causal effects of ENSO on dry and wet dust deposition over this region (Fig. 1). In addition, ENSO atmospheric teleconnections over Australia, North America, and South America (Ashok et al., 2007; Garfinkel et al., 2013; Taschetto and England, 2009; Yu and Zou, 2013) play an important role in dust deposition in these regions (Fig. 1).

Significant impacts of ENSO on atmospheric aerosol loading (Figs. 2a and 5) may lead to a strong response of marine productivity (i.e., the production of organic matter in the ocean from carbon dioxide by phytoplankton) to ENSO. For example, there is strong correlation between aerosol optical depth and iron deposition and satellite chlorophyll (Carslaw et al., 2010; Jickells et al., 2005). The controls of ENSO on the transport of atmospheric dust (Fig. 2a) are consistent with the influences of ENSO on global wind patterns (Dai and Wigley, 2000; Le and Bae, 2020; Yeh et al., 2018). As dust deposition over the ocean and lakes may provide important nutrients for phytoplankton development, productivity, and carbon uptake (Jickells et al., 2005; Jiménez et al., 2018), ENSO may potentially modulate oceanic biogeochemistry and the carbon cycle over the Pacific, Indian, and Southern oceans. For example, expansions in the dust supply of iron to the ocean may result in a decrease in atmospheric CO2 (Kohfeld et al., 2005). The phytoplankton growth productivity (Tagliabue et al., 2010) of the Southern Ocean strongly relies on the dust deposition from major dust sources; thus, ENSO may indirectly influence the marine productivity and atmospheric CO2 level.

The causal impacts of ENSO on dust deposition over South America (Fig. 1) are consistent with previous studies (Boy and Wilcke, 2008; Shao et al., 2013). Figures 1 and 2 show an agreement with recent works for the potential influences of ENSO on dust activities over regions from the Arabian Peninsula to Central Asia (Huang et al., 2021) and East Asia (Jeong et al., 2018). Substantial influences of ENSO on dust emission over central Australia (Fig. 3) suggest an agreement with earlier work (Marx et al., 2009), while we observe weak causal impacts of ENSO on regional dust emissions of major dust sources (Fig. 3). As the consistency between models is low (Fig. 3), large uncertainties remain for the causal impacts of ENSO on dust emissions. Previous studies indicate the important role of human influences in igniting local dust activities (Duniway et al., 2019; Webb and Pierre, 2018). For example, as anthropogenic land management leads to changes in land surface properties and dust availability (Jickells et al., 2005), an increase in population is likely to intensify dust emission and long-range dust transport (Moulin and Chiapello, 2006). Hence, the impacts of human activities and changes in land use on regional dust emissions might be a topic of future works.

Regarding the consistency across models, the response of dust emission to ENSO is much stronger in the models INM-CM5-0, MIROC-ES2L, and UKESM1_0_LL compared to other models (Fig. 6). This difference might be due to the use of different dust schemes and soil properties in this model, which lead to higher dust emissions (Mulcahy et al., 2020; Zhao et al., 2022). As models use different parameters to estimate dust emissions (Thornhill et al., 2021), this discrepancy leads to low consensus across models in modeling the response of dust emissions to ENSO (Figs. 3 and 6).

5 Conclusions

In this study, we showed that ENSO exhibits significant causal impacts on global dust deposition and transport (Figs. 1, 2, 4, and 5). However, we observed large uncertainty in the causal signatures of ENSO on regional dust emissions of major dust sources (Figs. 3 and 6).

As high-resolution models may improve the simulations of dust emission processes (Knippertz and Todd, 2012) and their connection with ENSO, further studies might use outputs from high-resolution models. Because there is a strong link between dust deposition over ocean and ocean biogeochemistry and carbon cycle (Rap et al., 2018) and there are possible changes in ENSO properties under a warming environment (Cai et al., 2021; Timmermann et al., 2018; Yeh et al., 2018), further works related to ENSO impacts on oceanic carbon cycle are necessary. While there is uncertainty in the projections of global dust deposition (Carslaw et al., 2010) and there is low confidence in projecting dust activities under greenhouse warming (Thornhill et al., 2021), additional studies may focus on the future impacts of ENSO on dust activities.

Data availability

CMIP6 data can be accessed from the ESGF website at https://esgf-node.llnl.gov/search/cmip6/ (ESGF, 2022).

Supplement

The supplement related to this article is available online at: https://doi.org/10.5194/acp-22-5253-2022-supplement.

Author contributions

TL designed the study, performed the data analysis, and wrote the manuscript. DHB contributed to the interpretation of results and the writing of the manuscript.

Competing interests

The contact author has declared that neither they nor their co-authors have any competing interests.

Disclaimer

Publisher’s note: Copernicus Publications remains neutral with regard to jurisdictional claims in published maps and institutional affiliations.

Acknowledgements

The authors thank the anonymous reviewers for their valuable comments and suggestions. We acknowledge the World Climate Research Programme, which through its Working Group on Coupled Modelling, coordinated and promoted CMIP6. We thank the climate modeling groups (listed in Table S1) for producing and making available their model output, the Earth System Grid Federation (ESGF) for archiving the data and providing access, and the multiple funding agencies who support CMIP6 and ESGF. CMIP6 data can be accessed from the ESGF website at https://esgf-node.llnl.gov/search/cmip6/ (last access: 15 December 2021). Thanh Le is supported by the National Research Foundation of Korea (NRF) grant funded by the Korean government (MSIT) (grant no. 2021R1G1A1004389).

Financial support

This research has been supported by the National Research Foundation of Korea (grant no. 2021R1G1A1004389).

Review statement

This paper was edited by Jianping Huang and reviewed by three anonymous referees.

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Here we assess the response of dust activities to El Niño–Southern Oscillation (ENSO) over the 1850–2014 period using climate model outputs. Our results show that ENSO is an important driver of dust deposition and dust transportation with high consensus across models. However, the results indicate that ENSO is unlikely to show causal impacts on dust emissions of major dust sources. This study allows us to obtain further understanding of the linkages between ENSO and dust cycle at a global scale.
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