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EARLY ONLINE RELEASE

This is a PDF of a manuscript that has been peer-reviewed

and accepted for publication. As the article has not yet been

formatted, copy edited or proofread, the final published

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This pre-publication manuscript may be downloaded,

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Commons Attribution 4.0 International (CC BY 4.0) license.

It may be cited using the DOI below.

The DOI for this manuscript is

DOI:10.2151/jmsj. 2018-023

J-STAGE Advance published date: January 26, 2018

The final manuscript after publication will replace the

preliminary version at the above DOI once it is available.

1

Lidar Network Observation of Dust Layer Development 2

over the Gobi Desert in Association with a Cold Frontal 3

System on 22–23 May 2013 4

5

Kei KAWAI1, Kenji KAI 6

7

Graduate School of Environmental Studies 8

Nagoya University, Nagoya, Japan 9

10

Yoshitaka JIN, Nobuo SUGIMOTO 11

12

National Institute for Environmental Studies 13

Tsukuba, Japan 14

15

and 16

17

Dashdondog BATDORJ 18

National Agency for Meteorology and Environmental Monitoring 19

Ulaanbaatar, Mongolia 20

21

22

23

January 16, 2018 24

25

26

1

------------------------------------ 27

1) Corresponding author: Kei Kawai, Graduate School of Environmental Studies, Nagoya 28

University, Furo-cho, Chikusa-ku, Nagoya 464-8601, Japan. 29

Email: kawai.kei@e.mbox.nagoya-u.ac.jp 30

Tel: +81-52-788-6045 31

Fax: +81-52-789-4257 32

33

Abstract 34

35

The Gobi Desert is one of the major sources of Asian dust, which influences the 36

climate system both directly and indirectly through its long-range transport by the 37

westerlies. In this desert, three ground-based lidars are operated in Dalanzadgad, 38

Sainshand, and Zamyn-Uud, Mongolia. This study firstly combined these lidars into a 39

lidar network and shows the spatial development of a dust layer over the desert and the 40

long-range transport of the dust during 22–23 May 2013 via the lidar network. During this 41

dust event, a cold front accompanying an extratropical cyclone moved southeastward 42

across the desert and sequentially passed through Dalanzadgad, Sainshand, and 43

Zamyn-Uud. In Dalanzadgad, in the central part of the desert, a dust storm occurred 44

owing to the strong wind (6–10 m s-1) associated with the cold front and reached a top 45

height of 1.6 km. Some of the dust floated at a height of 0.9–1.6 km along the cold frontal 46

surface. In Sainshand and Zamyn-Uud, in the eastern part of the desert, the dust layer 47

extended from the atmospheric boundary layer (ABL) to the free troposphere in the 48

updraft region of warm air in the cold frontal system. Overall, while the dust layer was 49

2

moving across the desert with the cold frontal system, it was developing up to the free 50

troposphere. The mechanism of this development can be explained by the combination 51

of two processes as follows: (1) continuous emission of dust from the desert surface to 52

the ABL by the strong wind around the cold front and (2) continuous transport of the dust 53

from the ABL to the free troposphere by the updraft of the warm air in the cold frontal 54

system. This mechanism can contribute to the long-range transport of dust by the 55

westerlies in the free troposphere. 56

57

Keywords Asian dust; cold front; the Gobi Desert; lidar network observation; 58

long-range transport 59

60

3

1. Introduction 61

Asian dust originates in arid and semi-arid regions of East Asia such as the Gobi Desert, 62

Taklimakan Desert, and Loess Plateau (Sun et al. 2001; Kurosaki and Mikami 2005; Wu et 63

al. 2016). In the source regions, dust is emitted from the ground surface to the atmospheric 64

boundary layer (ABL) by strong wind. If the dust ascends from the ABL to the free 65

troposphere, it is transported over a long range toward the North Pacific by the 66

middle-latitude westerlies (Kai et al. 1988; Husar et al. 2001; Hara et al. 2009; Uno et al. 67

2009; Yumimoto et al. 2009). This transported dust influences the climate system both 68

directly and indirectly (Huang et al. 2014). Therefore, the spatial distribution of dust over the 69

source regions is a key factor in the long-range transport of dust. 70

A ground-based lidar is effective for observing vertical distribution of dust continuously. In 71

the Taklimakan Desert, a depolarization lidar was installed in 2002 (Tsunematsu et al. 2005; 72

Kai et al. 2008) through the Japan–China Joint Studies on Origin and Transport of Aeolian 73

Dust and its Impact on Climate (ADEC) (e.g., Mikami et al. 2005; Takemi 2005). In the 74

Loess Plateau, a group from Lanzhou University, China, conducts a lidar observation and 75

many other measurements (Huang et al. 2008). In the Gobi Desert, there are two lidars in 76

the eastern part (Sugimoto et al. 2008) and one in the central part (Kawai et al. 2015). 77

In the Gobi Desert, almost all dust events arise from cold frontal activity (Shao and Wang 78

2003; Takemi and Seino 2005). A cold front often passes through the desert in spring 79

(Hayasaki et al. 2006). This is related to frequent cyclogenesis in the lee of the 80

4

Altai-Hangayn-Sayan Mountains (Fig. 1) in spring (Chen et al. 1991; Adachi and Kimura 81

2007; Wang et al. 2009). Therefore, it is important to understand the relationship between 82

dust events and cold fronts. In previous studies, dust events associated with cold fronts 83

were analyzed via satellite images and numerical models (Husar et al. 2001; Adachi et al. 84

2007; Hara et al. 2009). However, the spatial relationship between dust events and cold 85

fronts, which involves the long-range transport of dust, is not yet shown in detail based on 86

the lidar observations in the source region. 87

A dust event occurred in the Gobi Desert during the passage of a cold front on 22–23 88

May 2013. Our previous study showed the dust transport from the ABL to the free 89

troposphere by the cold frontal system during the dust event, based on the lidar in the 90

central part of the desert (Kawai et al. 2015). In the present study, we firstly combined the 91

three lidars in the desert into a lidar network and analyzed the spatial distribution of dust. 92

The purpose of the present study is to show the spatial development of a dust layer and the 93

long-range transport of the dust during the dust event by using the lidar network. 94

95

2. Observations and data 96

2.1 Gobi Desert lidar network 97

The lidar network in the Gobi Desert consists of three lidars: a ceilometer in the central 98

part and two AD-Net lidars in the eastern part. A ceilometer is a compact backscatter lidar 99

that is easy to operate and maintain. AD-Net is short for the Asian Dust and Aerosol Lidar 100

5

Observation Network, which is a widespread lidar network in East Asia (Sugimoto et al. 101

2008). 102

103

a. Ceilometer observation 104

The ceilometer is located in Dalanzadgad (43.58°N, 104.42°E, 1470 m above sea level 105

(ASL)) in southern Mongolia (Fig. 1). The ceilometer observation has been conducted since 106

the end of April 2013. It is part of the collaborative research between Nagoya University, 107

Japan, and the Information and Research Institute of Meteorology, Hydrology and 108

Environment (IRIMHE), Mongolia. The ceilometer is a Vaisala CL51. The laser wavelength 109

is 910 nm, the pulse repetition rate is 6.5 kHz, and the pulse energy is 3.0 μJ. A preliminary 110

ceilometer observation was carried out in Tsukuba, Japan, and the observational 111

performance of the ceilometer was verified via a sophisticated lidar (Jin et al. 2015). 112

The ceilometer outputs a vertical profile of attenuated backscatter coefficients up to a 113

height of 15.4 km with a height resolution of 10 m every 6 seconds. An attenuated 114

backscatter coefficient is a backscatter coefficient considering the attenuation of an emitted 115

laser pulse and the backscatter light in the atmosphere. The influence of water vapor on the 116

attenuated backscatter coefficients obtained from the ceilometer is probably small because 117

of low relative humidity in the Gobi Desert as discussed in Jin et al. (2015). The average of 118

the data for one minute was used in this study. 119

The major scatterers over the Gobi Desert in spring are dust, clouds, and precipitation. 120

6

Their detection and distinction are based on the magnitude, height, and distribution of 121

attenuated backscatter coefficients. During this dust event, the threshold of attenuated 122

backscatter coefficient for distinguishing dust and the others was about 9 × 10-3 km-1 sr-1. In 123

addition, relative humidity in a region of large attenuated backscatter coefficients supports 124

their distinction. Natsagdorj et al. (2003) showed that relative humidity was low in most dust 125

storms. 126

127

b. AD-Net lidar observations 128

The AD-Net lidars are located in Sainshand (44.87°N, 110.12°E, 937 m ASL) and 129

Zamyn-Uud (43.72°N, 111.90°E, 962 m ASL) in southeastern Mongolia (Fig. 1). These 130

lidars are operated by the National Institute for Environmental Studies (NIES), Japan, and 131

the National Agency for Meteorology and Environmental Monitoring (NAMEM), Mongolia. 132

The lidars are dual-wavelength polarization-sensitive backscatter lidars. The laser 133

wavelengths are 532 and 1064 nm, the pulse repetition rate is 10 Hz, and the pulse energy 134

is 50 mJ. The polarization of backscatter light is measured at a wavelength of 532 nm. 135

The observational data includes the vertical profiles of attenuated backscatter 136

coefficients at both wavelengths and volume depolarization ratio at a wavelength of 532 nm. 137

The time and height resolutions are 15 minutes and 30 m, respectively. The volume 138

depolarization ratio is an index of particle sphericity. This value is zero for a spherical 139

particle and increases with non-sphericity. We calculated volume color ratio, a relative index 140

7

of particle size, by dividing the 1064-nm attenuated backscatter coefficient by the 532-nm 141

one. This value increases as particle size increases. The 532-nm attenuated backscatter 142

coefficient near the ground in Zamyn-Uud was calibrated for an incomplete overlap function 143

by using data on 24 May 2013, when the atmosphere was clean following the dust event. 144

145

2.2 Meteorological data 146

Surface weather charts produced by the Japan Meteorological Agency (JMA) were used. 147

Surface meteorological observational data were obtained from 3-hourly SYNOP reports 148

acquired from the Integrated Surface Database produced by the National Oceanic and 149

Atmospheric Administration (NOAA), USA (Smith et al. 2011). Three-dimensional gridded 150

meteorological data produced by the National Centers for Environmental Prediction (NCEP) 151

of NOAA were used. The data are NCEP FNL (Final) Operational Global Analysis data of 1º 152

1º grids. This product is generated from the global meteorological data of the Global Data 153

Assimilation System (GDAS) using the same model as the NCEP global forecast system. In 154

addition, trajectory analyses were performed using the Hybrid Single-Particle Lagrangian 155

Integrated Trajectory (HYSPLIT) model provided by the NOAA Air Resources Laboratory 156

(Stein et al. 2015). The GDAS data of 1º 1º grids were selected as the input 157

meteorological data of the trajectory analyses. The local standard time (LST) of Mongolia, 158

which is 8 hours ahead of the coordinated universal time (UTC), is used in this paper. 159

160

8

3. Results 161

3.1 Meteorological conditions in Mongolia 162

Surface weather charts for Mongolia on 22–23 May 2013 are shown in Fig. 2. An 163

extratropical cyclone covered central Mongolia at 14 LST on 22 May (Fig. 2a) and moved 164

northeastward for the next 18 hours. The center pressure of the cyclone was almost 165

constant at 988 hPa during this period. Warm and cold fronts accompanied the cyclone 166

from 20 LST on 22 May (Figs. 2b–2d). The cold front extended from the cyclone center to 167

southern Mongolia across the Gobi Desert at 20 LST on 22 May (Fig. 2b) and then moved 168

southeastward through the desert at a speed of about 30 km h-1. During the movement, it 169

passed through Dalanzadgad between 14 and 20 LST on 22 May, Sainshand between 20 170

LST on 22 May and 02 LST on 23 May, and Zamyn-Uud between 02 and 08 LST on 23 171

May. 172

Figure 3 shows the meteorological fields observed around Mongolia at the same time as 173

the second and third weather charts (Figs. 2b and 2c) obtained from the SYNOP report. At 174

20 LST on 22 May, the cold air behind the cold front covered central Mongolia (including 175

Dalanzadgad), and the warm air in front of the cold front covered eastern Mongolia (Fig. 3a). 176

At 02 LST on 23 May, the cold air expanded to eastern Mongolia (including Sainshand) 177

while the cold front moved southeastward (Fig. 3b). At both these times, the wind directions 178

were between north and northwest in the cold air and between south and west in the warm 179

air. These wind conditions show cold and warm air advections. The cold and warm airflows 180

9

converged along the cold front. 181

Figure 4 presents meteorological fields at 700 hPa at the same times as in Fig. 3 182

obtained from the NCEP FNL data. The height at 700 hPa is about 1.5–2.0 km above the 183

ground in Mongolia. At both times in Fig. 4, updrafts spread the warm air in along the 184

surface cold front. These updrafts were caused by the convergence of the cold and warm 185

air on the ground (Fig. 3). Therefore, the warm air on the ground ascended onto the cold air, 186

as shown in the general cold frontal system (e.g., Simpson 1997; Wallace and Hobbs 187

2006). 188

189

3.2 Results in Dalanzadgad, located in the central part of the desert 190

Figure 5 indicates the temporal variations in surface meteorological elements observed in 191

Dalanzadgad from 12 LST on 22 May to 09 LST on 23 May 2013. Figure 6 shows the 192

time-height cross sections of a ceilometer observation result and meteorological conditions 193

obtained from the NCEP FNL data in Dalanzadgad during the same period as in Fig. 5. In 194

Fig. 6, four characteristic regions were discerned and are indicated by the letters A–D. They 195

are discussed as follows. 196

Region A of medium to large attenuated backscatter coefficients (>1.0 × 10-3 km-1 sr-1, 197

light blue to red) shows a dust storm between the ground and a height of 1.6 km from 14 198

LST on 22 May to 02 LST on 23 May (Fig. 6a). Near the ground during the dust storm, the 199

relative humidity was 11–14% (Fig. 5c), and the wind speed was 6–10 m s-1 (Fig. 5d). Thus, 200

10

the strong wind raised the dust from the desert surface. In the dust storm at 20 LST on 22 201

May, the potential temperature was constant at 312 K with height, and the wind speed was 202

12–14 m s-1 (region A in Fig. 6b). The atmospheric neutral stability and the strong wind 203

show that vertical and horizontal mixing was active because of turbulence in the dust storm. 204

The sea level pressure increased by 23.3 hPa from 17 LST on 22 May to 08 LST on 23 205

May (Fig. 5a). The temperature decreased from 28.9 °C at 17 LST on 22 May to 9.4 °C at 206

08 LST on 23 May (Fig. 5b). Hence, the cold front (Fig. 2) passed between 17 and 20 LST 207

on 22 May, and the cold air (Fig. 3) started to advect on the ground during the dust storm. 208

Judging from the potential temperature and wind conditions, the vertical structure of the 209

cold air is shown by region B under the dotted line in Fig. 6b. The sloping top height 210

between 20 LST on 22 May and 01 LST on 23 May was the cold frontal surface. The top 211

height of the cold air is assumed to be about 1.4 km at 02 and 08 LST on 23 May. In 212

particular, the top height at 08 LST corresponds to the cloud base height observed by the 213

ceilometer (Fig. 6a). The potential temperature was 301 K at 02 LST and 294–298 K at 08 214

LST on 23 May (Fig. 6b). The wind directions in and above the cold air were northeast and 215

west, respectively. Most of the cold air indicates small attenuated backscatter coefficients 216

(<0.5 × 10-3 km-1 sr-1, light purple) from 2230 LST on 22 May (Fig. 6a), where little dust was 217

floating. The leading edge of the cold air was occupied by the dust storm. 218

Region C of medium to large attenuated backscatter coefficients (>1.0 × 10-3 km-1 sr-1, 219

red) shows clouds over a height of 1.6 km between 02 and 07 LST on 23 May (Fig. 6a). It is 220

11

likely that the clouds were generated by the updraft of the warm air (Fig. 4), as a general 221

cold frontal system (e.g., Simpson 1997; Wallace and Hobbs 2006). Precipitation is shown 222

by the region of middle to large attenuated backscatter coefficients (>1.0 × 10-3 km-1 sr-1, 223

light blue to red) under the clouds between 05 and 07 LST on 23 May. The precipitation led 224

to the increase in relative humidity at 08 LST on 23 May (Fig. 5c). 225

Region D, which is indicated by medium attenuated backscatter coefficients (1.0–1.4 × 226

10-3 km-1 sr-1, light blue) at a height of 0.9−1.6 km between 22 LST on 22 May and 00 LST 227

on 23 May, shows a dust layer (Fig. 6a). The thickness of the dust layer ranged from 0.2 to 228

0.5 km. Because it was located over the cold frontal surface, the dust was probably 229

transported from the dust storm by the updraft of the warm air (Fig. 4). The subsequent 230

movement of the dust layer will be discussed in Section 4 by using trajectory analysis. 231

232

3.3 Results in Sainshand, located in the eastern part of the desert 233

Figure 7 presents the temporal fluctuations in surface meteorological elements observed 234

in Sainshand in the eastern part of the Gobi Desert from 18 LST on 22 May to 15 LST on 23 235

May 2013. Figures 8 and 9 show the time-height cross sections of lidar observation results 236

and meteorological conditions obtained from the NCEP FNL data, respectively, for 237

Sainshand during the same period as in Fig. 7. 238

Between 22 LST on 22 May and 01 LST on 23 May, a dust storm is shown by region E of 239

large attenuated backscatter coefficients (>5.5 × 10-3 km-1 sr-1, yellow to red) on the ground 240

12

(Fig. 8a). At 23 LST on 22 May, during the dust storm, the wind speed was 11 m s-1 (Fig. 7d), 241

and the relative humidity was 19% (Fig. 7c). In the dust storm, the volume depolarization 242

ratio was 0.2–0.3 (Fig. 8b), and the volume color ratio was about 2.0 (Fig. 8c). 243

The sea level pressure increased by 21.3 hPa from 20 LST on 22 May to 08 LST on 23 244

May (Fig. 7a). The temperature dropped from 35.4 °C at 17 LST on 22 May to 13.3 °C at 08 245

LST on 23 May (Fig. 7b). Between 20 and 23 LST on 22 May, the wind direction changed 246

from south to northwest, and the wind speed increased from 6 to 11 m s-1 (Fig. 7d). 247

According to these features, the cold front shown in Fig. 2 passed through between 20 and 248

23 LST on 22 May, and the cold air replaced the warm air, as shown in Fig. 3. 249

Judging from the potential temperature and wind conditions, the vertical structure of the 250

cold air is indicated in region F below the dotted line in Fig. 9a. The top height was 1.1 km 251

at 02 LST and 1.3 km at 08 and 14 LST on 23 May. The potential temperature was 303–307 252

K at 02 LST and 295 K at 08 and 14 LST on 23 May. At 08 and 14 LST on 23 May, there 253

was an inversion layer between 1.1 and 1.5 km in height. The wind directions in and above 254

the cold air were north and west, respectively. The attenuated backscatter coefficients were 255

small (<2.0 × 10-3 km-1 sr-1, blue) in the cold air after the dust storm (region F in Fig. 8a), 256

indicating little floating dust. 257

Region G of medium to large attenuated backscatter coefficients (>2.0 × 10-3 km-1 sr-1, 258

red) shows clouds, which were located around a height of 2–5 km (Fig. 8a). Most of the 259

clouds indicate volume depolarization ratios of more than 0.2 (Fig. 8b), indicating the 260

13

presence of ice crystals (Shimizu et al. 2004). The temperatures around the clouds were 261

between 0 and -10 °C according to the NCEP FNL data (not shown). Therefore, it is likely 262

that the dust particles mentioned later worked as ice nuclei, as suggested by Sakai et al. 263

(2003). The volume color ratio in the clouds was 2.0–2.4 (Fig. 8c). The region of medium 264

attenuated backscatter coefficients (2.0–6.0 × 10-3 km-1 sr-1, light blue to yellow) under the 265

clouds around 11 LST on 23 May shows precipitation (Fig. 8a). In the precipitation, the 266

volume depolarization ratio was about 0.1 (Fig. 8b), which is consistent with that reported 267

by Sassen (2006). The volume color ratio of the precipitation was 2.0–3.0 (Fig. 8c). 268

A dust layer is shown by the medium attenuated backscatter coefficients (2.0–6.0 × 10-3 269

km-1 sr-1, light blue to yellow) in region H (Fig. 8a). It extended from the dust layer (region E) 270

to the clouds (region G) over the cold air (region F). It seems that the dust layer was mixed 271

with the clouds. The top height of the dust layer increased from 1.6 km at 22 LST on 22 May 272

to at least 4.0 km at 04 LST on 23 May. The presence of the dust layer above a height of 273

4.0 km was unclear because of the clouds. The thickness of the dust layer was between 1.6 274

and 2.5 km. In the dust layer, the volume depolarization ratio was 0.1–0.3 (Fig. 8b), and the 275

volume color ratio was 1.0–2.0 (Fig. 8c). According to the volume color ratio, the dust 276

particles were smaller than the precipitation particles and the ice crystals of the clouds. 277

Vertical velocity represents updraft in the dust layer at 02 LST on 23 May (region H in Fig. 278

9b). Therefore, the dust layer was distributed in the updraft region of the warm air in the 279

cold frontal system. 280

14

281

3.4 Results in Zamyn-Uud, located in the eastern part of the desert 282

The time series of surface meteorological elements observed in Zamyn-Uud on 22–23 283

May 2013 are indicated in Fig. 10. Figures 11 and 12 show the time-height cross sections of 284

the lidar observation results and meteorological conditions obtained from the NCEP FNL 285

data, respectively, for Zamyn-Uud during the same period as in Fig. 10. Three characteristic 286

regions were found and are denoted with the letters I–K. As with Sainshand, a dust layer 287

(region I) was located over the cold air (region J) and probably mixed with a cloud (region 288

K). 289

The dust layer over the cold air is shown by medium attenuated backscatter coefficients 290

(1.6–4.0 × 10-3 km-1 sr-1, light blue to green) up to a height of about 4 km until 17 LST on 23 291

May (region I in Fig. 11a). The top height increased from 1.4 km at 03 LST to 3.8 km at 15 292

LST on 23 May. The thickness ranged from 0.3 to 1.7 km. In the dust layer, the volume 293

depolarization ratio was 0.2–0.3 (Fig. 11b), and the volume color ratio was 1.0–2.4 (Fig. 294

11c). As with Sainshand, the dust layer was located in the updraft region (region I in Fig. 295

12b). 296

The sea level pressure increased by 13.4 hPa from 17 LST on 22 May to 11 LST on 23 297

May (Fig. 10a). The temperature decreased from 32.5 °C at 17 LST on 22 May to 18.4 °C at 298

05 LST on 23 May (Fig. 10b). The wind direction changed from southwest to northwest 299

between 02 and 05 LST on 23 May (Fig. 10d). These characteristics show that the cold 300

15

front (Fig. 2) passed through between 02 and 05 LST on 23 May, and the cold air replaced 301

the warm air (Fig. 3). 302

Judging from the potential temperature and wind conditions, the cold air is indicated by 303

region J below the dotted line in Fig. 12a. The top height of the cold air was about 1.0 km at 304

08 LST and 1.3 km at 14 and 20 LST on 23 May. The potential temperature in the cold air 305

was 297–306 K. The wind directions rotated from north in the cold air to west above the 306

cold air. This counterclockwise rotation is consistent with the cold air advection. The 307

attenuated backscatter coefficients were small (<1.6 × 10-3 km-1 sr-1, blue) in the upper part 308

of the cold air (region J in Fig. 11a). 309

Region K, which is indicated by medium to large attenuated backscatter coefficients 310

(>1.6 × 10-3 km-1 sr-1, red) over a height of 2.2 km between 1700 and 1930 LST on 23 May, 311

shows a cloud (Fig. 11a). It seems that the cloud was mixed with the dust layer. In the cloud, 312

the volume depolarization ratio was mostly greater than 0.3 (Fig. 11b), and the volume color 313

ratio was more than 3.0 (Fig. 11c). As with Sainshand, it is likely that the dust particles 314

worked as ice nuclei. The ice crystals of the cloud were larger than the dust particles based 315

on their color ratios. 316

317

4. Discussion 318

4.1 Dust layer development 319

Figure 13 illustrates the observational models at the lidar observation sites during the 320

16

dust event. The characteristics of the dust layers over the cold air are summarized in Table 321

1. In Dalanzadgad, a dust storm occurred around the cold front and reached a top height of 322

1.6 km (Fig. 13a). A dust layer was distributed at a height of 0.9–1.6 km over the cold air, 323

with a thickness that ranged from 0.2 to 0.5 km. Forward trajectories for the dust layer are 324

presented in Fig. 14. The trajectories extended eastward, reaching the eastern part of the 325

Gobi Desert (Fig. 14a), and ascended to a height of more than 2.0 km for the first 13–15 326

hours (Fig. 14b). The relative humidity along the trajectories was about 50% until 08 LST on 327

23 May (Fig. 14c). In contrast, the dust layers observed in Sainshand and Zamyn-Uud 328

reached a height of about 4 km (Figs. 13b and 13c) and were 1.6–2.5 and 0.3–1.7 km thick, 329

respectively. Therefore, the dust layer produced during this dust event was developing 330

upward from the ABL to the free troposphere while moving eastward through the Gobi 331

Desert with the cold frontal system. 332

It is suggested that the development of the dust layer was based on the combination of 333

the following two processes: (1) the continuous emission of dust from the desert surface to 334

the ABL and (2) the continuous transport of the dust from the ABL up to the free 335

troposphere. 336

Process (1): Dust was raised from the ground to the ABL over the Gobi Desert by the 337

strong wind around the cold front. It is likely that the dust layer was supplied continuously 338

with new dust from the desert surface while moving through the desert. 339

Process (2): The dust in the ABL was transported to the free troposphere by the updraft 340

17

of the warm air in the cold frontal system, as suggested by Kawai et al. (2015). The updraft 341

is shown in Figs. 9b, 12b, and 14b. This transport must have continued while the dust layer 342

was moving through the desert with the cold frontal system. 343

In conclusion, the cold frontal system induced the dust layer development from the ABL 344

up to the free troposphere by the combination of the two processes. This mechanism 345

should have contributed to the long-range transport of the dust by the middle-latitude 346

westerlies. It will be discussed below (Section 4.2) through trajectory analyses. 347

348

4.2 Long-range transport of the dust 349

Forward trajectories for the dust layers observed in Sainshand and Zamyn-Uud are 350

shown in Figs. 15 and 16, respectively. The trajectories extended northeastward or 351

eastward and reached northeastern China and Russian Far East (Figs. 15a and 16a). 352

These directions are consistent with the westerly winds over the cold air (Figs. 9a and 12a). 353

Most of the trajectories extended upward and exceeded a height of 4 km (Figs. 15b and 354

16b). They were located in the free troposphere, where the middle-latitude westerlies 355

prevail. The height increase of these trajectories agrees with the updrafts in the dust layers 356

(Figs. 9b and 12b). Hence, it was caused by the updraft of warm air in the cold frontal 357

system. The relative humidity along the trajectories increased and, at times, exceeded 80% 358

(Figs. 15c and 16c). The high relative humidity indicates the presence of clouds. It is likely 359

that the clouds were generated by the updraft of warm air in the cold frontal system. In 360

18

conclusion, it is suggested that the dust produced during this dust event was transported 361

over a long range by the westerlies, as reported in previous studies (e.g., Kai et al. 1988; 362

Husar et al. 2001; Hara et al. 2009; Uno et al. 2009; Yumimoto et al. 2009). 363

364

5. Conclusions 365

The Gobi Desert lidar network observed the spatial distributions of dust during the dust 366

event that occurred over the desert on 22–23 May 2013. In this study, the dust event was 367

analyzed by using the lidar network and various meteorological data. The main findings are 368

summarized below. 369

(1) During the dust event, a cold front moved southeastward across the desert. 370

(2) In Dalanzadgad, in the central part of the desert, a dust storm was observed around 371

the cold front from the ground to a height of 1.6 km. A dust layer was distributed at a height 372

of 0.9–1.6 km over the cold frontal surface. The updraft of warm air in the cold frontal 373

system should have transported the dust emitted from the dust storm. 374

(3) In Sainshand and Zamyn-Uud, in the eastern part of the desert, a dust layer ascended 375

from the ABL to the free troposphere over the cold air and reached a top height of about 4 376

km. The dust layer was located in the updraft region of warm air. 377

(4) The overall dust layer was developing from the ABL up to the free troposphere while 378

moving across the desert with the cold front. It is suggested that this development was 379

caused by the combination of the continuous emission and transport of dust by the cold 380

19

frontal system. 381

This is the first study showing the spatial development of a dust layer in association with 382

a cold frontal system by using the Gobi Desert lidar network. It is important to maintain and 383

expand the lidar network and analyze many dust events. This effort will help us better 384

understand the mechanisms of the emission and transport of Asian dust. 385

386

Acknowledgments 387

The authors gratefully acknowledge the Dalanzadgad Meteorological Observatory for 388

supporting the ceilometer observation, Dr. Atsushi Shimizu of NIES for teaching the 389

calibration method of the AD-Net lidar data, JMA for the provision of weather charts 390

(http://www.jma.go.jp/jma/), NOAA’s National Climatic Data Center for the provision of ISD 391

data (https://www.ncei.noaa.gov/isd), NCEP for the provision of FNL data 392

(https://rda.ucar.edu/datasets/ds083.2/), and NOAA’s Air Resources Laboratory for the 393

provision of the HYSPLIT transport and dispersion model and the READY website 394

(http://www.ready.noaa.gov). This study was supported by Grants-in-Aid for Scientific 395

Research from JSPS (Nos. 24340111 and 16H02703) and by the JSPS Core-to-Core 396

Program (B. Asia-Africa Science Platforms). 397

398

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489

List of Figures 490

491

Fig. 1 Topographic map of Mongolia and surrounding areas. 492

493

Fig. 2 Surface weather charts for Mongolia at (a) 14 LST and (b) 20 LST on 22 May and at 494

(c) 02 LST and (d) 08 LST on 23 May 2013 provided by JMA. The red dots show the 495

locations of Dalanzadgad (D), Sainshand (S), and Zamyn-Uud (Z). The sparse and 496

dense red-shaded areas indicate altitudes of more than 1500 and 3000 m above sea 497

level, respectively. 498

499

Fig. 3 Potential temperature (red contours; every 3 K) and wind (barbs) observed at (a) 20 500

25

LST on 22 May and (b) 02 LST on 23 May 2013 obtained from the SYNOP report. The 501

half and full barbs represent the wind speeds of 2 and 4 m s-1, respectively. The blue 502

lines indicate the cold fronts transcribed from the weather charts (Figs. 2b and 2c). The 503

blue circles with the letters D, S, and Z show the locations of Dalanzadgad, Sainshand, 504

and Zamyn-Uud, respectively. 505

506

Fig. 4 Temperature (contours; every 3 K) and vertical velocity (color) at 700 hPa at (a) 20 507

LST on 22 May and (b) 02 LST on 23 May 2013 obtained from the NCEP FNL data. For 508

the vertical velocity, a negative value (red) indicates an updraft, whereas a positive value 509

(blue) indicates a downdraft. The green lines indicate the surface cold fronts transcribed 510

from the weather charts (Figs. 2b and 2c). The black dots with D, S, and Z show the 511

locations of Dalanzadgad, Sainshand, and Zamyn-Uud, respectively. 512

513

Fig. 5 Time series of the (a) sea level pressure (SLP), (b) temperature (T), (c) relative 514

humidity (RH), and (d) wind observed in Dalanzadgad from 12 LST on 22 May to 09 LST 515

on 23 May 2013 (after Kawai et al. 2015). The half and full barbs and the pennants 516

represent the wind speeds of 1, 2, and 10 m s-1, respectively. 517

518

Fig. 6 Time-height cross sections of the (a) 910-nm attenuated backscatter coefficient 519

(ABC) observed by the ceilometer (after Kawai et al. 2015) and (b) potential temperature 520

26

(PT) and horizontal wind obtained from the NCEP FNL data for Dalanzadgad during the 521

same period as in Fig. 5. The half and full barbs and pennants represent the wind speeds 522

of 2, 4, and 20 m s-1, respectively. Regions A–D correspond to a dust storm, cold air, 523

clouds, and a dust layer, respectively. The dotted line represents the top of the cold air. 524

525

Fig. 7 Same as Fig. 5, except that the location is Sainshand, and the period is from 18 526

LST on 22 May to 15 LST on 23 May 2013. 527

528

Fig. 8 Time-height cross sections of the (a) 532-nm attenuated backscatter coefficient 529

(ABC), (b) 532-nm volume depolarization ratio (VDR), and (c) 1064/532-nm volume color 530

ratio (VCR) at a height of 0–5 km observed by the AD-Net lidar in Sainshand during the 531

same period as in Fig. 7. Regions E–H correspond to a dust storm, cold air, clouds, and a 532

dust layer, respectively. 533

534

Fig. 9 Time-height cross sections of the (a) potential temperature (PT) and horizontal wind 535

and (b) vertical velocity (VV) and horizontal wind obtained from the NCEP FNL data for 536

Sainshand during the same period as in Figs. 7 and 8. The half and full barbs and 537

pennants represent wind speeds of 2, 4, and 20 m s-1, respectively. Regions F and H are 538

the same as in Fig. 8. 539

540

27

Fig. 10 Same as Fig. 5, except that the location is Zamyn-Uud, and the period is from 00 541

to 21 LST on 23 May 2013. 542

543

Fig. 11 Same as Fig. 8, except that the location is Zamyn-Uud, the height range is 0–4 km, 544

and the period is from 00 to 21 LST on 23 May 2013 (same as in Fig. 10). Regions I–K 545

correspond to a dust layer, cold air, and a cloud, respectively. 546

547

Fig. 12 Same as Fig. 9, except that the location is Zamyn-Uud, and the period is from 00 548

to 21 LST on 23 May 2013 (same as Fig. 10). Regions I and J are the same as in Fig. 11. 549

550

Fig. 13 Observational models for (a) Dalanzadgad, (b) Sainshand, and (c) Zamyn-Uud at 551

a height of 0–4 km during the dust event. The distance was calculated by using the 552

moving speed of the cold front (30 km h-1). The distance of 0 km indicates the leading 553

edge of the cold air (i.e., the cold front on the ground) at each observation site. The right 554

side is the moving direction of the cold front (southeast). The letter P means precipitation. 555

556

Fig. 14 (a) The locations, (b) the height above ground level (AGL), and (c) the relative 557

humidity (RH) of 24-hour forward trajectories of air parcels corresponding to the dust 558

layer that was observed over cold air in Dalanzadgad on 22–23 May 2013. In panel (a), 559

the dots on the trajectories indicate their location every 6 hours, and the numerical values 560

28

of 00 and 12 near the trajectories represent the hours of 00 and 12 LST, respectively. 561

562

Fig. 15 Same as Fig. 14, except that the location is Sainshand. 563

564

Fig. 16 Same as Fig. 14, except that the location is Zamyn-Uud, and the initial time of the 565

forward trajectories is 23 May 2013. 566

567

29

568

569

570

Fig. 1 Topographic map of Mongolia and surrounding areas. 571

572

30

573

574

575

Fig. 2 Surface weather charts for Mongolia at (a) 14 LST and (b) 20 LST on 22 May and at 576

(c) 02 LST and (d) 08 LST on 23 May 2013 provided by JMA. The red dots show the 577

locations of Dalanzadgad (D), Sainshand (S), and Zamyn-Uud (Z). The sparse and 578

dense red-shaded areas indicate altitudes of more than 1500 and 3000 m above sea 579

level, respectively. 580

581

31

582

583

584

Fig. 3 Potential temperature (red contours; every 3 K) and wind (barbs) observed at (a) 20 585

LST on 22 May and (b) 02 LST on 23 May 2013 obtained from the SYNOP report. The 586

half and full barbs represent the wind speeds of 2 and 4 m s-1, respectively. The blue 587

lines indicate the cold fronts transcribed from the weather charts (Figs. 2b and 2c). The 588

blue circles with the letters D, S, and Z show the locations of Dalanzadgad, Sainshand, 589

and Zamyn-Uud, respectively. 590

591

32

592

593

594

Fig. 4 Temperature (contours; every 3 K) and vertical velocity (color) at 700 hPa at (a) 20 595

LST on 22 May and (b) 02 LST on 23 May 2013 obtained from the NCEP FNL data. For 596

the vertical velocity, a negative value (red) indicates an updraft, whereas a positive value 597

(blue) indicates a downdraft. The green lines indicate the surface cold fronts transcribed 598

from the weather charts (Figs. 2b and 2c). The black dots with D, S, and Z show the 599

locations of Dalanzadgad, Sainshand, and Zamyn-Uud, respectively. 600

601

33

602

603

604

Fig. 5 Time series of the (a) sea level pressure (SLP), (b) temperature (T), (c) relative 605

humidity (RH), and (d) wind observed in Dalanzadgad from 12 LST on 22 May to 09 LST 606

on 23 May 2013 (after Kawai et al. 2015). The half and full barbs and the pennants 607

represent the wind speeds of 1, 2, and 10 m s-1, respectively. 608

609

34

610

611

612

Fig. 6 Time-height cross sections of the (a) 910-nm attenuated backscatter coefficient 613

(ABC) observed by the ceilometer (after Kawai et al. 2015) and (b) potential temperature 614

(PT) and horizontal wind obtained from the NCEP FNL data for Dalanzadgad during the 615

same period as in Fig. 5. The half and full barbs and pennants represent the wind speeds 616

of 2, 4, and 20 m s-1, respectively. Regions A–D correspond to a dust storm, cold air, 617

clouds, and a dust layer, respectively. The dotted line represents the top of the cold air. 618

619

35

620

621

622

Fig. 7 Same as Fig. 5, except that the location is Sainshand, and the period is from 18 623

LST on 22 May to 15 LST on 23 May 2013. 624

625

36

626

627

628

Fig. 8 Time-height cross sections of the (a) 532-nm attenuated backscatter coefficient 629

(ABC), (b) 532-nm volume depolarization ratio (VDR), and (c) 1064/532-nm volume color 630

ratio (VCR) at a height of 0–5 km observed by the AD-Net lidar in Sainshand during the 631

same period as in Fig. 7. Regions E–H correspond to a dust storm, cold air, clouds, and a 632

dust layer, respectively. 633

634

37

635

636

637

Fig. 9 Time-height cross sections of the (a) potential temperature (PT) and horizontal wind 638

and (b) vertical velocity (VV) and horizontal wind obtained from the NCEP FNL data for 639

Sainshand during the same period as in Figs. 7 and 8. The half and full barbs and 640

pennants represent wind speeds of 2, 4, and 20 m s-1, respectively. Regions F and H are 641

the same as in Fig. 8. 642

643

38

644

645

646

Fig. 10 Same as Fig. 5, except that the location is Zamyn-Uud, and the period is from 00 647

to 21 LST on 23 May 2013. 648

649

39

650

651

652

Fig. 11 Same as Fig. 8, except that the location is Zamyn-Uud, the height range is 0–4 km, 653

and the period is from 00 to 21 LST on 23 May 2013 (same as in Fig. 10). Regions I–K 654

correspond to a dust layer, cold air, and a cloud, respectively. 655

656

40

657

658

659

Fig. 12 Same as Fig. 9, except that the location is Zamyn-Uud, and the period is from 00 660

to 21 LST on 23 May 2013 (same as Fig. 10). Regions I and J are the same as in Fig. 11. 661

662

41

663

664

665

Fig. 13 Observational models for (a) Dalanzadgad, (b) Sainshand, and (c) Zamyn-Uud at 666

a height of 0–4 km during the dust event. The distance was calculated by using the 667

moving speed of the cold front (30 km h-1). The distance of 0 km indicates the leading 668

edge of the cold air (i.e., the cold front on the ground) at each observation site. The right 669

side is the moving direction of the cold front (southeast). The letter P means precipitation. 670

671

42

672

673

674

Fig. 14 (a) The locations, (b) the height above ground level (AGL), and (c) the relative 675

humidity (RH) of 24-hour forward trajectories of air parcels corresponding to the dust 676

layer that was observed over cold air in Dalanzadgad on 22–23 May 2013. In panel (a), 677

the dots on the trajectories indicate their location every 6 hours, and the numerical values 678

of 00 and 12 near the trajectories represent the hours of 00 and 12 LST, respectively. 679

680

43

681

682

683

Fig. 15 Same as Fig. 14, except that the location is Sainshand. 684

685

44

686

687

688

Fig. 16 Same as Fig. 14, except that the location is Zamyn-Uud, and the initial time of the 689

forward trajectories is 23 May 2013. 690

691

45

692

List of Tables 693

694

Table 1 Summary of the maximum top height and thickness range of the dust layer over 695

cold air observed in each site on 22–23 May 2013. In Sainshand, the presence of the 696

dust layer above a height of 4.0 km was unclear because of clouds. 697

698

699

46

Table 1 Summary of the maximum top height and thickness range of the dust layer over 700

cold air observed in each site on 22–23 May 2013. In Sainshand, the presence of the 701

dust layer above a height of 4.0 km was unclear because of clouds. 702

703

Dust layer Dalanzadgad Sainshand Zamyn-Uud

Maximum top height 1.6 km (4.0 km) 3.8 km

Minimum thickness 0.2 km 1.6 km 0.3 km

Maximum thickness 0.5 km 2.5 km 1.7 km

704

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