Pleistocene dust concentrations

Late Pleistocene variations of the background aeolian dust concentration in the Carpathian Basin: an estimate using decomposition of grain-size distribution curves of loess deposits

Original paper: Varga et al. (2012).Late Pleistocene variations of the background aeolian dust concentration in the Carpathian Basin: an estimate using decomposition of grain-size distribution curves of loess deposits. Netherlands Journal of Geosciences – Geologie en Mijnbouw 91. (1–2) pp. 159–171.

Abstract

Aeolian dust deposits can be considered as one of the most important archives of past climatic changes. Alternating loess and paleosol strata display variations of the dust load in the Pleistocene atmosphere. By using the observations of recent dust storms, we are able to employ Late Pleistocene stratigraphic datasets (with accurate chronological framework) and detailed granulometric data for making conclusions on the atmospheric dust load in the past.
Age-depths models, created from the absolute age data and stratigraphic interpretation, allow us to calculate sedimentation rates and dust fluxes, while grain-size specifies the dry-deposition velocity, i.e. the atmospheric residence time of mineral particles. Thus, the dust concentration can be expressed as the quotient of the dust flux and gravitational settling velocity.
Recent observations helped to clarify the mechanisms behind aeolian sedimentation and the physical background of this process has nowadays been well-established. Based on these two, main contrasting sedimentary modes of dust transport and deposition can be recognized: the short suspension episodes of the coarse (silt and very fine sand) fraction and the long-range transport of a fine (clay and fine silt) component. Using parametric curve-fitting the basic statistical properties of these two sediment populations can be revealed for Pleistocene aeolian dust deposits, as it has been done for loess in Hungary. As we do not have adequate information on the magnitude and frequency of the Pleistocene dust storms, conclusions could only be made on the magnitude of continuous background dust load. The dust concentration can be set in the range between 1100 and 2750 μg/m3. These values are mostly higher than modern dust concentrations, even in arid regions. Another interesting proxy of past atmospheric conditions could be the visibility, being proportional to the dust concentration. According to the known empirical dust concentration–visibility equations, its value is around 6.5 to 26 kilometres.


Introduction

The global annual input of mineral dust aerosols, lifted into the atmosphere from deflating surfaces in arid-semiarid regions, is estimated to be between 1 to 3 billion t/y (Tegen et al., 1996; Zender et al., 2003). The magnitude and frequency of these dust storm events are sensitive to environmental changes and climate owing to changing precipitation levels, wind strength, regional moisture balance, and extent of dust sources and also due to anthropogenic factors. 
Dust is an active component of the climate and other environmental systems and plays important role in climate forcing. The atmospheric mineral dust particles reflect, scatter, and absorb the incoming shortwave solar and also the outgoing long wave terrestrial radiation, thereby modifying the Earth’s radiation balance in a direct way (Harrison et al., 2001; Kohfeld & Tegen, 2007; Pósfai & Buseck 2010). However, its indirect effects are also significant. By acting as cloud condensation nuclei, these particles may alter cloud characteristics (e.g. more and smaller cloud droplets, brighter clouds) and also the hydrological cycle (Rosenfeld, 2001; Sassen, 2003). Due to their high Fe-content, dust particles transported to the oceans potentially play an important role in the biogeochemical cycles providing micronutrients and affecting the carbon cycle (Ridgewell, 2002; Jickells et al., 2005). 
Dust particles deposited on land surfaces could accumulate in large quantities, especially during the dustier periods of the Pleistocene glacials. In certain ecological environments, the accumulated dust might form loess via diagenesis. Loess sediments cover ca. 10% of continental surfaces (Pécsi, 1990), and almost the half of Carpathian Basin, where aeolian processes played gradually a more and more dominant role in the sedimentation from the Late Pliocene onwards. These widespread and thick loess-paleosol sequences record the Pleistocene glacial-interglacial variations. By correlating these sequences with ice cores and marine sequences conclusions on the timing and local/regional manifestation of global changes of environmental conditions (e.g. paleotemperature, atmospheric conditions, dust concentration) can be drawn. 
A previous study on Hungarian loess (Varga, 2011) revealed that the grain-size distribution (GSD) curves of loess deposits are bimodal, with a pronounced peak in the coarse silt fraction and a shoulder in the clay-, fine silt fraction. These characteristics have been found common to our formerly analysed aeolian dust deposits in Hungary such as Lower and Middle Pleistocene loess–paleosol and Pliocene–Lower Pleistocene red clays (Kovács, 2008; Kovács et al., 2008; Varga, 2011) and also to other globally investigated terrestrial wind-blown sediments (e.g. Sun et al. 2002, 2004). The bimodal pattern of GSDs represents the mixing of two sediment populations that can be separated from each other by using mathematical methods i.e. fitting appropriate functions). These two populations can be interpreted as the fine-grained continuous background dust-load of the atmosphere and the coarse-grained product of episodic dust storms, by analogy with grain-size data of recent dust observations (McTainsh et al. 1997).
In this study we made an attempt to estimate the average Pleistocene aeolian background dust concentration in the Carpathian Basin by using sedimentation rates and granulometric data from loess-paleosol sequences. These dust-concentration data might be essential for Earth climate system models in evaluating their performances in terms of dust flux reconstruction capabilities.

Materials and methods

Stratigraphy and its relation to the atmospheric dust load

Alternating loess and paleosol strata of aeolian dust deposits mirror the variations of atmospheric dust load in the Pleistocene (Fig. 1.). During the dusty cold-arid glacial periods loess formation prevailed, while in the warmer and moister interglacial/interstadial phases soils were formed on loess by weathering and pedogenic processes. Varga (2011) claims that there was no significant dust input during the formation of the Hungarian Middle and Upper Pleistocene paleosols, based on grain-size data. 

Fig.1. Generalized loess-paleosol sequence of Hungary and its possible correlation with benthic δ18O record of deep sea sediments, and δD and insoluble dust in the EPICA DOME C ice core. (In absence of age data, the correlations of Phe 1-2 and Mtp 1-2 weakly developed sandy and hydromorphic soils with MIS13 and MIS15 carry significant uncertainties. Sources: Pécsi & Schweitzer, 1995; Gábris, 2007; Lisiecki & Raymo, 2005; EPICA community members 2004).

The Upper Pleistocene loess series of Hungary include a pedocomplex that dates to the last interglacial (MF2), early-last-glacial loess, an interstadial pedocomplex (MF1), late-last-glacial loess and the modern, Holocene soil. This stratigraphic feature fits well into the regional picture, shows similarity to the Croatian (Galović et al., 2009), Serbian (Markovic et al., 2006, 2009; Antoine et al., 2009; Stevens et al., 2011) and Austrian (Peticzka et al., 2010) sections. If any of these stratigraphic units is missing, then the series cannot be regarded as a complete sequence (Mahowald et al., 2006).
In the case of poorly dated sections, the low stratigraphic preservation potential of loess sediments, being susceptible to reworking and redeposition by hydrological processes or mass movements, is querying the use of the assumed linear aeolian sedimentation models. The origin of paleosols is another problem of loess stratigraphy; thence sometimes it is difficult to assign the initiation of paleosols in the stratigraphic column since the material from which the soils were formed are glacial loesses and the soil formation proceeded downwards in the section during interglacial periods, so the thickness of the glacial aeolian dust deposits is underestimated in most cases. This was also emphasized in a study focused on other loess-paleosol sequences in Southeastern Europe (e.g. Buggle et al., 2009). Probably, the Lower Pleistocene red paleosols reflect a largely different depositional system, and these paleosols have been formed as vertically-accreted soil direct from the wind-blown dust (Varga, 2011). For these reasons, sections with accurate chronological framework (mostly with two or more independent dating series) and almost complete stratigraphic column were used in our calculations (Table 1.).

Table 1. The list of the sites used in our calculations (source: Újvári et al., 2010).

Site name
Dating method
Stratigraphic/dating framework
Age model
Hungary
Albertirsa
IRSL
21
21
Basaharc
14C, TL, IRSL, AAR
5,23,32,34,36
5,32,34
Bodrogkeresztúr I
14C
30,31,32
30,31,32
Csorgókút I
14C
30,31,32
30,31,32
Csorgókút II
14C
30,31,32
30,31,32
Debrecen (Alföldi brickyard)
14C
30,32
30,32
Dunaszekcső
14C
24,27
24,27
Dunaújváros
14C
24,27
24,27
Katymár
14C
9, 14,30,32,34
30,32,34
Lakitelek I
14C
30,32,34
30,32,34
Látókép
14C
30,32
30,32
Madaras
14C
4,10,30,32,34
4,10,30,32,34
Mende
14C, TL, IRSL, AAR
5,8,23,26,29,35,37
5,8,26,29
Paks
TL, IRSL, AAR
5,23,25,35
5
Ságvár
14C
7,8,12,33
7,8,12
Süttő
AMS 14C, IRSL, AAR
22,23
22
Szeged-Öthalom I
14C
13,30,32
13,30,32
Tápiósüly
14C, TL
8,35
8,35
Tokaj (Kereszt Hill II)
14C
30,32
30,32
Tokaj (Patkó-quarry)
14C
30,31,32
30,31,32
Üveghuta-2 borehole
MS
11,20
11,20
Croatia
Erdut
IRSL
6
6
Zmajevac
IRSL
6
6
Serbia
Batajnica
MS
3,18,19
3,18,19
Crvenka
MS
18
18
Irig
MS, IRSL
17,18
17,18
Mošorin
MS
18
18
Petrovaradin
MS, AAR
15
15
Ruma
MS, AAR
16
16
Stari Slankamen
MS, IRSL-OSL
18,28
28
Surduk
AMS 14C, IRSL-OSL
1
1
Susek
MS
18
18
Titel
MS, IRSL
1,2,18
2
Abbreviations: 14C=conventional radiocarbon dating; AMS 14C=Accelerator Mass Spectrometry radiocarbon dating; TL=thermoluminescence; OSL=optically stimulated luminescence; IRSL=infrared optically stimulated luminescence; AAR=amino acid racemization; MS=magnetic susceptibility

1=Antoine et al. (2009); 2=Bokhorst et al. (2009); 3=Buggle et al. (2009); 4=Dobosi (1967); 5=Frechen et al. (1997); 6=Galović et al. (2009); 7=Gábori-Csánk (1960); 8=Geyh et al. (1969); 9=Hupuczi et al. (2006); 10=Hupuczi & Sümegi (2010); 11=Koloszár & Marsi (2005); 12=Krolopp & Sümegi (2002); 13=Krolopp et al. (1996); 14=Lócskai et al. (2006); 15=Marković et al. (2005); 16=Marković et al. (2006); 17=Marković et al. (2007); 18=Marković et al. (2008); 19=Marković et al. (2009); 20=Marsi et al. (2004); 21=Novothny et al. (2002); 22=Novothny et al. (2009); 23=Oches & McCoy (1995); 24=Pécsi & Pevzner (1974); 25=Pécsi (1979); 26=Pécsi et al. (1979); 27=Pécsi (1985); 28=Schmidt et al. (2009); 29=Seppäla (1971); 30=Sümegi (2005); 31=Sümegi & Hertelendi (1998); 32=Sümegi et al. (2007); 33=Vogel & Waterbolk (1964); 34=Willis et al. (2000); 35=Wintle & Packman (1988); 36=Zöller et al. (1994); 37=Zöller & Wagner (1990).

Grain-size analysis

309 samples from Hungarian key-sites were collected (Fig. 2.), with the focus on sections comprising Upper Pleistocene loess deposits to determine typical granulometric characteristics. The grain-size distribution of all samples was measured after chemical treatment described by Konert & Vandenberghe, (1997). After treating the samples with (10 ml, 30%) H2O2 and (10 ml, 10%) HCl to remove the organic material and the carbonate, 10 ml of 3.6% Na4P2O7·10H2O was added to the samples in order to disperse the particles. All of the measurements were made on a Fritsch Analysette 22 Compact laser grain-size analyser, with 0.3–300 μm measurement ranges and a resolution of 62 channels.

Fig.2. Location of loess profiles considered in the paper. 1 – Süttő; 2 – Basaharc; 3 – Tápiósüly; 4 – Mende; 5 – Albertirsa; 6 – Dunaújváros; 7 – Ságvár; 8 – Paks; 9 – Üveghuta; 10 – Dunaszekcső; 11 – Zók; 12 – Hegyszentmárton; 13 – Beremend; 14 – Bodrogkeresztúr; 15 – Csorgókút I.; 16 – Csorgókút II.; 17 – Tokaj (Patkó-quarry); 18 – Tokaj (Kereszt Hill); 19 – Látókép; 20 – Debrecen (Alföldi brickyard); 21 – Lakitelek; 22 – Szeged-Öthalom; 23 – Madaras; 24 – Katymár; 25 – Zmajevac; 26 – Erdut; 27 – Crvenka; 28 – Susek; 29 – Irig; 30 – Ruma; 31 – Petrovaradin; 32 – Mošorin; 33 – Titel; 34 – Starí Slankamen; 35 – Surduk; 36 – Batajnica. (The 309 samples for the grain-size measurements were collected from Sites 2, 4, 8, 10, 11, 12, 13, 25.).

Estimation of past aeolian dust concentrations

Crucial points in the discussion of past dust concentration are the reliable chronological framework and the sedimentary features of aeolian deposits. The age data, together with the stratigraphy determine the sedimentation rate (i.e. the amount of settled dust), while the grain-size defines the dry deposition velocity of the particles (i.e. the atmospheric residence time of the particles).

Dust flux

The sedimentation rate is defined as:

SR= LLT / DD, (Eq.1.)

where LLT is the layer of loess thickness in meters and DD is the duration of deposition in years. By computing dust fluxes the effect of syn- and post-sedimentary compaction can be compensated for

DF=SR × ρ, (Eq.2.)

where ρ is dry bulk density, and DF represents the mass of deposited dust per unit area per unit time (in g/m2/y). Recently published age and sedimentation rate data and a dry density value of ρ=1.5 g/cm3 (Újvári et al., 2010) have been employed for calculations of DF. Since only weakly developed paleosols and humic horizons intercalate loess deposits in the investigated Upper Pleistocene sections, the same ρ=1.5 g/cm3 dry bulk density has been used for the whole series.

Grain-size and the proportion of background dust-load

According to recent observations, two main sedimentary modes of aeolian dust transport and deposition can be recognized (Pye, 1987, 1995): larger particles are transported by surface winds in short suspension episodes, during discontinuous dust storms, smaller grains disperse to higher levels of the atmosphere and are transported by upper level air flows far from the source area as continuous back-ground dust load. However, it is worth noting that in some cases even the larger particles can transported far away from their source areas (Stuut et al. 2009). The two main modes of dust entrainment can also be identified in the bimodal GSDs of aeolian dust deposits (Sun et al., 2002, 2004; Varga, 2011 – Fig. 3.). 


Fig.3. Typical grain-size distribution curves of Upper Pleistocene loess samples from the Carpathian Basin.

The separation of these sediment populations can be made by different mathematic techniques, including parametric curve-fitting (PCF) and end-member modelling algorithms (EMMA – Weltje, 1997; Weltje & Prins, 2003; Vriend & Prins, 2005). We believe that the differences (Weltje & Prins 2007) between these two methods arise from their different approach and scope. Whereas EMMA is based on the simultaneous analysis of the whole sequence based on the covariance structure of the dataset, the input of the PCF is only one sample. The resulting (and generally) three EMMA end-members of loess samples (Prins & Vriend, 2007; Prins et al., 2007) represent the average dust GSD of three temporal aeolian sediment clusters of seasonal or other short-term intervals. In the case of loess deposits, the PCF populations are proposed to illustrate the background and the local-derived dust components for each sample. The process-related partitioning of EMMA end-members could justify the supposed differences of results of the two methods (Fig. 4.).

Fig.4. Possible relationship of different mathematical methods to partitioning grain-size distribution curves: End-Member Modelling Algorithm (EMMA) and the Parametric Curve-Fitting (PCF) methods.

In this study, as it is aimed at providing information on the amount of background dust load, the PCF technique has been applied. According to this approach the bimodal GSDs can be interpreted as the sum of two overlapping Weibull functions (Sun et al., 2002, 2004). It must be emphasized here concerning the Weibull distribution that the wind speed at a given site also follows this continuous probability distribution (Lun & Lam 2000), and it is expected that the GSDs of wind-blown sediments should reflect the transport agent. The applied distribution function has a form of:


where W1 and W2 are the two sediment populations, α1 and α2 are the shape parameters, defining the kurtosis of the curves (i.e. the sorting), β1 and β2 are the location parameters, defining the position of the curves (i.e. the grain-size), while c1 and c2 are weighting parameters. Iterative numerical methods were used to determine the location, shape and weight parameters as a least-squares problem, and to assess the appropriate goodness of fit of the measured and calculated data (Fig.5.).

Fig.5. Typical measured (a) and mathematically partitioned (b) grain-size distribution curves of loess samples from the Carpathian Basin.

Dust concentration

For Late Pleistocene dust concentration calculations only the continuous background dust component of the grain-size distribution curves were used, owing to the unknown magnitude and frequency of Pleistocene dust storm events. The relatively short duration of dust storms and short atmospheric residence time of storm-related coarse particles could be the source of significant uncertainties in calculations.
Dust flux represents the mass of deposited dust per unit area per unit time, so its quotient by the gravitational settling velocity (vs) will give the average atmospheric dust concentration (C):

C [μg/m3] = DF / vs. (Eq.4.)

The gravitational settling velocity, vs, for spherical particles larger than 1 μm can be calculated approximately according to the Stokes Law as a function of the square of the grain diameter:


where d is the grain diameter, δ is the particle density, g is gravity, η is the dynamic viscosity of air. The typical grain diameter of the background dust is given by:


where xi is the measurement range of the ith channel of the laser analyser, mi is the mass proportion of particles related to the background dust population in the ith channel. The gravitational settling velocities for different sizes of quartz (2.65 g/cm3) in still air are shown in Fig.6.

Fig.6. Gravitational settling velocities of different sizes of quartz particles in still air.

After these calculations, the dust concentration (C) can be expressed as


a function of the dust flux and the grain-size related gravitational settling velocity.

Results and discussion

The average sedimentation rate in the Carpathian Basin for the Late Pleistocene can be set in the range 0.1 to 0.95 m/ky with a median value of 0.23 m/ky and a mean of 0.28 m/ky (Újvári et al., 2010). According to (Eq.2.), the dust flux values related to the above sedimentation rates are 150 to ~1400 g/m2/y with median and mean values of 338 and 417 g/m2/y, in general (the range of the first and third quartile) between 200 and 500 g/m2/y (Table 2.). The 0.95 m/ky sedimentation rate and 1400 g/m2/y dust flux of the Paks site is exceptionally high, which was possibly caused by the activation of additional source areas. However, this observation needs further investigations since the GSDs were similar to granulometric characteristics of other sections.
Due to the low stratigraphic preservation potential of loess deposits, being susceptible to reworking and redeposition, reconstructed sedimentation-rate values depend on the geomorphological settings of the investigated sections. The DF values were found by Újvári et al. (2010) to be higher on loess plateaus and river terraces than on hill slopes and alluvial plains.
The bimodal grain-size distribution curves of the collected samples were mathematically partitioned into sediment populations. Statistical parameters of the separated components proved to be more useful for describing and analysing the samples than traditional statistical measures such as mean grain size, etc. The dust storm-related coarse-grained (7–71 μm) sediment population has positive skewness and leptokurtic kurtosis, i.e. the material is well sorted: it represents the dust material of local source areas (e.g. alluvial plains of Danube, Tisza and other rivers – Buggle et al., 2008; Újvári et al., 2008). In contrast to other well-studied regions (e.g. Chinese Loess Plateau), it is difficult to draw conclusions from GSDs to source-to-sink distances in the Carpathian Basin, due to the complex system of many local sources (Bokhorst et al., 2011).
Skewness of the fine-grained (2.1–7.8 μm) component produced by the background dust load, is also positive, but the kurtosis is platykurtic, poorly sorted. The proportion of the background-dust population varied between 12.65% and 17.95%, the typical grain size ranged from 4.1 to 4.4 μm. Further, the grain size of the fine-grained populations did not show large differences; their average GSD illustrates well the regional features of background dust load (Fig. 7.).

Fig.7. Sedimentary populations of the decomposed bimodal grain-size distribution curve.

Based on the relationship (Eq.7.) between dust concentration, dust flux and gravitational settling velocity, the calculated value of the background dust concentration can be set in the range of 1100 to 2750 μg/m3 if we count with regionally typical 200–500 g/m2/y dust fluxes. Decomposition results are detailed in Table 2. Because of the usage of average GSD, a correction coefficient of ±20% must be applied.

Table 2. Average Late Pleistocene sedimentation rates, dust flux and dust concentration values in the Carpathian Basin (source of the SR and DF values for the bulk samples: Újvári et al., 2008).

Site name
Bulk sample
Fine-grained population
SR [m/ky]
DF [g/m2/y]
SR [m/ky]
DF [g/m2/y]
C [μg/m3]
Hungary
Albertirsa
0,39
587
0,05–0,07
74,3–105,4
1489–2113
Basaharc
0,23
348
0,03–0,04
44–62,5
878–1246
Bodrogkeresztúr I
0,25
381
0,03–0,04
48,2–68,4
955–1355
Csorgókút I
0,19
284
0,02–0,03
35,9–51
726–1030
Csorgókút II
0,3
453
0,04–0,05
57,3–81,3
1146–1626
Debrecen (Alföldi brickyard)
0,16
237
0,02–0,03
30–42,5
611–867
Dunaszekcső
0,47
707
0,06–0,08
89,4–126,9
1795–2547
Dunaújváros
0,83
1238
0,1–0,15
156,6–222,2
3170–4498
Katymár
0,42
632
0,05–0,08
79,9–113,4
1604–2276
Lakitelek I
0,17
254
0,02–0,03
32,1–45,6
649–921
Látókép
0,14
212
0,02–0,03
26,8–38,1
535–759
Madaras
0,25
375
0,03–0,04
47,4–67,3
955–1355
Mende
0,51
761
0,06–0,09
96,3–136,6
1948–2764
Paks
0,95
1422
0,12–0,17
179,9–255,2
3628–5148
Ságvár
0,12
176
0,02–0,02
22,3–31,6
458–650
Süttő
0,39
584
0,05–0,07
73,9–104,8
1489–2113
Szeged-Öthalom I
0,22
332
0,03–0,04
42–59,6
840–1192
Tápiósüly
0,34
504
0,04–0,06
63,8–90,5
1298–1842
Tokaj
(Kereszt Hill)
0,15
222
0,02–0,03
28,1–39,8
573–813
Tokaj
(Patkó-quarry)
0,22
332
0,03–0,04
42–59,6
840–1192
Üveghuta-2
0,23
338
0,03–0,04
42,8–60,7
878–1246
Croatia
Erdut
0,14
215
0,02–0,03
27,2–38,6
535–759
Zmajevac
0,29
437
0,04–0,05
55,3–78,4
1107–1571
Serbia
Batajnica
0,22
329
0,03–0,04
41,6–59,1
840–1192
Crvenka
0,13
197
0,02–0,02
24,9–35,4
496–704
Irig
0,13
192
0,02–0,02
24,3–34,5
496–704
Mošorin
0,26
395
0,03–0,05
50–70,9
993–1409
Petrovaradin
0,12
174
0,02–0,02
22–31,2
458–650
Ruma
0,13
192
0,02–0,02
24,3–34,5
496–704
Stari Slankamen
0,11
168
0,01–0,02
21,3–30,2
420–596
Surduk
0,29
434
0,04–0,05
54,9–77,9
1107–1571
Susek
0,1
150
0,01–0,02
19–26,9
382–542
Titel
0,34
510
0,04–0,06
64,5–91,5
1298–1842

These values match and many times exceed the present-day background dust concentration values, even in arid, dusty regions (e.g. Gillies et al., (1996) have observed 755 μg/m3 suspended, background dust concentration in Sevaré, Mali). Still, during severe dust storms the concentration of the particles can exceed 104–105 μg/m3 (Pye, 1987). Ganor & Foner (2001) have measured 23 000 μg/m3 dust concentration in the Negev, while Gillies et al., 1996 have reported more than 13 000 μg/m3 in the Sahara. However, the concentrations of dust, even during intensive dust outbreaks, rarely reach the 1000 μg/m3 value at the Canary Islands (Querol et al., 2004) or at Cape Verde (Jaenicke & Schütz, 1978). The highest "total dust concentration" ever recorded in Australia was measured at the Birdsville station with a value of 29 000 μg/m3/y (McTainsh et al., 2009). (The total dust concentration was defined as the sum of the daily dust concentration values.) But the magnitude and frequency of Pleistocene dust storms is unknown, conclusions can be made only on the magnitude of continuous background dust load.
As the visibility is strongly dependent on dust concentration (e.g. Chepil & Woodruff, 1957), we are allowed to compute Late Pleistocene visibility from our calculated dust concentration data. Below are some of the empirical relationships derived by fitting dust concentration measurements to visibility, and the opposite way:


where C is the dust concentration [μg/m3] and Vis is the visibility in kilometres. According to Shao (2008), the differences of (Eq.8.1–8.4) were caused by (1) small data sets; (2) effects of grain size and humidity; and (3) subjectivity. However, it could be interesting to know more about the visibility relations of the Late Pleistocene, also in regard to other disciplines. From the viewpoint of archaeology, the limited view distance made the orientation, hunting and communication of the prehistoric societies more difficult.
The results of (Eq.8-3) and (Eq.8-4) provided too low visibility values (<5 km) even at relatively low dust concentration (<200 μg/m3). So, the Chepil–Woodruff and the Patterson–Gillette formulas were used in our calculations. However these results have shown some differences as well, therefore their combined minimum and maximum were chosen as limits of average visibility (Fig. 8).

Fig.8. Relationship between the dust concentration and the visibility by Chepil & Woodruff, (1957) and Patterson & Gillette, (1977), and the estimated range of the Pleistocene dust concentration.

Based on the above-mentioned relationships, the average Late Pleistocene visibility can be set in the range between 6.5 to 26 kilometres. According to the World Meteorological Organization’s protocol, these values can be classified into dust-in-suspension and blowing dust categories. However, these values are averages and related only to the background dust load. During severe Late Pleistocene dust storms the visibility could certainly drop to almost zero.

Conclusions

Aeolian dust deposits can be considered as one of the most important archive of past environmental and climatic changes. The well-dated loess-paleosol sequences from the Carpathian Basin reflect the Pleistocene glacial-interglacial changes. By using the sedimentary data of these deposits; conclusions can be made on the atmospheric dust load, especially for the last glacial period.
The detailed grain-size measurements and the mathematical methods allow us to separate the different sedimentation modes of dust particles. According to Pye (1987) the fine-grained sediment population was formed during the almost continuous deposition of the background dust with relatively long atmospheric residence time. The background dust concentration can be expressed as the function of stratigraphic and sedimentary parameters: as the quotient of dust flux and gravitational settling velocity.
By using published data on sedimentation rate and dust flux for Upper Pleistocene loess deposits (Újvári et al., 2010) and average loess grain-size properties (determined from the several hundred collected samples) the dust concentration can be set in the range between 1100 and 2750 μg/m3. These values are mostly higher than modern dust concentrations, even in arid regions. Another interesting proxy of past atmospheric conditions could be the visibility, being proportional to the dust concentration. According to the known empirical dust concentration–visibility equations, its value is around 6.5 to 26 kilometres. These values, however, are only averages and relate to the background dust load, i.e. intense Late Pleistocene dust storms could reduce the visibility close to zero. This means that the aeolian dust might have affected past environments and the everyday life of humans and animals as well.

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