Introduction
On the surface of buildings in areas sheltered from rainwater, one generally observes the presence of black crusts, which result for the successive deposition of atmospheric particles, followed by their cementation by gypsum. Among the diverse particles encountered, industrial fly ash originating from heavy fuel and/or coal combustion have been evidenced by Del Monte et al. [1], and subsequently systematically detected in numerous black crusts sampled in polluted urban environments [2-6], as well as in marine regions [7, 8]. According to Camuffo et al. [2], the fly ash play an active role in the formation of gypsum cement, since they transport metals such as Fe, Ni, V, that catalyse to heterogeneous oxidation of SO2 into sulphate, in the presence of H2O. This hypothesis was accordingly adopted by other authors [1, 2, 7, 9] and was experimentally verified, in particular by Cheng et al. [10]. Ausset et al. [11] and Sabbioni et al. [12]- Preliminary studies conducted at Tours highlighted the presence of typical fly ash within the black crusts on tuffeau and windows of the Saint-Gatien Cathedral and also in the air and rainwater sampled on the said Cathedral [13-15]. Without disputing the catalytic role of fly ash, we believe ilis important not to neglect the other particles present in the atmosphere.
Thus, the aim of the present article is to characterise the particulate content of the atmosphere in Tours and, in particular, to establish, apart from fly ash , the sources and nature of the particles contributing to the formation of the gypsum cement of the black crusts, such as the sulphates which are generally abundant in urban particles.
Description of the site, sampling and analysis
Description of the site
The city of Tours is situated in the Loire Valley at 230 km from the Atlantic Ocean. The west-east orientation of the valley favours the penetration of oceanic winds.
Sampling
Atmospheric particles were sampled in the city centre, on the first floor of the Psalette Cloister, located on the northern side of the Saint-Gatien Cathedral, at a height of 5 m above the ground. Two sampling campaigns were carried out, one in winter from 3 December to the night of 20 December 1994, the other in summer from 3 July to the night of 5 August 1995.
Black Carbon (BC) concentrations in the air were continuously measured by means of an aethalometer (Magee Scientific, model AE-9) [16]. The pump rate was set at 20 l min-1 and measurements were performed every five minutes. BC concentrations measured by aethalometer method agreed well with particulate elemental carbon measured by thermo/ optical reflectance [17, 18].
The particles were collected by air filtration through polycarbonate membranes of 0.4 µm porosity (Nuclepore®) placed in a tiller support linked to an electric pump (Reciprotor Sweden AB) and to a volumetric counter (Gallus 2000). Thus, all the particles having a diameter superior to 0.4 µm are theoretically collected.
Two air filtration units functioning simultaneously permitted particles to be collected on two series of membranes. The first was employed for global chemical analysis by X-Ray Fluorescence (XRF), the second for the observation and chemical analysis of individual particles by Analytical Scanning Electron Microscopy (ASEM). Two samples were collected every 24 hours, the first during the day (from 7.00 to 21.00 h), the second during the night (from 21.00 to 7.00 h the next morning). The initial pump rate was 5 l min-1 in winter and 8 l min-1 in summer.
The concentrations of particulates (PM10) are now currently measured on five stations in Tours by the air quality network survey Lig'Air [19, 20]. The concentrations of NOx were measured in the city centre, at approximately 800 m south-west of the Cathedral, by the Laboratoire Départemental de Touraine (LDT).
There being no meteorological station within the town walls, the meteorological parameters employed were those measured by the Météo-France station at the Tours-Saint-Symphorien Airport, located 6 km north of the city centre. Wind speed and direction were measured every 3 hours, the duration and density of precipitation every 6 hours and atmospheric pressure reported to sea level every 12 hours.
The trajectographies of the air masses were calculated at Laboratoire Interuniversitaire des Systèmes Atmosphériques (LISA) using the current version of the TM2 model of atmospheric transport initially developed at the Max Planck Institute in Hamburg and modified by Ramonet [21].
Analysis methods
The measurement of the BC concentrations in air is based on the optical measurement of the black body properties of the particles. The aethalometer pumps the air through a quartz fibre filter, measuring at regular intervals the attenuation of the light beam transmitted (530 nm) through the filter. The mass of deposited SC was estimated, alter which the concentration was calculated by dividing the mass by the volume of filtered air.
The overall elemental concentrations of the particles were measured by XRF (SIEMENS SRS 303) with wavelength dispersion over all the first series of membranes (104 filters). This method permits a quantitative elemental analysis of particles since the intensity of fluorescence of an element is proportional to its mass deposited on the tiller, provided that the samples constitute a thin layer. This hypothesis has been confirmed experimentally by the measurement of filter transmission using the « radiator » technique [22]. The masses of the 15 chemical elements (Na, Mg, Al, Si, S, Cl, K, Ca, Ti, V, Cr, Fe, Cu, Zn, Pb) were determined on each filter according to the procedure defined by Quisefit and al. [23].
The individual analysis of particles was carried out on 8 filters (4 for winter, 4 for summer) , on the second series of membrane, by SEM (JEOL JSM 840 A) coupled with an X-Ray energy dispersive spectrometer (TRACOR TN 5400) allowing the detection of elements with atomic number higher than 6 (carbon). However the presence of C can be assumed by the presence of an important background in the spectra. The operative conditions were as follows: accelerating voltage: 15 kV; probe current: 6.10-10 A; working distance: 39 mm; measurement time: 100 s; spectrum acquisition from 0 to 10 keV; dead time between 20 and 25%. The study of the filters, previously made conductors by the deposition of a carbon film, was performed following the protocol described by Chabas and Lefèvre [24] and consisted of observing, measuring and analysing the particles larger than 1 µm present in randomly chosen areas under an enlargement of X 1000. The mineralogical classification of the particles is performed starting from a semi-quantitative analysis of their chemistry and elemental composition, and of their morphology.
Certain particles underwent specific study by means of low intensity field effect SEM (JEOL JSM-6301-F) and Transmission Electron Microscopy (TEM) (JEOL 100 CX II) coupled with a X-Ray energy dispersive spectrometer (respectively, Link ISIS 300 and TRACOR TN 421), which allowed the detection of elements with atomic number greater than 5. The operating conditions chosen for the field effect ASEM were the following: accelerating voltage: 20 kV; probe current: 6.10-10 A; working distance: 15 mm; measurement time: 100 s; spectrum acquisition from 0 to 20 keV; dead time between 20 and 30%. The operating conditions chosen for the ATEM were: accelerating voltage: 100 kV; working distance: 28 mm; tilt: 35 °; measurement time: 100 s; spectrum acquisition from 0 to 10 keV; dead time between 20 and 25%.
Results and discussion
Global chemical and elemental composition of particles
Geometric means and standard deviations
The geometric concentration means and their associated standard deviations were calculated for the BC measured by aethalometry and for 12 elements out of 15 determined by XFS on the 104 filters (Na, Mg, Al, Si, S, Cl, K, Ca, Ti, Fe, Zn and Pb). ln fact, V, Cr and Cu frequently present levels that are below the detection threshold of the spectrometer.
The results presented in Table 1 p. 106 indicate that S, BC and Na are the predominant elements (relative abundance > 10%) and that Si, Ca, Fe, K, Al, Cl and Mg are the minor elements (1% < relative abundance < 10%). The elements Ti, Zn and Pb, which were present in trace (relative abundance < 1%) are not studied below. The geometric standard deviations calculated for each major and minor element are close (variation between 1.85 and 2.94), with the exception of Cl, whose value of 5.22 highlights a strong temporal variability in its concentration.
The mean concentrations measured in Tours are of the same order of magnitude as those measured in other towns in France (Figure 1) and the higher level of S and BC confirms the predominance of anthropic sources in urban sites. The levels of BC in Tours and Arles are, however, far lower than those measured in Paris (4600 ng m-3 according to Brémond et al. [25]; 7900 ng m-3 according Del Delumyea and Kalivretenos [26]). Conversely, the concentration of Na, almost identical to that encountered in Arles, is double in Tours compared to Paris. Thus, the town of Tours seems to undergo, like Arles (some 30 km from the Mediterranean Sea), an oceanic influence, in spite of its relatively great distance from the Atlantic Ocean (230 km).
|
Geometric mean |
Standard deviation |
Relative abundance |
|
|
BC |
1432 |
2.44 |
24 |
|
Na |
853 |
2.54 |
15 |
|
Mg |
126 |
1.99 |
2 |
|
Al |
184 |
2.61 |
3 |
|
Si |
578 |
2.94 |
9 |
|
S |
1662 |
2.32 |
28 |
|
Cl |
169 |
5.22 |
3 |
|
K |
213 |
1.85 |
3 |
|
Ca |
495 |
2.88 |
8 |
|
Fe |
240 |
2.11 |
4 |
|
Ti, Zn, Pb |
24, 42, 86 |
1,74, 2,60, 1,62 |
<1, <1, <1 |
Table 1. Geometric means (ng m-3), standard deviations and relative abundance (%) of major and minor elements of the particles sampled in Tours.
Moyennes géométriques (ng m-3), écarts types géométriques des concentrations et abondance relative ( %) en éléments majeurs et mineurs des aérosols prélevés à Tours.
Figure 1. Comparison of geometric means of elemental concentrations (ng m-3) in particles sampled in Tours [27] , Arles [28] and Paris [29].
Comparaison de la moyenne géométrique des concentrations élémentaires (ng m-3) des particules prélevées à Tours [27], en Arles [28] et à Paris [29].
Enrichment factors
Enrichment factors (EF) allow one to establish the probable origin (marine, terrigenous or other) of the major and minor elements present in the particles, except for BC, which is emitted mainly by anthropogenic sources (fossil fuel or biomass combustion). The EF are calculated according to Mason's earth crust model [30] (1) and Brewer's seawater model [31] (2). Al is taken as reference element for the crustal model and Namarine (Na corrected for its crustal contribution) for the seawater model (3).
ln the results reported in Table 2, one can distinguish three groups of chemical elements:
-
Al, Si and Fe where EFterrigenous is close to 1 and EFmarine high, are exclusively of terrigenous origin;
-
Na, Mg and Cl, where EFmarine is close to 1 (except for Cl) and EFterrigenous high, are mainly of marine origin. According to Eriksson [32], the depletion of Cl in relation to seawater (EFmarine= 0,1) indicates that marine particles such as halite (NaCl) react strongly with the acid compounds present in the air (H2SO4 and HNO3). This chemical reaction leads to the release of HCl to the gaseous state and the enrichment of the particles by sulphates and nitrates;
-
S, K and Ca present high EF regardless of the reference, resulting from the contribution of different sources (terrigenous, marine and others). S is mainly emitted by « other »' sources and partly by the marine source, while K and Ca tend to be of mixed origin (terrigenous, marine) and « other »'.
Table 2. Enrichment factors (EF) of the particles sampled in Tours compared with the crustal model of Mason [30] and the seawater model of Brewer [31].
Facteurs d'enrichissement (FE) par rapport au modèle de croûte de Mason [30] et au modèle d'eau de mer de Brewer [31] des particules prélevées à Tours.
|
Na |
Mg |
Al |
Si |
S |
Cl |
K |
Ca |
Fe |
|
|
EFterrigenous |
13 |
3 |
1 |
1 |
2825 |
573 |
4 |
6 |
2 |
|
EFmarine |
1 |
2 |
1442534 |
4528 |
29 |
0,1 |
9 |
19 |
1830336 |
Seasonal and diurnal evolution of concentrations
Generally speaking, and with the exception of BC, Na and Cl, the concentrations are 2 to 3 limes lower in winter than in summer (Figure 2, p. 108). This is due to the abatement effect of rain, which diminishes the number of suspended particles, a phenomenon more active in winter, when the rainy days are more numerous (68% in winter against 23% in summer) and the ratio of precipitations to the number of days higher (2,5 mm j-1 in winter against 1,2 mm j-1 in summer).
The high winter concentrations of Na and Cl are linked to the presence of winds arriving mainly from the southwesterly sector (Figure 3, p. 108), i.e. of oceanic winds transporting marine particles. ln summer, winds are more frequently continental and follow a northeast to southwest trajectory, corresponding to the direction of the Loire Valley towards Tours.
Element concentrations show two types of diurnal evolution in both seasons: day/night cycle with higher day concentrations for terrigenous chemical elements (example in winter Figure 4, p. 109) and sporadic evolution for marine chemical elements and S (example in winter Figures 5 and 6, p. 109 and 110. Day/night variations seem dependent on the human activity because day variations correspond to the remobilization of deposited dust at night when human activities slow down.
Concentrations of BC are generally higher in winter due to the decrease in the mixing layer height [25] and to the contribution of supplementary sources such as heating plants [33]. The latter hypothesis cannot apply in the present case since the BC, in Tours, is mainly emitted by automobile traffic. ln fact, the profile of its hourly mean concentrations (Figure 7, p. 110) reveals two maxima (9.00 h and 19.00 h) corresponding to automobile rush hour times. Finally, there is a good correlation (R= 0.83) between BC and NOx (Figure 8, p. 111), with the nitrogen oxides in Tours mainly originating from automobiles [27].
Specific study of S
Calculations of contributions
The respective contribution of natural (marine and terrigenous) sources responsible for the measured levels of S is calculated following the method of Marchal [34] using the above-mentioned models.
Smarine= Namarine × (S/Na)seawater
and Sterrigenous = Alaerosol × (S/Al)crustal rock
The contribution of the « other »' or « excess » source in relation to the previous sources is calculated from the difference:
Sexcess = S - (Smarine + Sterrigenous)
Figure 2. Geometric means of elemental concentrations (ng m-3) of particles sampled in Tours in December 1994 (■) and July-August 1995 (□).
Moyennes géométriques des concentrations élémentaires (ng m-3) des particules prélevées à Tours en décembre 1994 (■) et en juillet-août 1995 (□).
Figure 3. Means frequencies of wind directions (°) in Tours in December 1994 (■) and July-August 1995 (□) (Météo-France Data).
Fréquences moyennes des directions des vents (°) à Tours en décembre 1994 (■) et en juillet-août 1995 (□). (Données Météo-France).
Figure 4. Day-night variation of terrigenous elements concentrations (ng m-3) in Tours in December 1994.
Variation jour-nuit des concentrations (ng m-3) en éléments terrigènes à Tours en décembre 1994
Figure 5. Day-night variation of marine elements concentrations (ng m-3) in Tours in December 1994.
Variation jour-nuit des concentrations (ng m-3) en éléments marins à Tours en décembre 1994.
Figure 6. Day-night variation of S concentrations (ng m-3) in Tours in December 1994.
Variation jour-nuit des concentrations (ng m-3) en S à Tours en décembre 1994.
Figure 7. Profile of hourly mean concentrations of BC (ng m-3) measured in Tours in December 1994.
Profil des concentrations moyennes horaires en BC (ng m-3) mesurées à Tours en décembre 1994.
Figure 8. Relation between hourly mean concentrations (ng m-3) of NOx. (Laboratoire Départemental de Touraine, LTD data) and BC measured in Tours in December 1994.
Relation entre les concentrations moyennes horaires (ng m-3) de NOx (Données du Laboratoire Départemental de Touraine, LTD) et de BC mesurées à Tours en décembre 1994.
The results obtained in Tours indicate that the source « in excess » emits most of the S, regardless of the season (90% in winter and 98% in summer), although the contribution of the marine source is far from negligible, especially in winter (10%). The crustal source has only a very weak contribution (< 1%). Thus, S is primarily produced by a gas-particle conversion (SO2-sulphate), which explains why its concentration is higher in summer than in winter. ln fact, the conversion rate is much higher in summer [35], when the heterogeneous oxidation is favoured by significant photochemical activity [36], compared to winter, when oxidation takes place preferentially in a heterogeneous manner in the aqueous phase in the presence of carbonate particles [37, 38].
However, observing the daily variations of marine and « excess » contributions of S, it can be seen that the contribution « in excess » generally prevails over the marine component, although this tendency may be reversed, according to the case [27].
Smarine
Representing Smarine concentrations on a compass card (Figure 9, p. 112), it is clearly seen how, both in winter and summer, the concentrations are great in the south-west quarter (direction between 180 and 270 °) rather than in the remainder of the windrose. The mean concentrations calculated for this wind sector are in the order of 326 ng m-3 in winter against 220 ng m-3 in summer , while they are six time weaker in the remaining sectors (56 ng m-3 in winter and 35 ng m-3 in summer). It is equally clear that the winds in the south-west sector have on average a higher speed (4 m s-1) compared to those of the other sectors (3 m s-1). Finally, the retro-trajectories of air masses, reported by way of example for five winter filters with high levels of Smarine (Figure 10,p. 112), indicate that the air masses arrive directly from the Altantic Ocean where they are loaded with marine particles and that their course over the land is reduced, as well as their passage over high-industrialised regions.
Sexcess
Concentrations of Sexcess remain essentially the same, regardless of wind direction and season (Figure 11, p. 113), indicating that there are no contributions of Sexcess from any particular wind sector and that there are no particular anthropogenic sources. Nevertheless, for the summer campaign, six significant values are observed for the north and north-east wind sector. However, an examination of the wind speeds corresponding to the six samples reveals them to be weak and of the same order as the samples low in Sexcess.
It appears that wind speed has a greater influence on Sexcess concentrations than wind direction since, the greater the wind speed, the smaller the concentration of Sexcess· Figure 12, p. 114, shows that there is an exponential relation (R = 0.80 in winter and R = 0.98 in summer) between wind speed and mean concentrations of Sexcess taking wind speed groups of 1 m s-1.
Finally, especially in winter, high levels of Sexcess are systematically observed for high values of atmospheric pressure. This can be seen in Figure 13, p. 114, which represents the atmospheric pressures associated with mean concentrations of Sexcess taking wind speed group of 1 m s-1. The figure reveals that the level of Sexcess is higher, when wind speed is weaker and the atmospheric pressure is higher. This reflects in fact a strong atmospheric stability characterised by the absence of wind and the presence of high pressure areas. The combination of these two factors is responsible for winter episodes of pollution, causing a considerable increase in the concentration of fine sulphated particles in the air [39].
Figure 9. Concentrations of Smarine (ng m-3) as a function of wind direction (°) for the sampling campaigns conducted in Tours in December 1994 (■) and July-August 1995 (□). (1, 2,3,4,5:December 1994 filters with high Smarine concentrations).
Concentrations du Smarin, (ng m-3) en fonction de la direction du vent (°) pour les campagnes de prélèvement effectuées à Tours en décembre 1994 (■) et en juillet -août 1995 (□). (1, 2. 3. 4, 5 :filtres de décembre 1994 à forte concentration en Smarin·
Figure 10. Retro-trajectories of air masses (at 934 hPa) associated with the December 1994 filters (1,2, 3, 4 and 5) presentîng the highest Smarine concentrations sampled ln Tours.
Rétrotrajectoires des masses d'air (à 934 hPa) associées aux filtres de décembre 1994 (1, 2, 3. 4 et 5) présentant les concentrations en Smarin les plus fortes relevées à Tours.
Single particle analysis by Analytical Scanning Electron Microscopy (ASEM)
Of the total of air filter sampling performed (104), 8 filters (4 in winter, 4 in summer) were selected (Table 3, p. 115) as a function of their respective levels of Smarine and Sexcess for analysis by ASEM. The first group of filters (Group 1) , comprising two winter filters (TA10J, TA10N) and two summer filters (TA49N, TA50J), is characterised by high levels of Smarine but also Na, Mg and Cl, while the second group (Group 2), also comprising two winter filters (TA17J, TA17 N) and two summer filters (TA31N,TA32J), presents very high levels of Sexcess.
The analysed particles were divided into six categories (Table 4, p. 116): marine, terrigenous, mixed marine and terrigenous, S bearing terrigenous, anthropogenic, biogenic (+ undeterminate).
Figure 11. Concentrations of Sexcess (ng m-3) as a function of wind direction (°) for the sampling campaigns conducted in Tours in December 1994 (■) and July-August 1995 (□).
Concentrations du Sexcès (ng m-3) en fonction de la direction du vent (°) pour les campagnes de prélèvement effectuées à Tours en décembre 1994 (■) et en juillet-août 1995 (□).
Figure 12. Relation between mean concentrations of Sexcess (ng m-3) calculated for wind speed groups of 1 m s-1 and the wind speed in Tours in December 1994 (■) and July-August 1995 (□).
Relation entre les concentrations moyennes en Sexcès (ng m-1) calculées par groupe de vitesse de 1 m s-1 et la vitesse du vent à Tours en décembre 1994 (■) et en juillet-août 1995 (□).
Figure 13. Relation between Sexcess concentration (ng m-3) and atmospheric pressure (hPa) (reduced to sea level) in Tours in December 1994 (■) taking groups of wind speed 1 m.s-1.
Relation entre la concentration en Sexcès (ng m-1· ) et la pression atmosphérique (hPa)(réduite au niveau de la mer) à Tours en décembre 1994 (■) par groupe de vitesse de 1 m s-1
Table 3. Sampling conditions and concentrations of Smarine and Sexcess of the eight filters selected for study by Analytical Scanning Electron microscopy (ASEM).
Conditions de prélèvement et concentrations.en Smarin et Sexcès des huit filtres sélectionnés pour l'étude en microscopie electronique analytique en balayage (MEAS).
|
Filters |
Sampling Date |
Wind direction (°) |
Wind speed (m s-1) |
Atmospheric pressure (hPa) |
Smarine |
Sexcess |
|
|
TA10J |
6/12/94 |
187 |
3 |
1022 |
585 |
325 |
|
|
Group |
TA10N |
6‑7/12/94 |
183 |
6 |
1022 |
258 |
328 |
|
1 |
TA49N |
26‑27/7/95 |
220 |
5 |
1017 |
372 |
550 |
|
TA50J |
27/17/95 |
242 |
6 |
1017 |
368 |
486 |
|
|
TA17J |
13/12/94 |
240 |
2 |
1031 |
35 |
3083 |
|
|
Group |
TA17N |
13‑14/12/94 |
246 |
2 |
1028 |
32 |
2920 |
|
2 |
TA31N |
8‑9/7/95 |
50 |
2 |
1015 |
63 |
8090 |
|
TA32J |
9/7/95 |
116 |
2 |
1015 |
21 |
2486 |
The relative proportion or these categories for each filter is reported in Figure 14, p. 117. Group 1 is characterised by the abundance of marine particles (63 to 85%). These particles, entirely absent from Group 2, were .sampled in the depressionary meteorological conditions of the south-west sector, associated with the arrival of oceanic air masses (Figure 7, p. 110, for filter 1: TA10J and filter 2: TA10N) . Group 2 is distinguished by a high proportion of anthropogenic particles (28 to 79%) composed mainly of sulphated particles and, to a lesser extent, by the abundance of S bearing terrigenous particules (8 to 45%). Filter TA17N presents a higher percentage of S bearing terrigenous particles (45%) than of anthropogenic particles (28%). However, if one considers the two categories, the sulphated and S bearing particles are predominant in the filters of Group 2 (72 to 90%). These tilters were collected in a period of strong atmospheric stability characterised by the absence of wind and, particularly in winter, in a strong anti-cyclonic situation.
Table 4, p. 116, presents the elemental chemical composition, the number, the relative abundance, the concentration in number and the possible mineralogical interpretation of analysed particles. The mineralogical interpretation may be subject of discussion in absence of X-Ray diffraction pattern impossible to perform on the filters containing very low mass of particles.
Detailed study of marine particles
Marine particles are composed of equal proportions of chlorides and sulphates (Table 4).
Chlorides are invariably associated with Na and are present in the form of halite (NaCl) crystals which are frequently cubic (Figure 15, p. 118). The crystals are sometimes associated with S and Ca and constitute a mixture of salts composed partly by halite and partly by gypsum (CaSO4 ,2H2O) or anhydrite (CaSO4 ) . Sometimes the halite is associated with Mg, S, K and Ca in traces and forms a mixture which is difficult to interpret mineralogically. Another type of chlorides , far less common than halite, has also been identified as probably consisting of bischofite (MgCl2,6H2O).
Sulphates always contain Ca and are rarely present in the form of pure gypsum or anhydrite but more frequently mixed with other salts. Thus, they are sometime associated with Na, Cl and K, which are present in trace and cannot be identified mineralogically. More often, they are found in the form of oblong particles resembling grains of rice (Figure 16, p.118) of length varying from 1 to 2 µm. They are therefore rich in Na and Cl and also contain traces of Mg and K. The particles appear to be crystals of polyhalite (K2MgCa2(SO4)4 ,2H2O) systematically mixed with halite (NaCl). This association of salts has also been observed in the eastern Mediterranean on the island of Delos [24] in particles of the same morphology. Moreover, the coexistence of polyhalite and halite is common and has been noted in the sequence of salt crystallisation resulting from seawater evaporation [40].
These chlorites and sulphates salts can also be found in groups (Figure 17, p. 119), in this case resulting from the crystallisation of salts contained in the liquid droplets impacting on the filter and subsequently evaporating [41].
Detailed study of anthropogenic particles
Anthropogenic particles are composed mainly of sulphated particles (Table 4) of diameter less than or equal to 1 µm. Such isolated particles can be either spherical or bean-like in shape (Figure 18, p. 119). The superposition of the chemical analysis spectra of the particle and that of the tiller reveals the absence of carbon and the presence of sulphur in the particle (Figure 18). The peak of C is due to the metallisation by carbon and to the polycarbonate filter membrane. Under ATEM, these particles turn out to be little opaque to the electrons and very instable under the electronic beam (Figure 19, p. 120). Very quickly, under the effect of the beam, bubbles appeared inside the particle, which is completely emptied of its contents . Once it has totally vaporised , all that remains is an imprint whose shape is identical to that of the initial particle. Because of this particularity, it was not possible to identify their electron microdiffraction pattern.
Table 4. Elemental chemical composition, number, relative abundance, number concentration and possiblemineralogical interpretation of analysed particles by ASEM on eight filters sampled in Tours.
Composition chimique élémentaire, nombre. abondance relative, concentration en nombre et identification minéralogique possible des particules analysées par MEAB et recueillies par filtration de l'air à Tours sur huit filtres.
Table 4 (continued). Elemental chemical composition, number, relative abundance, number concentration and possible mineralogical interpretation of analysed particles by ASEM on eight filters sampled in Tours
Composition chimique élémentaire, nombre, abondance relative. concentration en nombre et identification minéralogique des particules analysées par MEAB et recueillies par filtration de l'air à Tours sur huit filtres.
Figure 14. Comparison of the proportion of particles according to category for the two groups of filters collected in Tours in December 1994 and July-August 1995 (Group 1: strong concentrations of Smarine; Group 2:strong concentrations of Sexcess·
Comparaison de la proportion de particules selon la catégorie sur les deux groupes de filtres prélevés à Tours en décembre 1994 et en juillet-août 1995 (Groupe 1 ·fortes concentrations en Smarin ; Groupe 2 :fortes concentrations en Sexcès
Figure 15. Cubic halite crystal observed by ASEM. Photo : M. Derbez (LISA).
Cristal de halite de forme cubique observe par MEAS. Photo :M. Derbez (LISA).
Figure 16. Polyhalite crystal with rice-grain shape observed by ASEM. Photo : M.Derbez (LISA).
Cristaux de polyhalite en forme de grains de riz observés par MEAS. Photo ·M. Derbez (LISA).
Figure 17. Accumulation (a) of cubic halite crystals and (b) of oblong polyhalite crystals juxtaposed to a rounded halite particle. This accumulation results from the evaporation of seawater droplets deposited on the filters. Photo : M. Derbez (LISA).
Amas (a) de cristaux cubiques de halite et (b) de cristaux oblongs de polyhalite juxtaposés à une particule arrondie de halite. Ces amas sont issus de l'évaporation de gouttes d'eau de mer déposées sur les filtres. Photo :M Derbez (LISA).
Figure 18. Micronic particles observed by field effect ASEM and superposition of chemical analytical spectra of the top right-hand particle (grey line) and of the filter obtained using a light element detector (black line). The analytical spectra indicate that the particle is sulphated but does not contain carbon. The carbon ray originates from the metallisation and filter. Photo :M. Derbez (LISA).
Particules microniques observées par MEB à effet de champ et superposition des spectres d'analyse chimique de la particule située en haut à droite (en gris) et du filtre (en noir) obtenus à l'aide d'un détecteur à éléments légers. Les spectres d'analyse indiquent que la particule est soufrée mais qu'elle ne contient pas de carbone. La raie du carbone est issue de la métallisation et du filtre. Photo : M. Derbez (LISA).
Figure 19. (a) Micronic particle observed by ATEM sublimated under the electronic beam and (b) imprint left on the filter alter vaporisation of ils contents. Photo : M. Derbez (LISA).
(a) Particule micronique observée par MEAT se sublimant sous le faisceau électronique et (b) empreinte laissée sur le filtre après vaporisation de son contenu. Photo : M. Derbez (LISA).
This type of micronic sulphated particles has already been observed and account for the greater part of the fine aerosol fraction of very many urban sites, such as Antwerp [42], Arles [28], Brest [43], Khartoum [44], Philadelphia [45] and Phoenix [46], but also in rural sites, such as Arizona [47], Maryland [48] and in the vicinity of London [49].They have also been observed by other authors on the Equatorial Pacific Ocean [50], the North Atlantic [51], the Mediterranean Sea [24, 52] and even in Alaska [53]. It is agreed that the said particles are composed of ammonium sulfates produced by the neutralisation of sulphuric acid (H2SO4) by ammonium (NH4+). Charlson and al. [54] emphasises that according to the intensity of this reaction, one observes both mascagnite ((NH4)2SO4 ) once the reaction is complete, and ammonium sulfates of varying acidity, such as (NH4)HSO4 and (NH4)3(HSO4)2. Since the particles observed here are isolated, according to Mamane and Dzubay [48], they are probably mascagnite. The absence of the nitrogen peak on the analysis spectra is due to the rapid deterioration of the particles under the electronic beam and to the weak intensity of the X-rays emitted by the light elements [46, 50, 51]. No localised source of ammonium appears to exist in Tours, although according to Buijsman and al. [55], in Europe, 95% of anthropogenic emissions of ammoniac originate from agricultural activities, mainly animal excrements and, to a lesser extent, fertilizers.
The other categories of anthropogenic particles are, in order of decreasing abundance, carbonaceous particles, metallic residues and smooth microspherules. Carbonaceous particles are encountered in groups or clusters composed of a large number of microspherules of diameter ranging from 0.02 to 0.05 µm and are stable under the electronic beam. These agglomerations of microspherules can reach a size of a dozen or so µm (Figure 20). Their global chemical analysis indicates the presence of an important carbonate matrix associated at times with S, at times with Cl accompanied by traces of Na and S. Such particles are microsoot emitted by petrol-based fossil fuel combustion [56]. They have previously been observed in the atmosphere of Tours [13] and are responsible for the measured levels of BC. Microsoot are the privileged site for the heterogeneous oxidation of SO2 and its conversion into sulphate [38]. Both terrigenous and biogenic particles may play the same role [57-60] and their amount proportion can assume great importance (filter TA17N).
Metallic residues are exclusively ferriferous and of any shape. They are probably emitted by metal-working industries [57], although no such source has been localised in Tours.
Spherical particles (mean diameter: 5 m) always have a smooth surface, but their chemical composition may vary.Some are alumino-silicates and contain significant concentrations of K, Ti and Fe. Others are ferriferous (Figure 21, p. 122), sometimes presenting traces of Al, Si, Ca, S or Ti. These two types of spherules have previously been observed in the air and rain of Tours [13, 14] and are fly-ash emitted by coal [45, 48, 61-64].
Figure 20. Agglomeration of sulphated microsoot observed by ASEM. Photo :M.Derbez (LISA).
Amas de microsuies carbonées et soufrées observé par MEAB. Photo:M. Derbez {LISA).
Figure 21. Smooth hyper-ferriferous fly ash observed by ASEM. Photo : M. Derbez (LISA).
Cendre volante lisse hyperferrifère observee par MEAB. Photo :M. Derbez (LISA).
Conclusion
The study of the particulate content in the atmosphere of Tours was based on the data obtained during two air sampling campaigns (winter and summer) and required the use of aethalometry to measure the BC, X-Ray Fluorescence for the global chemical analysis of particles and ASEM/ATEM for the individual characterisation of particles.
From the results of the study it is possible to affirm that the city of Tours is influenced by two main sources of particles emissions: a marine source marked by the considerable concentrations of Na, Mg, Cl and Smarine and an anthropic source characterised the high levels of Sexcess and BC measured on the site. It follows that the particulate content of the atmosphere varies as a function of the contribution of one or the other of the said sources. It is equally clear how meteorological conditions play an important role: with a depression in the south-west sector, air masses that have stayed over the Atlantic Ocean arrive at Tours, causing an increase in the amount of marine particles in the air (halite or polyhalite crystals, either isolated or in agglomerates). Conversely, in the absence of wind, with strong atmospheric stability, in winter, and only in strongly anticyclonic conditions, the amount of anthropic particles increases. The latter are composed essentially of small isolated particles of ammonium sulphates (principally mascagnite), clusters of sulphated carbonaceous microsoot emitted by automobiles, which are responsible for the measured levels of BC, and finally, a few fly-ash. Sulphate is also associated with terrigenous or biogenic particles.
Thus, the importance of the amount of sulphate particles in relation to other types of particles, as well as their dual origin, must be taken into consideration in order to determine the mechanism of formation of the gypsum cement of the black crusts encountered on the tuffeau and stained glass windows of the Saint-Gatien Cathedral in Tours. However, the constant and significative decrease of the amount of atmospheric sulphur during the last decades leads probably to a subsequent decrease of sulphate particulates and consequently to a decrease of the development of gypseous black crusts.
The present work received the financial support of the Programme Franco-Allemand de Recherche pour la Conservation des Monuments Historiques and of the Programme SESAME of the Ile-de-France Region.
This article was translated by the care of Doctor Lincoln of University of Bologna.
























