Distribution and Mode of Occurrence of Co, Ni, Cu, Zn, As, Ag, Cd, Sb, Pb in the Feed Coal, Fly Ash, Slag, in the Topsoil and in the Roots of Trees and Undergrowth Downwind of Three Power Stations in Poland
Abstract
:1. Introduction
2. Materials and Methods
2.1. Studied Area and Materials
- Area A; high density of pine forests adjoining Kozienice Landscape Park [87]. In this area there are few towns, with a maximum population of 17,500 people. In area A, except PS-a, there are no other industrial emitters of particulates. The power station started operating in 1972. Currently, it generates energy of approximately 4000 MW. The soil samples were collected between 7.7 km and 13.1 km NE, E, and S of the PS-a.
- Area B is burdened with many years of industrial activities (coking plants, hard coal mines, zinc and lead ore mines, steel and zinc works, small PS, chemical plants) and 19 neighboring cities, with a total population of 2.013 million people, forming the Upper Silesian conurbation [88]. PS-b is located in this area, which has been combusting feed coals since 1954; and, currently, it generates energy of approximately 220 MW. In area B, oak and pine trees prevail.The soil samples were collected between 9.9 km and 12.9 km NNE and NE of PS-b.
- Area C includes mainly pine forests adjoining landscape conservation areas (Stobrawa—Turawa Forests, Niemodlin Forests). It includes a few towns and villages with a total population of 9800 people and a few small industry plants [89]. In area C, there is a coal-fired power station (PS-c), operating since 1993, which generates energy of approximately 1500 MW. Opole is located approximately 12 km south of area C (118,300 people). In the area, there were no and there are no metal works and no other power stations. The soil samples were collected at a distance between 5.2 km and 11.1 km NNE and E of PS-c.
2.2. Research Range, Methods, and Calculations
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- The share of grain size classes and of magnetic and nonmagnetic fractions in the fly ash and the share of magnetic and nonmagnetic fraction in the feed coal and the slag in concentrating elements in the whole fly ash, whole feed coal, and whole slag. To do this, the percentage share of each of the components of the weighted average in the total value of the weighted average was calculated. The weighted average component is the product of the element content in each class of fly ash grains and in each slag fraction, as well as the percentage mass share of each class and grain fraction in the composition of whole fly ash and in the whole slag. The calculations were made according to the Equations (1) and (2) and their results are presented in Figure 2 (see Table S1);
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- The share of the horizon/subhorizon of soil (sorted into magnetic and nonmagnetic fractions) in concentrating elements in the whole topsoil of 30 cm thickness. To do this, the percentage share of each of the components of the weighted average was calculated. The component is the product of the content of a given element in each fraction of soil horizon/subhorizon and the percentage share of the weight of each fraction of soil horizon/subhorizon in the composition of the whole topsoil. The total of the components of the weighted average is 100%. The calculations were made according to the Equations (1) and (2) and their results are presented in Figure 3 (see Table S2).
3. Results
3.1. General Petrographic and Geochemical Characteristics of the Subject of the Research
3.2. Distribution and Mode of Occurrence of the Elements in Coal and Combustion Residues
3.3. Distribution and Mode of Occurrence of the Elements in Topsoil and Roots
4. Conclusions
- The hosts of the elements in the feed coal are most often: magnetite, fusinite (mainly with ingrowths or agglomerate with pyrite, carbonates, and clay minerals) together with pyrite and chalcopyrite, followed by siderite, vitrinite (often fused with minerals) and dolomite, present in the magnetic fractions of the feed coal. The highest point of content of the elements was observed in magnetite and cassiterite (Co, Ni, Cu, As, Ag, Cd, Pb), in macerals with siderite (Co, Zn, As, Ag, Cd, Sb, Pb) as well as in pyrite and chalcopyrite (Cu, Zn, and As). The nonmagnetic fraction has the greatest influence on the average content of the elements in the whole feed coal.
- The hosts of the highest content of the elements in the fly ash are microspheres and ferrospheres incrusted with crystals, dendrites and/or iron oxides (mainly of magnetite), and single grains of magnetite (concerns Co, Ni, Cu, Ag, Cd, Sb, and Pb), as well as tenuispheres and crassispheres, cenospheres, and subhedral grains of magnetite (Zn and As), being the main components of the magnetic fraction of the fly ash and the slag. The hosts of the highest content of theelements in the slag are iron oxide on the surface of cenospheres and the crassinetwork, ferrospheres, and iron oxide grains. More rarely the host is is apatite. The biggest influence onthe average content of the elements in the whole fly ash and the whole slag has a group of <0.05 mm nonmagnetic particles of the fly ash and the nonmagnetic fraction of the slag. If the finest solid particles found in the <0.05 mm fraction of the analyzed fly ash are emitted by the power stations, then they were the particles most enriched with Co and Cu (in areas A–C), Ni, Zn and Pb (A, C), As and Sb (C), and Cd (A), in comparison with the feed coal, which reached the analyzed topsoil, whereas the >0.5 mm fly ash particles, enriched mainly with As, Ag, and Cd, were probably separated by the electrostatic precipitators.
- In subhorizon Oi, and secondarily in Oe, the content of theelements is the highest. Most often their hosts are various morphotypes of microspheres and char, emitted by power stations located in large wooded areas (area A and C). The content of Zn, As, Cd, and Pb in each subhorizon/horizon of the topsoil in the area exposed to many years of industrial activities (area B) is greater than in the potentially emitted<0.05 mm particles of the fly ash. It is also greater than in the soil in areas A and C. Together with the power station(PS-b) the main emitters of the elements on the surface of the soil in area B were probably zinc, lead, and ironworks (operating in the past). The values of the enrichment factor for the magnetic fraction of the topsoil are always higher than the for the nonmagnetic fraction. The particles of the topsoil show lower enrichment with Co, Cu, Cd, and Sb and greater enrichment with Ni, Zn, As, Ag, and Pb, than the <0.05 mm particles of the fly ash. The elution of elements accumulated in the several-micron surface layer of sedimenting particles (mainly <0.05 mm), with the use of rainwater or flowing water, can still enrich topsoil with ecotoxic elements.
- The significant enrichment of the topsoil with the elements resulted in an increase in the content of the elements in the roots of trees and undergrowth. In the soil exposed to the long-term emission of the technogenic particles by thermo-emitters (area B), the roots have the highest content of Cu, Zn, Cd, Sb, and Pb, and in the topsoil in the wooded areas with the power station as the only pollution emitter, the roots had the highest content of As (area C) and Ag (area A). The enrichment of the roots with Ci, Ni, Zn, As, Ag, Sb, and Pb is between 0.2 for Co and 41.0 for Cd. It is usually proportional to the increase in the content of the elements in the whole topsoil and the value of the enrichment factor for the topsoil. The highest content of the elements occurs in the tiny roots, especially in the rhizodermis and the primary cortex, more seldom in the axle roller and cortex cells.
- Along the way from the feed coal to the roots, the highest enrichment with elements was observed in the <0.05 mm magnetic (for Co, Ni, Cu, Zn, Cd, Sb, and Pb) and nonmagnetic (Cd, Sb, and Pb)particles of the fly ash; in the >0.5 mm nonmagnetic particles of the fly ash (As and Ag); in the magnetic particles of the slag (Sb), and in the magnetic particles of the soil in subhorizon/horizon Oi (Ni, Cu, and Ag), Oe (Zn, Cd, Sb, and Pb), Ah (Co), and in horizon B (As). A high content of elements in particles of falling dust from power plants, which is potentially dangerous for topsoil and plants, can be significantly reduced by preparing coal which is free from extremely high content of ecotoxic elements. The choice of methods for obtaining such coal will be facilitated by studies of the occurrence and distribution of elements in the feed coal.
Supplementary Materials
Author Contributions
Funding
Institutional Review Board Statement
Informed Consent Statement
Data Availability Statement
Conflicts of Interest
References
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Object/Formula | A | B | C |
---|---|---|---|
(In vol. %) | |||
Vitrinite | 66.0 | 62.8 | 52.0 |
Liptinite | 2.1 | 5.0 | 6.0 |
Inertinite | 11.1 | 22.9 | 23.0 |
Pyrite/FeS2 | 5.8 | 2.0 | 3.8 |
Magnetite/Fe2+Fe3+2O4 | 0.2 | 0.1 | 0.3 |
Hematite/Fe2O3 | <0.1 | <0.1 | not found |
Quartz/SiO2 | 0.1 | 0.1 | 1.4 |
Feldspar/KAlSi3O8-NaAlSi3O8-CaAl2Si2O8 | <0.1 | <0.1 | <0.1 |
Apatite/Ca5(PO4)3(F,Cl,OH | not found | not found | <0.1 |
Chlorite/(X,Y)4–6(Si,Al)4O10(OH,O)8; X and Y = Fe+2, Fe+3, Mg+2, Mn+2, Ni+2, Zn+2, Al+3, Li+1, or Ti+4 | not found | not found | <0.1 |
Kaolinite/Al2Si2O5(OH)4 | 8.8 | 4.0 | 4.1 |
Illite+muscovite/K0.65Al2.0[Al0.65Si3.35O10](OH)2-KAl2(AlSi3O10)(OH)2 | 0.1 | 0.1 | 1.9 |
Calcite/CaCO3/ | not found | not found | not found |
Dolomite/CaMg[CO3]2 | not found | 2.7 | 7.0 |
Ankerite/Ca(Fe2+, Mg, Mn)(CO3)2 | not found | 0.1 | not found |
Siderite/Fe2+CO3 | 5.8 | 0.2 | 0.5 |
Gypsum/CaSO4·2H2O) | not found | not found | not found |
Reflectance (%) | 0.92 | 0.81 | 0.81 |
Ash yield (wt %) | 43.92 | 11.38 | 24.57 |
Element | Object | Sample from Studied Areas | Research Results of Other | PCS ** | ||
---|---|---|---|---|---|---|
A | B | C | Authors * | |||
Co *** | 1 **** | 17.1 | 5.5 | 10.3 | 6.0 ± 0.2 1 | |
2 | 37.6 | 17.9 | 38.5 | 44.6 2, 14.6 3 | ||
3 | 20.4 | 18.3 | 27.5 | 12.0 3, 15 4 | ||
4 | 10.1 | 3.3 | 0.1 | World cambisols 10 5 | 50 | |
Topsoil in the vicinity of the PS | 38.5 16, 4.8 7, 18.0 8, 1.4 9, 0.9 10 | |||||
5 | 2.5 | 2.6 | 0.8 | nd ***** | ||
Ni | 1 | 72.3 | 28.2 | 72.7 | 17 ± 1 1 | |
2 | 123.7 | 58.2 | 111.5 | 138.8 2, 35.5 3, 97.3 11 | ||
3 | 70.5 | 52.6 | 77.4 | 33.2 3 | ||
4 | 15.0 | 7.7 | 1.4 | World cambisols 26 5 | 150 | |
Topsoil in the vicinity of the PS | 52.4 16, 21.8 7, 30.3 8, 2.9 9, 2.4 10, 36.0 12, 3.5 13, 40.4 14, 73 15 | |||||
5 | 40.3 | 8.8 | 4.6 | 1.85 6 | ||
Cu | 1 | 51.0 | 20.4 | 25.8 | 16 ± 1 1 | |
2 | 196.6 | 124.4 | 123.2 | 123.4 2, 72 17 | ||
3 | 106.1 | 101.3 | 63.1 | 35.7 3, 41.0 18 | ||
4 | 10.1 | 9.4 | 2.3 | World cambisols 23 5 | 200 | |
Topsoil in the vicinity of the PS | 70.4 16, 12.3 7, 40.3 8, 1.7 10, 35.6 12, 33.9 14, 0.6 19, 28.0 20, 8.1 21 | |||||
5 | 21.9 | 32.9 | 7.3 | 1.2–3.5 5 | ||
Zn | 1 | 53.9 | 29.6 | 58.9 | 28 ± 2 1 | |
2 | 245.8 | 139.6 | 242.4 | 199.2 2, 282 4,148 18 | ||
3 | 77.1 | 214.3 | 58.7 | 31.7 3, 317 4, 79.0 18 | ||
4 | 48.5 | 221.0 | 17.7 | World cambisols 605 | 500 | |
Topsoil in the vicinity of the PS | 148.5 16, 56.1 7, 124.7 8, 715 9, 0.9 10,33.4 12, 83.0 14, 0.7 19, 34 21 | |||||
5 | 81.9 | 582.7 | 369.7 | nd | ||
As | 1 | 14.4 | 1.1 | 8.3 | 9.0 ± 0.7 1 | |
2 | 13.6 | 3.5 | 28.5 | 28.22, 60.0 17, 24.8 22 | ||
3 | 4.8 | 4.3 | 0.5 | 0.173, 19.6 17, 7.0 22 | ||
4 | 5.0 | 8.4 | 1.8 | World cambisols 8.4 5 | 25 | |
Topsoil in the vicinity of the PS | 3.5 16, 5.1 12, 17.8 13, 6.7 14, <0.1 19, 12.0 20 | |||||
5 | <0.1 | 8.6 | 19.2 | 1.96 6 | ||
Ag | 1 | 0.3 | 0.1 | 0.2 | 0.090 ± 0.016 1 | |
2 | 0.6 | 0.4 | 0.4 | 0.7 2, 0.8 3 | ||
3 | 0.1 | <0.0 | <0.0 | 0.6 23 | ||
4 | 4.4 | 3.0 | 3.5 | World cambisols 0.1 5 | nd | |
Topsoil in the vicinity of the PS | nd | |||||
5 | 3.5 | 1.4 | 2.2 | nd | ||
Cd | 1 | <0.01 | <0.01 | <0.01 | 0.20 ± 0.04 1 | |
2 | 0.52 | 0.37 | 0.83 | 0.9 2, 0.8 3, 0.7 4, 1.3 17 | ||
3 | <0.01 | 1.89 | 0.85 | 0.6 3, 0.5 4, 0.6 17 | ||
4 | 0.03 | 2.55 | 0.07 | World cambisols 0.45 5 | 2.0 | |
Topsoil in the vicinity of the PS | 0.45 5, 1.08 16, 0.33 7, 2.94 9, 0.08 10, 0.69 13, 3.85 14, 0.01 15, 0.58 20, 0.10 21 | |||||
5 | 0.80 | 4.53 | 0.72 | 0.28 6 | ||
Sb | 1 | <0.01 | <0.01 | 0.01 | 1.00 ± 0.09 1 | |
2 | 5.00 | <0.01 | 4.30 | 7.92, 5.8 4, 3.8 17 | ||
3 | <0.01 | 0.61 | 7.03 | 4.3 4, 2.0 17, 0.6 18 | ||
4 | 1.49 | 0.38 | 0.99 | World cambisols 0.62 5 | nd | |
Topsoil in the vicinity of the PS | 1.14 21 | |||||
5 | <0.01 | 4.67 | 0.38 | nd | ||
Pb | 1 | 34.8 | 12.2 | 18.8 | 9.0 ± 0.7 1 | |
2 | 114.3 | 40.3 | 54.2 | 196.8 2, 52.0 3, 48 4, 66.0 7 | ||
3 | 30.2 | 55.3 | 12.4 | 31.0 3, 61 4, 16.3 7, 23.0 10 | ||
4 | 35.2 | 178.2 | 16.5 | World cambisols 28 5 | 200 | |
Topsoil in the vicinity of the PS | 26.6 16, 13.5 7, 39.7 8, 138 9, 1.3 10, 18.9 12, 13.7 13, 46.9 14, 33.7 20 | |||||
5 | 28.2 | 455.8 | 32.6 | 0.1–0.3 16, 11.64 8 |
Element | Area | Feed Coal | Fly Ash | Slag | Topsoil | Root | |||||
---|---|---|---|---|---|---|---|---|---|---|---|
Cn ** | Compound | Cn | Compound | Cn | Compound | Cn | Compound | Cn | Compound | ||
Co | A * | 0.13 | Anhedral pyrite | 0.12 | Al-Si crassisphere with Fe | 0.22 | Apatite on microsphere | 0.34 | Fe-oxide in cenosphere | 0.17 | Primary cortex |
B * | 0.22 | Hematite with siderite | 0.08 | Calcimagnesiaferrosphere | 0.14 | Cenosphere | 0.27 | Ferrosphere | 0.11 | Primary cortex | |
C * | 0.45 | Fusinite with siderite | 0.07 | Fe-oxide on ferrosphere | 0.07 | Al-Si-Fe crassinetwork | 0.34 | Ca-Mg-Fe-Mn carbonate | 0.14 | Rhizodermis | |
Ni | A | 0.17 | Cassiterite with maceral | 0.34 | Fe-oxide on microsphere | 0.27 | Fe-oxide on microsphere | 0.30 | Organic matter | 0.36 | Primary cortex |
B | 1.63 | Hematite skeletal | 0.32 | Fe-oxide on microsphere | 0.16 | Magnetite? grain | 0.39 | Barite | 0.11 | Primary cortex | |
C | 4.44 | iron oxide grain | 0.42 | Fe-oxide on cenosphere | 1.32 | Al-Si-Fe crassinetwork | 3.46 | Siderite after hematite | 0.60 | Primary cortex | |
Cu | A | 1.51 | Cassiterite with maceral | 1.51 | Fe-oxide on cenosphere | 0.22 | Fe-oxide on cenosphere | 0.51 | Fe-oxide in cenosphere | 0.18 | Rhizodermis |
B | 17.61 | Chalcopyrite in siderite | 0.21 | Magnetite? grain | 0.12 | Magnetite? grain | 0.24 | Fe-dendrite on ferrosphere | 0.81 | Axle roller | |
C | 0.33 | Hematite grain | 2.44 | Fe-oxide on ferrosphere | 0.12 | Al-Si-Fe crassinetwork | 0.73 | Ca-Mg-Fe-Mn carbonate | 0.49 | Primary cortex | |
Zn | A | 0.50 | Vitrinite with siderite | 0.11 | Teniusphere with Fe-oxide | 0.60 | Cenosphere | 0.16 | Magnetite in cenosphere | <0.01 | No data |
B | 0.72 | Pyrite in siderite | 0.07 | Si microsphere | 0.01 | No data | 0.31 | Fusinoid | <0.01 | No data | |
C | 0.84 | Siderite grain | 1.23 | Cenosphere | 0.17 | Al-Si-Fe crassinetwork | 0.46 | Hematite in organic | <0.01 | No data | |
As | A | 0.41 | Fusinite with siderite | 0.17 | Crassisphere wit Fe-oxide | 0.29 | Fe-oxide on microsphere | 0.58 | Fe-oxide in cenosphere | <0.01 | No data |
B | 0.12 | Chalcopyrite in siderite | 0.04 | Cenosphere | 0.22 | Calcimagnesiaferrosphere | 0.17 | Ferrosphere | 0.14 | Rhizodermis | |
C | 0.19 | Magnetite massive grain | <0.01 | No data | 0.39 | Al-Si-Fe crassinetwork | 0.52 | Ca-Fe aluminosilicate | <0.01 | No data | |
Ag | A | 0.26 | Cassiterite with maceral | 0.22 | Fe-oxide on Si-microsphere | 0.28 | Fe-oxide in cenosphere | 0.19 | Quartz with organic | 0.22 | Cortex cell |
B | 0.19 | Hematite with siderite | 0.12 | Magnetite? on microsphere | 0.10 | Si-Ca microsphere | 0.28 | Ferrosphere | 0.11 | Axle roller | |
C | 0.65 | Fusinite with siderite | 0.52 | Fe-oxide in cenosphere | 0.60 | Crassinetwork with Fe-oxide | 2.31 | Monazite | 0.04 | Primary cortex | |
Cd | A | 0.35 | Cassiterite | 0.14 | Fe-oxide on cenosphere | 0.21 | Fe-oxide in cenosphere | 0.12 | Fe-oxide on Si-cenosphere | 0.42 | Rhizodermis |
B | 0.29 | Hematite with siderite | 0.23 | Cenosphere | 0.18 | Crassinetwork | 0.24 | Barite | 0.21 | Primary cortex | |
C | 0.61 | Siderite grain | 0.39 | Fe-oxide in cenosphere | 0.44 | Crassinetwork with Fe-oxide | 1.21 | Monazite | 0.37 | Primary cortex | |
Sb | A | 0.53 | Vitrinite with siderite | 0.24 | Fe-oxide on microsphere | 0.36 | Fe-oxide in cenosphere | 0.78 | Organic matter | 0.62 | Primary cortex |
B | 0.34 | Siderite | 0.43 | Magnetite? on microsphere | 0.29 | Ferrosphere | 0.22 | Cenosphere with Fe-oxide | 1.28 | Axle roller | |
C | 0.37 | Fusinite with minerals? | 0.42 | Fe-oxide in cenosphere | 0.28 | Al-Si-Fe crassinetwork | 1.20 | Ca-Mg-Fe-Mn carbonate | 0.52 | Rhizodermis | |
Pb | A | 2.86 | Cassiterite with maceral | 1.37 | Fe-oxide on cenosphere | 1.72 | Fe-oxide on microsphere | 1.47 | Cenosphere | 1.16 | Primary cortex |
B | 1.62 | Hematite with siderite | 0.68 | Cenosphere | 0.69 | Cenosphere | 1.02 | Siderite after hematite | 0.63 | Axle roller | |
C | 3.79 | Siderite grain | 1.07 | Fe-oxide on crassinetwork | 0.47 | Crassinetwork with Fe-oxide | 1.60 | Siderite after hematite | 0.80 | Primary cortex |
Object/PS/Element | Fly Ash | Slag | |||
---|---|---|---|---|---|
>0.5 mm | 0.5–0.2 mm | 0.2–0.05 mm | <0.05 mm | ||
Yield of Magnetic Fraction (wt %) | |||||
PS-a | 0.03 | 1.96 | 3.98 | 26.01 | 15.07 |
PS-b | 0.37 | 1.85 | 11.67 | 6.30 | 7.84 |
PS-c | 0.11 | 3.57 | 6.26 | 2.39 | 10.54 |
Yield of Nonmagnetic Fraction (wt %) | |||||
PS-a | 0.08 | 13.73 | 22.42 | 31.79 | 84.93 |
PS-b | 0.28 | 8.88 | 49.58 | 21.07 | 92.16 |
PS-c | 0.09 | 5.99 | 31.32 | 50.27 | 89.16 |
Fe content in Magnetic Fraction (wt %) | |||||
PS-a | 5.30 | 7.65 | 15.33 | 21.60 | 13.57 |
PS-b | 39.30 | 12.72 | 33.47 | 33.01 | 7.60 |
PS-c | 4.24 | 2.66 | 9.84 | 14.14 | 12.61 |
Content of Unburned Organic Matter in Magnetic Fraction (vol %) | |||||
PS-a | 5 | 4 | <0.5 | <0.5 | 1 |
PS-b | 2 | 6 | <0.5 | <0.5 | <0.5 |
PS-c | 8 | 3 | <0.5 | <0.5 | 4 |
Element Content in Unburned Organic Matter in Magnetic Fraction (wt %) | |||||
PS-a | |||||
Co | 0.07 | no data | no data | 0.02 | 0.11 |
Ni | <0.01 | no data | no data | <0.01 | <0.01 |
Cu | <0.01 | no data | no data | <0.01 | <0.01 |
Zn | 0.08 | no data | no data | <0.01 | 0.60 |
As | 0.15 | no data | no data | <0.01 | 0.08 |
Ag | <0.01 | no data | no data | <0.01 | <0.01 |
Cd | <0.01 | no data | no data | <0.01 | <0.01 |
Sb | <0.01 | no data | no data | 0.26 | 0.15 |
Pb | <0.01 | no data | no data | 0.52 | <0.01 |
PS-b | |||||
Co | <0.01 | no data | <0.01 | <0.01 | 0.14 |
Ni | <0.01 | no data | 0.10 | <0.01 | 0.08 |
Cu | <0.01 | no data | 0.16 | <0.01 | <0.01 |
Zn | <0.01 | no data | <0.01 | <0.01 | <0.01 |
As | <0.01 | no data | <0.01 | <0.01 | <0.01 |
Ag | <0.01 | no data | <0.01 | <0.01 | 0,01 |
Cd | <0.01 | no data | <0.01 | <0.01 | 0.14 |
Sb | <0.01 | no data | <0.01 | <0.01 | <0.01 |
Pb | 0.54 | no data | <0.01 | <0.01 | 0.09 |
PS-c | |||||
Co | <0.01 | 0.10 | no data | 0.02 | <0.01 |
Ni | 0.05 | 0.04 | no data | <0.01 | 0.07 |
Cu | <0.01 | <0.01 | no data | <0.01 | <0.01 |
Zn | <0.01 | <0.01 | no data | <0.01 | 0.13 |
As | <0.01 | <0.01 | no data | <0.01 | 0.28 |
Ag | <0.01 | <0.01 | no data | <0.01 | 0.60 |
Cd | <0.01 | <0.01 | no data | <0.01 | 0.29 |
Sb | <0.01 | <0.01 | no data | 0.26 | <0.01 |
Pb | 0.12 | <0.01 | no data | 0.53 | <0.01 |
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Parzentny, H.R.; Róg, L. Distribution and Mode of Occurrence of Co, Ni, Cu, Zn, As, Ag, Cd, Sb, Pb in the Feed Coal, Fly Ash, Slag, in the Topsoil and in the Roots of Trees and Undergrowth Downwind of Three Power Stations in Poland. Minerals 2021, 11, 133. https://doi.org/10.3390/min11020133
Parzentny HR, Róg L. Distribution and Mode of Occurrence of Co, Ni, Cu, Zn, As, Ag, Cd, Sb, Pb in the Feed Coal, Fly Ash, Slag, in the Topsoil and in the Roots of Trees and Undergrowth Downwind of Three Power Stations in Poland. Minerals. 2021; 11(2):133. https://doi.org/10.3390/min11020133
Chicago/Turabian StyleParzentny, Henryk R., and Leokadia Róg. 2021. "Distribution and Mode of Occurrence of Co, Ni, Cu, Zn, As, Ag, Cd, Sb, Pb in the Feed Coal, Fly Ash, Slag, in the Topsoil and in the Roots of Trees and Undergrowth Downwind of Three Power Stations in Poland" Minerals 11, no. 2: 133. https://doi.org/10.3390/min11020133
APA StyleParzentny, H. R., & Róg, L. (2021). Distribution and Mode of Occurrence of Co, Ni, Cu, Zn, As, Ag, Cd, Sb, Pb in the Feed Coal, Fly Ash, Slag, in the Topsoil and in the Roots of Trees and Undergrowth Downwind of Three Power Stations in Poland. Minerals, 11(2), 133. https://doi.org/10.3390/min11020133