SEM/EDS characterisation of dusty deposits in precipitation and assessment of their origin

Detailed scanning electron microscopy/energy dispersive spectroscopy (SEM/EDS) analysis of dusty material in rainfall residue, deposited and collected on February 19th 2014 in Ljubljana, was carried out with the intention to characterise it according to its chemical and mineral composition and to...

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Main Author: Miloš Miler
Format: Article
Language:English
Published: Geological Survey of Slovenia 2014-07-01
Series:Geologija
Subjects:
Online Access:http://www.geologija-revija.si/dokument.aspx?id=1193
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spelling doaj-053bfd42aa5f4607b5f47990b288917a2021-07-02T01:36:37ZengGeological Survey of SloveniaGeologija0016-77891854-620X2014-07-0157151410.5474/geologija.2014.001SEM/EDS characterisation of dusty deposits in precipitation and assessment of their originMiloš MilerDetailed scanning electron microscopy/energy dispersive spectroscopy (SEM/EDS) analysis of dusty material in rainfall residue, deposited and collected on February 19th 2014 in Ljubljana, was carried out with the intention to characterise it according to its chemical and mineral composition and to assess its origin. The material consists of poorly sorted and sharp-edged particles of mostly very fine-grained silt and clay fractions, which is consistent with long-range aerial transport. Particles are represented by illite, chlorite and kaolinite group clay minerals, quartz, feldspars, carbonates, accessory minerals and secondary Fe-oxy-hydroxide minerals. Quantities of minerals and illite/ kaolinite ratio (4.5) correspond to dusts in rainfall residues originating from Moroccan Atlas, while chlorite/kaolinite ratio (2.8) agrees better with dust from central Libya. The element ratios Al/Si, Ca/Al, K/Ca, Mg/Al, Fe/Al and (Ca+Mg)/Fe in the studied dusty deposit are in good agreement with ratios in dusts from rainfall residues originating from Morocco and northern Mauritania. This was also confirmed by the trajectories of cloud movement that caused precipitation with dusty deposit, although the back trajectory HYSPLIT simulation of air masses indicated northern Mauritania, central Niger, southern Algeria, southwestern and central Libya as the most possible source regions.http://www.geologija-revija.si/dokument.aspx?id=1193dusty depositsprecipitationsource areamineral compositionchemical compositionSEM/EDSSlovenia
collection DOAJ
language English
format Article
sources DOAJ
author Miloš Miler
spellingShingle Miloš Miler
SEM/EDS characterisation of dusty deposits in precipitation and assessment of their origin
Geologija
dusty deposits
precipitation
source area
mineral composition
chemical composition
SEM/EDS
Slovenia
author_facet Miloš Miler
author_sort Miloš Miler
title SEM/EDS characterisation of dusty deposits in precipitation and assessment of their origin
title_short SEM/EDS characterisation of dusty deposits in precipitation and assessment of their origin
title_full SEM/EDS characterisation of dusty deposits in precipitation and assessment of their origin
title_fullStr SEM/EDS characterisation of dusty deposits in precipitation and assessment of their origin
title_full_unstemmed SEM/EDS characterisation of dusty deposits in precipitation and assessment of their origin
title_sort sem/eds characterisation of dusty deposits in precipitation and assessment of their origin
publisher Geological Survey of Slovenia
series Geologija
issn 0016-7789
1854-620X
publishDate 2014-07-01
description Detailed scanning electron microscopy/energy dispersive spectroscopy (SEM/EDS) analysis of dusty material in rainfall residue, deposited and collected on February 19th 2014 in Ljubljana, was carried out with the intention to characterise it according to its chemical and mineral composition and to assess its origin. The material consists of poorly sorted and sharp-edged particles of mostly very fine-grained silt and clay fractions, which is consistent with long-range aerial transport. Particles are represented by illite, chlorite and kaolinite group clay minerals, quartz, feldspars, carbonates, accessory minerals and secondary Fe-oxy-hydroxide minerals. Quantities of minerals and illite/ kaolinite ratio (4.5) correspond to dusts in rainfall residues originating from Moroccan Atlas, while chlorite/kaolinite ratio (2.8) agrees better with dust from central Libya. The element ratios Al/Si, Ca/Al, K/Ca, Mg/Al, Fe/Al and (Ca+Mg)/Fe in the studied dusty deposit are in good agreement with ratios in dusts from rainfall residues originating from Morocco and northern Mauritania. This was also confirmed by the trajectories of cloud movement that caused precipitation with dusty deposit, although the back trajectory HYSPLIT simulation of air masses indicated northern Mauritania, central Niger, southern Algeria, southwestern and central Libya as the most possible source regions.
topic dusty deposits
precipitation
source area
mineral composition
chemical composition
SEM/EDS
Slovenia
url http://www.geologija-revija.si/dokument.aspx?id=1193
work_keys_str_mv AT milosmiler semedscharacterisationofdustydepositsinprecipitationandassessmentoftheirorigin
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