Orange Snow—A Saharan Dust Intrusion over Romania During Winter Conditions
Autor: | Mihai Boldeanu, Bogdan Antonescu, Oana Cadar, Dragos Ene, Cătălin Viţelaru, Erika Andrea Levei, Cristina Marin, Simona Andrei, Jeni Vasilescu, Luminiţa Mărmureanu |
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Jazyk: | angličtina |
Rok vydání: | 2019 |
Předmět: |
Calcite
010504 meteorology & atmospheric sciences Single-scattering albedo 010501 environmental sciences Mineral dust Snow Atmospheric sciences 01 natural sciences Saharan dust snow deposition chemical composition physical properties chemistry.chemical_compound Mediterranean sea chemistry saharan dust General Earth and Planetary Sciences Environmental science lcsh:Q Clay minerals lcsh:Science Chemical composition Quartz 0105 earth and related environmental sciences |
Zdroj: | Remote Sensing, Vol 11, Iss 21, p 2466 (2019) Remote Sensing; Volume 11; Issue 21; Pages: 2466 |
ISSN: | 2072-4292 |
Popis: | On the morning of 23 March 2018, an unusual phenomenon was observed over Romania where the southeastern part of the country was covered in a fresh-layer of orange snow. The event was extensively reported in mass-media and social-media and raised questions about the origin and the possible impact of the orange snow. Even if this type of events, intrusions of Saharan dust, have been reported before in Romania, and in Europe in general, their occurrence during negative temperature conditions is very rare. Saharan dust intrusion occurs over Europe mainly during spring and, in general, is not accompanied by snow at low altitudes. In this article, for the first time, the synoptic-scale conditions leading to the Saharan dust intrusion over Romania and the chemical and physical properties of the deposited dust particles in a snow layer were analyzed. The Saharan dust event affected a permanent atmospheric measurement research infrastructure located southwest of Bucharest, the capital city of Romania. In-situ and remote sensing measurements conducted at this research infrastructure allowed the identification of the dust source as the north Sahara. The source was confirmed by the elemental ratios of the main components (e.g., Al, Ca, Mg, Fe, K). For example, the (Ca+Mg)/Fe ratio of 1.39 was characteristic for the north Sahara. The dust morphology and the minerals were analyzed by scanning electron microscopy with energy disperse X-ray spectrometry (SEM/EDX). The size distribution of the particle geometric diameter showed that they are centred on 1 μ m, but larger particles up to 40 μ m are also present. To visualize the minerals, an approach was developed which emphasized the presence of the calcite, quartz or clay minerals. The optical parameters of dust were measured by re-suspending the particles. Values of the optical parameters (i.e., asymmetry parameter at 550 nm was 0.604, single scattering albedo was 0.84−0.89) were similar to those measured for Saharan dust intrusions over the Iberian Peninsula. Also, the non-refractory particles found in the dust-contaminated snow layer were analyzed, indicating the presence of HULIS-like compounds, most probably advected from the Mediterranean sea. |
Databáze: | OpenAIRE |
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