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Multispectroscopic methodology to study Libyan desert glass and its formation conditions

Overview of attention for article published in Analytical & Bioanalytical Chemistry, March 2017
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Title
Multispectroscopic methodology to study Libyan desert glass and its formation conditions
Published in
Analytical & Bioanalytical Chemistry, March 2017
DOI 10.1007/s00216-017-0299-5
Pubmed ID
Authors

Leticia Gomez-Nubla, Julene Aramendia, Silvia Fdez-Ortiz de Vallejuelo, Ainhoa Alonso-Olazabal, Kepa Castro, Maria Cruz Zuluaga, Luis Ángel Ortega, Xabier Murelaga, Juan Manuel Madariaga

Abstract

Libyan desert glass (LDG) is a melt product whose origin is still a matter of controversy. With the purpose of adding new information about this enigma, the present paper analyzes the inner part of LDG specimens and compares them with the results of LDG surfaces. An integrated analytical methodology was used combining different techniques such as Raman spectroscopy, in point-by-point and imaging modes, scanning electron microscopy with X-ray microanalysis (SEM-EDS), energy-dispersive micro X-ray fluorescence spectrometry (μ-EDXRF), electron probe micro analyzer (EPMA), and optical cathodoluminescence (Optical-CL). According to our results, flow structures of the melt and the amorphous nature of the matrix could be discerned. Moreover, the observed displacement of Raman bands, such as in the cases of quartz and zircon, and the identification of certain compounds such as coesite (the most clarifying phase of high pressures), α-cristobalite, gypsum, anhydrite, corundum, rutile, amorphous calcite, aragonite, and calcite allowed us to know that LDGs could be subjected to shock pressures between 6 and more than 30 GPa, and temperatures between 300 and 1470 °C. The differences of temperature and pressure would be provoked by different cooling processes during the impact. Besides, in most cases the minerals corresponding to high pressure and temperatures were located in the inner part of the LDGs, with some exceptions that could be explained because they were trapped subsequently to the impact; there was more than one impact or heterogeneous cooling.Furthermore, nitrogen and oxygen gases were identified inside bubbles, which could have been introduced from the terrestrial atmosphere during the meteorite impact.These data helped us to clarify some clues about the origin of these enigmatic samples.

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Geographical breakdown

Country Count As %
Unknown 20 100%

Demographic breakdown

Readers by professional status Count As %
Professor 3 15%
Researcher 3 15%
Student > Doctoral Student 2 10%
Professor > Associate Professor 2 10%
Student > Ph. D. Student 2 10%
Other 4 20%
Unknown 4 20%
Readers by discipline Count As %
Earth and Planetary Sciences 5 25%
Chemistry 2 10%
Mathematics 1 5%
Business, Management and Accounting 1 5%
Agricultural and Biological Sciences 1 5%
Other 5 25%
Unknown 5 25%
Attention Score in Context

Attention Score in Context

This research output has an Altmetric Attention Score of 1. This is our high-level measure of the quality and quantity of online attention that it has received. This Attention Score, as well as the ranking and number of research outputs shown below, was calculated when the research output was last mentioned on 28 April 2017.
All research outputs
#22,764,772
of 25,382,440 outputs
Outputs from Analytical & Bioanalytical Chemistry
#7,543
of 9,619 outputs
Outputs of similar age
#283,518
of 323,059 outputs
Outputs of similar age from Analytical & Bioanalytical Chemistry
#95
of 146 outputs
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