Materials Map

Discover the materials research landscape. Find experts, partners, networks.

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The Materials Map is an open tool for improving networking and interdisciplinary exchange within materials research. It enables cross-database search for cooperation and network partners and discovering of the research landscape.

The dashboard provides detailed information about the selected scientist, e.g. publications. The dashboard can be filtered and shows the relationship to co-authors in different diagrams. In addition, a link is provided to find contact information.

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Materials Map under construction

The Materials Map is still under development. In its current state, it is only based on one single data source and, thus, incomplete and contains duplicates. We are working on incorporating new open data sources like ORCID to improve the quality and the timeliness of our data. We will update Materials Map as soon as possible and kindly ask for your patience.

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in Cooperation with on an Cooperation-Score of 37%

Topics

Publications (5/5 displayed)

  • 2023Spectroscopic Characterization of Impactites and a Machine Learning Approach to Determine the Oxidation State of Iron in Glass‐Bearing Materials2citations
  • 2011Spitzer Observations of Eta Corvi : Evidence at ~1 Gyr for an LHB-Like Delivery of Organics & Water-Rich Material to the THZ of a Sun-Like Star.citations
  • 2011Spitzer Observations of Eta Corvi : Evidence at ~1 Gyr for an LHB-Like Delivery of Organics & Water-Rich Material to the THZ of a Sun-Like Star.citations
  • 2011Spitzer Observations of Eta Corvi : Evidence at ~1 Gyr for an LHB-Like Delivery of Organics & Water-Rich Material to the THZ of a Sun-Like Starcitations
  • 2011Spitzer Observations of Eta Corvi : Evidence at ~1 Gyr for an LHB-Like Delivery of Organics & Water-Rich Material to the THZ of a Sun-Like Starcitations

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Chart of shared publication
Stojic, Aleksandra
1 / 1 shared
Andreozzi, G. B.
1 / 1 shared
Skogby, H.
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Carli, Cristian
1 / 3 shared
Bruschini, Enrico
1 / 1 shared
Chen, C. H.
4 / 5 shared
Wyatt, M. C.
4 / 6 shared
Thebault, P.
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Watson, D. M.
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Manoj, P.
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Currie, T. M.
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Lisse, C. M.
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Sheehan, P.
4 / 4 shared
Chart of publication period
2023
2011

Co-Authors (by relevance)

  • Stojic, Aleksandra
  • Andreozzi, G. B.
  • Skogby, H.
  • Carli, Cristian
  • Bruschini, Enrico
  • Chen, C. H.
  • Wyatt, M. C.
  • Thebault, P.
  • Watson, D. M.
  • Manoj, P.
  • Currie, T. M.
  • Lisse, C. M.
  • Sheehan, P.
OrganizationsLocationPeople

article

Spectroscopic Characterization of Impactites and a Machine Learning Approach to Determine the Oxidation State of Iron in Glass‐Bearing Materials

  • Stojic, Aleksandra
  • Andreozzi, G. B.
  • Morlok, A.
  • Skogby, H.
  • Carli, Cristian
  • Bruschini, Enrico
Abstract

<jats:title>Abstract</jats:title><jats:p>We investigated a suite of impact glass‐bearing rocks using a multi‐analytical approach including visible‐near‐infrared diffuse reflectance spectroscopy, Mössbauer spectroscopy, and powder X‐ray diffraction. In order to better understand and interpret the obtained results, we built a database containing physical, chemical, and spectroscopic information on glasses and glass‐bearing materials using new results from this study and published works. We used the database to explore systematic relationships between parameters of interest and finally we applied several machine learning algorithms (support vector machine, random forests, and gradient boosting) to test the possibility to regress the oxidation state of iron from chemical and spectroscopic information. Our results show that even small amounts of mafic crystalline phases have a big influence on the spectral features of glass‐bearing rocks. Samples without mafic crystalline inclusions show the typical spectrum of glasses (two broad and shallow bands roughly centered around 1,100 and 1,900 nm) with minor variations due to bulk chemistry. We described a non‐linear relationship between average reflectance (average reflectance value between 500 and 1,000 nm), FeO + TiO<jats:sub>2</jats:sub> content, grain size, and Fe<jats:sup>3+</jats:sup>/Fe<jats:sub>TOT</jats:sub>. We tested the relation for the finer grain size (0–25 μm), and we qualitatively assessed how it is affected by grain size, Fe<jats:sup>3+</jats:sup>/Fe<jats:sub>TOT</jats:sub>, and crystal content. Finally, we developed a machine learning pipeline to regress the Fe<jats:sup>3+</jats:sup>/Fe<jats:sub>TOT</jats:sub> of glass‐bearing materials using the proposed database. Our machine learning calculations give satisfactory results (MAE: 0.0321) and additional data will enable the application of our computational strategy to remotely acquired data to extract chemical and mineralogical information of planetary surfaces.</jats:p>

Topics
  • impedance spectroscopy
  • surface
  • grain
  • inclusion
  • grain size
  • crystalline phase
  • glass
  • glass
  • iron
  • random
  • machine learning
  • Mössbauer spectroscopy
  • microwave-assisted extraction