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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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 (4/4 displayed)

  • 2022Compositional Effects of Additively Manufactured Refractory High-Entropy Alloys under High-Energy Helium Irradiation20citations
  • 2019Localized corrosion of low-carbon steel at the nanoscale38citations
  • 2017Passivation of Stainless Steel Components for Tritium Containment.citations
  • 2014Thermal and collisional history of Tishomingo iron meteorite: More evidence for early disruption of differentiated planetesimals15citations

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Chart of shared publication
Aitkaliyeva, Assel
1 / 3 shared
Lang, Eric
1 / 6 shared
Wang, Yongqiang
1 / 4 shared
Kustas, Andrew B.
1 / 4 shared
Rodriguez, Sal
1 / 1 shared
Ostraat, Michele L.
1 / 1 shared
Pilyugina, Tatiana S.
1 / 1 shared
Aguiar, Jeffery
1 / 1 shared
Taie, Ihsan M.
1 / 1 shared
Bufford, Daniel C.
1 / 1 shared
Mook, William M.
1 / 2 shared
Kucharski, Timothy
1 / 1 shared
Hayden, Steven C.
1 / 1 shared
Chisholm, Claire
1 / 1 shared
Hattar, Khalid
1 / 6 shared
Grudt, Rachael
1 / 1 shared
Moore, George
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Peebles, Henry C.
1 / 1 shared
Jarek, Russell L.
1 / 1 shared
Bierner, Jessica Anne
1 / 1 shared
Wyrwas, Richard
1 / 3 shared
Gibson, Cory S.
1 / 1 shared
Stein, Edward
1 / 1 shared
Hitchcock, Dale
1 / 1 shared
Muntifering, Brittany
1 / 2 shared
Korinko, Paul
1 / 5 shared
Paisley, Elizabeth A.
1 / 1 shared
Spencer, Bill
1 / 1 shared
Peters, Brent
1 / 2 shared
Grimberg, Ansgar
1 / 3 shared
Scott, Edward R. D.
1 / 1 shared
Goldstein, Joseph I.
1 / 1 shared
Michael, Joseph R.
1 / 3 shared
Leya, Ingo
1 / 3 shared
Yang, Jijin
1 / 3 shared
Chart of publication period
2022
2019
2017
2014

Co-Authors (by relevance)

  • Aitkaliyeva, Assel
  • Lang, Eric
  • Wang, Yongqiang
  • Kustas, Andrew B.
  • Rodriguez, Sal
  • Ostraat, Michele L.
  • Pilyugina, Tatiana S.
  • Aguiar, Jeffery
  • Taie, Ihsan M.
  • Bufford, Daniel C.
  • Mook, William M.
  • Kucharski, Timothy
  • Hayden, Steven C.
  • Chisholm, Claire
  • Hattar, Khalid
  • Grudt, Rachael
  • Moore, George
  • Peebles, Henry C.
  • Jarek, Russell L.
  • Bierner, Jessica Anne
  • Wyrwas, Richard
  • Gibson, Cory S.
  • Stein, Edward
  • Hitchcock, Dale
  • Muntifering, Brittany
  • Korinko, Paul
  • Paisley, Elizabeth A.
  • Spencer, Bill
  • Peters, Brent
  • Grimberg, Ansgar
  • Scott, Edward R. D.
  • Goldstein, Joseph I.
  • Michael, Joseph R.
  • Leya, Ingo
  • Yang, Jijin
OrganizationsLocationPeople

article

Thermal and collisional history of Tishomingo iron meteorite: More evidence for early disruption of differentiated planetesimals

  • Grimberg, Ansgar
  • Kotula, Paul G.
  • Scott, Edward R. D.
  • Goldstein, Joseph I.
  • Michael, Joseph R.
  • Leya, Ingo
  • Yang, Jijin
Abstract

Tishomingo is a chemically and structurally unique iron with 32.5 wt.% Ni that contains 20% residual taenite and 80% martensite plates, which formed on cooling to between -75 and -200 °C, probably the lowest temperature recorded by any meteorite. Our studies using transmission (TEM) and scanning electron microscopy (SEM), X-ray microanalysis (AEM) and electron backscatter diffraction (EBSD) show that martensite plates in Tishomingo formed in a single crystal of taenite and decomposed during reheating forming 10-100 nm taenite particles with ∼50 wt.% Ni, kamacite with ∼4 wt.%Ni, along with martensite or taenite with 32 wt.% Ni. EBSD data and experimental constraints show that Tishomingo was reheated to 320-400 °C for about a year transforming some martensite to kamacite and to taenite particles and some martensite directly to taenite without composition change. Fizzy-textured intergrowths of troilite, kamacite with 2.7 wt.% Ni and 2.6 wt.% Co, and taenite with 56 wt.% Ni and 0.15 wt.% Co formed by localized shock melting. A single impact probably melted the sub-mm sulfides, formed stishovite, and reheated and decomposed the martensite plates. Tishomingo and its near-twin Willow Grove, which has 28 wt.% Ni, differ from IAB-related irons like Santa Catharina and San Cristobal that contain 25-36 wt.% Ni, as they are highly depleted in moderately volatile siderophiles and enriched in Ir and other refractory elements. Tishomingo and Willow Grove therefore resemble IVB irons but are chemically distinct. The absence of cloudy taenite in these two irons shows that they cooled through 250 °C abnormally fast at >0.01 °C/yr. Thus this grouplet, like the IVA and IVB irons, suffered an early impact that disrupted their parent body when it was still hot. Our noble gas data show that Tishomingo was excavated from its parent body about 100 to 200 Myr ago and exposed to cosmic rays as a meteoroid with a radius of ∼50-85 cm....

Topics
  • impedance spectroscopy
  • single crystal
  • scanning electron microscopy
  • transmission electron microscopy
  • forming
  • iron
  • electron backscatter diffraction
  • analytical electron microscopy
  • refractory