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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1.080 Topics available

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977 Locations available

693.932 PEOPLE
693.932 People People

693.932 People

Show results for 693.932 people that are selected by your search filters.

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PeopleLocationsStatistics
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in Cooperation with on an Cooperation-Score of 37%

Topics

Publications (2/2 displayed)

  • 2019The Thermal, Mechanical, Structural, and Dielectric Properties of Cometary Nuclei After Rosetta91citations
  • 2006Spitzer Spectral Observations of the Deep Impact Ejecta319citations

Places of action

Chart of shared publication
Tosi, F.
1 / 5 shared
Ciarletti, V.
1 / 5 shared
Skorov, Y.
1 / 1 shared
Filacchione, G.
1 / 3 shared
Pelivan, I.
1 / 1 shared
Marshall, D.
1 / 1 shared
Knollenberg, J.
1 / 1 shared
Knapmeyer, M.
1 / 1 shared
Gundlach, B.
1 / 1 shared
Fischer, H.-H.
1 / 1 shared
Davidsson, B.
1 / 1 shared
Brouet, Y.
1 / 5 shared
Attree, N.
1 / 1 shared
Leyrat, C.
1 / 4 shared
Snodgrass, Colin
1 / 1 shared
Kokotanekova, Rosita
1 / 1 shared
Kührt, E.
1 / 1 shared
Spohn, T.
1 / 7 shared
Vancleve, J.
1 / 1 shared
Adams, A. C.
1 / 1 shared
Mcfadden, L. A.
1 / 2 shared
Belton, M. J. S.
1 / 1 shared
Grillmair, C. J.
1 / 1 shared
Ingalls, J.
1 / 1 shared
Farnham, T. L.
1 / 2 shared
Ahearn, M. F.
1 / 1 shared
Fernández, Y. R.
1 / 1 shared
Clark, B. C.
1 / 3 shared
Schultz, P. H.
1 / 1 shared
Meech, K. J.
1 / 1 shared
Sunshine, J. M.
1 / 1 shared
Lisse, C. M.
1 / 7 shared
Feaga, L. M.
1 / 1 shared
Chart of publication period
2019
2006

Co-Authors (by relevance)

  • Tosi, F.
  • Ciarletti, V.
  • Skorov, Y.
  • Filacchione, G.
  • Pelivan, I.
  • Marshall, D.
  • Knollenberg, J.
  • Knapmeyer, M.
  • Gundlach, B.
  • Fischer, H.-H.
  • Davidsson, B.
  • Brouet, Y.
  • Attree, N.
  • Leyrat, C.
  • Snodgrass, Colin
  • Kokotanekova, Rosita
  • Kührt, E.
  • Spohn, T.
  • Vancleve, J.
  • Adams, A. C.
  • Mcfadden, L. A.
  • Belton, M. J. S.
  • Grillmair, C. J.
  • Ingalls, J.
  • Farnham, T. L.
  • Ahearn, M. F.
  • Fernández, Y. R.
  • Clark, B. C.
  • Schultz, P. H.
  • Meech, K. J.
  • Sunshine, J. M.
  • Lisse, C. M.
  • Feaga, L. M.
OrganizationsLocationPeople

article

Spitzer Spectral Observations of the Deep Impact Ejecta

  • Vancleve, J.
  • Adams, A. C.
  • Mcfadden, L. A.
  • Belton, M. J. S.
  • Grillmair, C. J.
  • Ingalls, J.
  • Farnham, T. L.
  • Ahearn, M. F.
  • Fernández, Y. R.
  • Groussin, O.
  • Clark, B. C.
  • Schultz, P. H.
  • Meech, K. J.
  • Sunshine, J. M.
  • Lisse, C. M.
  • Feaga, L. M.
Abstract

Spitzer Space Telescope imaging spectrometer observations of comet 9P/Tempel 1 during the Deep Impact encounter returned detailed, highly structured, 5- to 35-micrometer spectra of the ejecta. Emission signatures due to amorphous and crystalline silicates, amorphous carbon, carbonates, phyllosilicates, polycyclic aromatic hydrocarbons, water gas and ice, and sulfides were found. Good agreement is seen between the ejecta spectra and the material emitted from comet C/1995 O1 (Hale-Bopp) and the circumstellar material around the young stellar object HD100546. The atomic abundance of the observed material is consistent with solar and C1 chondritic abundances, and the dust-to-gas ratio was determined to be greater than or equal to 1.3. The presence of the observed mix of materials requires efficient methods of annealing amorphous silicates and mixing of high- and low-temperature phases over large distances in the early protosolar nebula.

Topics
  • impedance spectroscopy
  • amorphous
  • Carbon
  • phase
  • annealing