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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Max Planck Institute for Solar System Research

in Cooperation with on an Cooperation-Score of 37%

Topics

Publications (3/3 displayed)

  • 2023Measured mechanical, optical and electrical properties of dust partciles collected in the coma of comet 67/Pcitations
  • 2020Electrical properties of cometary dust particles derived from line shapes of TOF-SIMS spectra measured by the ROSETTA/COSIMA instrument3citations
  • 2020Electrical properties of cometary dust particles derived from line shapes of TOF-SIMS spectra measured by the ROSETTA/COSIMA instrument3citations

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Hilchenbach, Martin
3 / 5 shared
Hornung, Klaus
3 / 4 shared
Kissel, Jochen
2 / 2 shared
Langevin, Yves
2 / 2 shared
Silen, Johan
1 / 1 shared
Modica, Paola
2 / 2 shared
Koch, Andreas
2 / 5 shared
Varmuza, Kurt
2 / 2 shared
Bardyn, Anais
2 / 2 shared
Schulz, Rita
2 / 3 shared
Engrand, Cecile
2 / 2 shared
Siljeström, Sandra
1 / 8 shared
Paquette, John
2 / 2 shared
Rynö, Jouni
2 / 3 shared
Baklouti, Donia
2 / 5 shared
Briois, Christelle
2 / 5 shared
Fischer, Henning
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Cottin, Hervé
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Thirkell, Laurent
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Merouane, Sihane
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Mellado, Eva Maria
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Fray, Nicolas
2 / 7 shared
Lehto, Harry
2 / 3 shared
Siljestrom, Sandra
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Silén, Johan
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Chart of publication period
2023
2020

Co-Authors (by relevance)

  • Hilchenbach, Martin
  • Hornung, Klaus
  • Kissel, Jochen
  • Langevin, Yves
  • Silen, Johan
  • Modica, Paola
  • Koch, Andreas
  • Varmuza, Kurt
  • Bardyn, Anais
  • Schulz, Rita
  • Engrand, Cecile
  • Siljeström, Sandra
  • Paquette, John
  • Rynö, Jouni
  • Baklouti, Donia
  • Briois, Christelle
  • Fischer, Henning
  • Cottin, Hervé
  • Thirkell, Laurent
  • Merouane, Sihane
  • Mellado, Eva Maria
  • Fray, Nicolas
  • Lehto, Harry
  • Siljestrom, Sandra
  • Silén, Johan
OrganizationsLocationPeople

article

Electrical properties of cometary dust particles derived from line shapes of TOF-SIMS spectra measured by the ROSETTA/COSIMA instrument

  • Kissel, Jochen
  • Langevin, Yves
  • Silen, Johan
  • Modica, Paola
  • Hornung, Klaus
  • Koch, Andreas
  • Stenzel, Oliver
  • Varmuza, Kurt
  • Bardyn, Anais
  • Schulz, Rita
  • Engrand, Cecile
  • Hilchenbach, Martin
  • Siljeström, Sandra
  • Paquette, John
  • Rynö, Jouni
  • Baklouti, Donia
  • Briois, Christelle
  • Fischer, Henning
  • Cottin, Hervé
  • Thirkell, Laurent
  • Merouane, Sihane
  • Mellado, Eva Maria
  • Fray, Nicolas
  • Lehto, Harry
Abstract

Between Aug. 2014 and Sept. 2016, while ESA's cornerstone mission Rosetta was operating in the vicinity of the nucleus and in the coma of comet 67P/Churyumov-Gerasimenko, the COSIMA instrument collected a large number of dust particles with diameters up to a millimeter. Positive or negative ions were detected by a time-of-flight secondary ion mass spectrometer (TOF-SIMS) and the composition of selected particles was deduced. Many of the negative ion mass spectra show, besides mass peaks at the correct position, an additional, extended contribution at the lower mass side caused by partial charging of the dust. This effect, usually avoided in SIMS applications, can in our case be used to obtain information on the electrical properties of the collected cometary dust particles, such as the specific resistivity (ρ<SUB>r</SUB> &gt; 1 . 2 ⋅10<SUP>10</SUP>Ω m) and the real part of the relative electrical permittivity (ε<SUB>r</SUB> &lt; 1.2). From these values a lower limit for the porosity is derived (P &gt; 0.8)....

Topics
  • impedance spectroscopy
  • resistivity
  • porosity
  • selective ion monitoring