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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University College London

in Cooperation with on an Cooperation-Score of 37%

Topics

Publications (2/2 displayed)

  • 2019Bistatic full-wave radar tomography detects deep interior voids, cracks and boulders in a rubble-pile asteroid model.15citations
  • 2017“TNOs are Cool”: A survey of the trans-Neptunian region XIII. Statistical analysis of multiple trans-Neptunian objects observed with Herschel Space Observatory19citations

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Sorsa, Liisa-Ida
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Doressoundiram, A.
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2017

Co-Authors (by relevance)

  • Sorsa, Liisa-Ida
  • Takala, Mika
  • Pursiainen, Sampsa
  • Deller, Jakob
  • Bambach, Patrick
  • Lellouch, E.
  • Stansberry, J.
  • Doressoundiram, A.
  • Kovalenko, I. D.
  • Müller, T.
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article

Bistatic full-wave radar tomography detects deep interior voids, cracks and boulders in a rubble-pile asteroid model.

  • Sorsa, Liisa-Ida
  • Takala, Mika
  • Pursiainen, Sampsa
  • Vilenius, Esa
  • Deller, Jakob
  • Bambach, Patrick
Abstract

In this paper, we investigate full-wave computed radar tomography (CRT) using a rubble-pile asteroid model in which a realistic shape (Itokawa) is coupled with a synthetic material composition and structure model. The aim is to show that sparse bistatic radar measurements can distinguish details inside a complex-structured rubble-pile asteroid. The results obtained suggest that distinct local permittivity distribution changes such as surface layers, voids, low-permittivity anomalies, high-permittivity boulders, and cracks can be detected with bistatic CRT, when the total noise level in the data is around −10 dB with respect to the signal amplitude. Moreover, the bistatic measurement setup improves the robustness of the inversion compared to the monostatic case. Reconstructing the smooth Gaussian background distribution was found to be difficult with the present approach, suggesting that complementary techniques, such as gravimetry, might be needed to improve the reliability of the inference in practice.

Topics
  • impedance spectroscopy
  • surface
  • tomography
  • crack
  • void