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
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in Cooperation with on an Cooperation-Score of 37%

Topics

Publications (4/4 displayed)

  • 2018Radar evidence of subglacial liquid water on Mars426citations
  • 2016Interpretation of Radar Sounder MARSIS Data from Lucus Planum, Mars: A Complex Geological Setting.citations
  • 2012Three Dimensional Structure of the Mars North Polar Basal Unit from MARSIS datacitations
  • 2007Marsis Data Inversion Approach: Preliminary Results on Mars South Polar Regioncitations

Places of action

Chart of shared publication
Pettinelli, E.
2 / 3 shared
Lauro, S. E.
1 / 1 shared
Martufi, R.
1 / 1 shared
Seu, R.
2 / 2 shared
Frigeri, A.
1 / 2 shared
Giuppi, S.
1 / 1 shared
Pajola, Maurizio
1 / 8 shared
Cassenti, F.
1 / 1 shared
Soldovieri, F.
1 / 2 shared
Cosciotti, B.
1 / 1 shared
Mitri, G.
2 / 2 shared
Coradini, M.
1 / 1 shared
Di Paolo, F.
1 / 1 shared
Flamini, E.
2 / 2 shared
Mattei, E.
1 / 2 shared
Cartacci, M.
3 / 3 shared
Cicchetti, A.
4 / 4 shared
Noschese, R.
1 / 1 shared
Restano, M.
1 / 2 shared
Masdea, A.
2 / 2 shared
Nenna, C.
1 / 1 shared
Caprarelli, G.
1 / 1 shared
Carter, L. M.
1 / 1 shared
Cantini, F.
1 / 1 shared
Rossi, A. P.
1 / 1 shared
Noschese, Raffaella
3 / 5 shared
Cartacci, Marco
1 / 3 shared
Papiano, I.
1 / 1 shared
Plaut, J.
2 / 2 shared
Frigeri, Alessandro
2 / 7 shared
Giuppi, Stefano
2 / 4 shared
Picardi, G.
2 / 6 shared
Chart of publication period
2018
2016
2012
2007

Co-Authors (by relevance)

  • Pettinelli, E.
  • Lauro, S. E.
  • Martufi, R.
  • Seu, R.
  • Frigeri, A.
  • Giuppi, S.
  • Pajola, Maurizio
  • Cassenti, F.
  • Soldovieri, F.
  • Cosciotti, B.
  • Mitri, G.
  • Coradini, M.
  • Di Paolo, F.
  • Flamini, E.
  • Mattei, E.
  • Cartacci, M.
  • Cicchetti, A.
  • Noschese, R.
  • Restano, M.
  • Masdea, A.
  • Nenna, C.
  • Caprarelli, G.
  • Carter, L. M.
  • Cantini, F.
  • Rossi, A. P.
  • Noschese, Raffaella
  • Cartacci, Marco
  • Papiano, I.
  • Plaut, J.
  • Frigeri, Alessandro
  • Giuppi, Stefano
  • Picardi, G.
OrganizationsLocationPeople

document

Marsis Data Inversion Approach: Preliminary Results on Mars South Polar Region

  • Pettinelli, E.
  • Gurnett, D.
  • Piccari, F.
  • Zampolini, E.
  • Melacci, P.
  • Nielsen, E.
  • Bombaci, O.
  • Jordan, R.
  • Marinangeli, L.
  • Federico, C.
  • Flamini, E.
  • Giuppi, Stefano
  • Biccari, D.
  • Cicchetti, A.
  • Calabrese, D.
  • Plaut, J.
  • Huff, R.
  • Seu, R.
  • Edenhofer, P.
  • Plettemeier, D.
  • Kirchner, D.
  • Johnson, W.
  • Williams, I.
  • Orosei, R.
  • Safaeinili, A.
  • Hagfors, T.
  • Vannaroni, G.
  • Frigeri, Alessandro
  • Picardi, G.
  • Marini, A.
  • Cartacci, M.
  • Noschese, Raffaella
  • Masdea, A.
Abstract

An approach to the inversion of the data available from the MARSIS (Mars Advanced Radar for Subsurface and Ionosphere Sounding) instrument on Mars Express is described. The data inversion gives an estimation of the materials composing the different detected interfaces, including the impurity (inclusion) of the first layer, if any, and its percentage, by the evaluation of the values of the permittivity that would generate the observed radio echoes. The data inversion method is based on the analysis of the surface to subsurface power ratio and the relative time delay as measured by MARSIS. A volume scattering and a multilayer analysis has been performed in order to analyze the influence of these scattering process on the obtained results. The data inversion has been performed at several frequencies to estimate the frequency dependent parameters affecting the behaviour of the radar echoes. The main complexity, pertaining to the data inversion, is related to the accuracy needed on the values of the dielectric constant on the surface (∊'m(0)), as well as on the accuracy in the radar data influenced by various causes as, for instance, the ionosphere residual distortion. Taking into account that along the orbits the echo frames exhibit a non stationary behaviour, due to the shape of the surface and subsurface, in order to obtain a proper inversion, the frames have been selected only in regions of MARS that are moderately flat as can be determined, a priori, from MOLA data and by the echoes' behaviour. Few models of the subsurface has been considered and a list of inclusion material considered as end to end members of possible scenarios have been assumed....

Topics
  • impedance spectroscopy
  • surface
  • inclusion
  • dielectric constant