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

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Ferrari, S.

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in Cooperation with on an Cooperation-Score of 37%

Topics

Publications (11/11 displayed)

  • 2019Managing transport properties in composite electrodes/electrolytes for all-solid-state lithium-based batteries45citations
  • 2013Calcium pyroxenes at Mercurian surface temperatures: investigation of in-situ emissivity spectra and thermal expansioncitations
  • 2012New electrolyte membranes for Li-based cells: Methacrylic polymers encompassing pyrrolidinium-based ionic liquid by single step photo-polymerisation33citations
  • 2012Electrical properties of V 2O 5 nanomaterials prepared by twin rollers technique20citations
  • 2011Structural, morphological and electrochemical properties of nanocrystalline V2O5 thin films deposited by means of r.f magnetron sputtering37citations
  • 2011Simulating thermal stress features on hot planetary surfaces in vacuum at high temperature facility in the PEL laboratorycitations
  • 2010Lithium ion conducting PVdF-HFP composite gel electrolytes based on N-methoxyethyl-N-methylpyrrolidinium bis(trifluoromethanesulfonyl)-imide ionic liquid228citations
  • 2010Lithium ion conducting PVdF-HFP composite gel electrolytes based on N-methoxyethyl-N-methylpyrrolidinium bis(trifluoromethanesulfonyl)-imide ionic liquidcitations
  • 2006The use of illitic clay in the production of stoneware tile ceramics150citations
  • 2006Rietveld structure refinement of zeolite ECR-121citations
  • 2006Sinterizzazione a microonde di polveri sferiche da lavorazioni industrialicitations

Places of action

Chart of shared publication
Gerbaldi, C.
3 / 47 shared
Falco, M.
1 / 18 shared
B., Appetecchi G.
1 / 2 shared
Massironi, M.
1 / 1 shared
Domeneghetti, M.
1 / 1 shared
Damore, Mario
2 / 2 shared
Alvaro, M.
1 / 10 shared
Maturilli, A.
2 / 4 shared
Nestola, F.
1 / 10 shared
Helbert, J.
2 / 4 shared
Hiesinger, H.
1 / 1 shared
Meligrana, Giuseppina
1 / 19 shared
Gerbaldi, Claudio
1 / 59 shared
Bongiovanni, Roberta Maria
1 / 18 shared
Chiappone, Annalisa
1 / 23 shared
Penazzi, Nerino
1 / 8 shared
Nair, Jr
1 / 2 shared
Zanarini, Simone
1 / 1 shared
Mustarelli, P.
4 / 25 shared
Wasiucionek, M.
1 / 5 shared
L., Nowinski J.
1 / 1 shared
K., Pietrzak T.
1 / 1 shared
Maciaszek, M.
1 / 1 shared
Wzorek, M.
1 / 2 shared
E., Garbarczyk J.
1 / 1 shared
Slubowska, W.
1 / 1 shared
Quartarone, E.
2 / 12 shared
Quinzeni, I.
1 / 1 shared
Dincecco, P.
1 / 1 shared
Magistris, A.
1 / 4 shared
Protti, S.
1 / 1 shared
Spinella, A.
2 / 4 shared
Fagnoni, M.
1 / 1 shared
Albini, Angelo
1 / 3 shared
Fagnoni, Maurizio
1 / 5 shared
Mustarelli, Piercarlo
1 / 22 shared
Magistris, Aldo
1 / 1 shared
Quartarone, Eliana
1 / 8 shared
Gualtieri, Alessandro
2 / 13 shared
Renzo, F. Di
1 / 2 shared
Galli, Ermanno
1 / 2 shared
Beek, W. Van
1 / 2 shared
Poli, Giorgio
1 / 23 shared
Veronesi, Paolo
1 / 50 shared
Chart of publication period
2019
2013
2012
2011
2010
2006

Co-Authors (by relevance)

  • Gerbaldi, C.
  • Falco, M.
  • B., Appetecchi G.
  • Massironi, M.
  • Domeneghetti, M.
  • Damore, Mario
  • Alvaro, M.
  • Maturilli, A.
  • Nestola, F.
  • Helbert, J.
  • Hiesinger, H.
  • Meligrana, Giuseppina
  • Gerbaldi, Claudio
  • Bongiovanni, Roberta Maria
  • Chiappone, Annalisa
  • Penazzi, Nerino
  • Nair, Jr
  • Zanarini, Simone
  • Mustarelli, P.
  • Wasiucionek, M.
  • L., Nowinski J.
  • K., Pietrzak T.
  • Maciaszek, M.
  • Wzorek, M.
  • E., Garbarczyk J.
  • Slubowska, W.
  • Quartarone, E.
  • Quinzeni, I.
  • Dincecco, P.
  • Magistris, A.
  • Protti, S.
  • Spinella, A.
  • Fagnoni, M.
  • Albini, Angelo
  • Fagnoni, Maurizio
  • Mustarelli, Piercarlo
  • Magistris, Aldo
  • Quartarone, Eliana
  • Gualtieri, Alessandro
  • Renzo, F. Di
  • Galli, Ermanno
  • Beek, W. Van
  • Poli, Giorgio
  • Veronesi, Paolo
OrganizationsLocationPeople

document

Simulating thermal stress features on hot planetary surfaces in vacuum at high temperature facility in the PEL laboratory

  • Damore, Mario
  • Dincecco, P.
  • Maturilli, A.
  • Ferrari, S.
  • Helbert, J.
Abstract

In the Planetary Emissivity Laboratory (PEL) at the Institute for Planetary Research of the German Aerospace Center (DLR) in Berlin, we set-up a simulation chamber for the spectroscopic investigation of minerals separates under Mercurial conditions. The chamber can be evacuated to 10-4 bar and the target samples heated to 700 K within few minutes, thanks to the innovative inductive heating system. While developing the protocol for the high temperature spectroscopy measurements we discovered interesting "morphologies" on the sample surfaces. The powders are poured into stainless steel cups of 50 mm internal diameter, 8 mm height and 3 mm depth, having a 5 mm thick base (thus leaving 3 mm free space for the minerals), and rim 1 mm thick. We selected several minerals of interest for Mercurial surface composition and for each of them we analyzed various grain size separates, to study the influence of grain dimensions to the process of thermal stressing. We observed that for the smaller grain size separate (0-25 μm) the thermal stress mainly induces large depressions and fractures, while on larger grain sizes (125-250 μm) small depressions and a cratered surface. Our current working hypothesis is that these features are mainly caused by thermal stress induced by a radiatively quickly cooling surface layer covering the much hotter bulk material. Further investigation is ongoing to understand the processes better. The observed morphologies exhibit surprising similarities to features observed at planetary scale size for example on Mercury and even on Venus. Especially the high resolution images provided currently from MESSENGER'S Mercury Dual Imaging System (MDIS) instrument has revealed plains dominated by polygonal fractures whose origin still have to be determined. Our laboratory analogue studies might in the future provide some insight into the processes creating those features...

Topics
  • impedance spectroscopy
  • mineral
  • surface
  • grain
  • stainless steel
  • grain size
  • simulation
  • Mercury