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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in Cooperation with on an Cooperation-Score of 37%

Topics

Publications (1/1 displayed)

  • 2019Cosmic Ray Physics with the LOFAR Radio Telescopecitations

Places of action

Chart of shared publication
Mulrey, K.
1 / 1 shared
Mitra, P.
1 / 2 shared
Nelles, A.
1 / 1 shared
Falcke, H.
1 / 1 shared
Hare, B. M.
1 / 1 shared
Hörandel, J. R.
1 / 1 shared
Bonardi, A.
1 / 1 shared
Rossetto, L.
1 / 2 shared
Scholten, O.
1 / 2 shared
Corstanje, Arthur
1 / 1 shared
Rachen, J. P.
1 / 1 shared
Buitink, Stijn
1 / 3 shared
Veen, S. Ter
1 / 1 shared
Winchen, Tobias
1 / 1 shared
Thoudam, S.
1 / 1 shared
Trinh, T. N. G.
1 / 1 shared
Chart of publication period
2019

Co-Authors (by relevance)

  • Mulrey, K.
  • Mitra, P.
  • Nelles, A.
  • Falcke, H.
  • Hare, B. M.
  • Hörandel, J. R.
  • Bonardi, A.
  • Rossetto, L.
  • Scholten, O.
  • Corstanje, Arthur
  • Rachen, J. P.
  • Buitink, Stijn
  • Veen, S. Ter
  • Winchen, Tobias
  • Thoudam, S.
  • Trinh, T. N. G.
OrganizationsLocationPeople

article

Cosmic Ray Physics with the LOFAR Radio Telescope

  • Mulrey, K.
  • Mitra, P.
  • Nelles, A.
  • Falcke, H.
  • Hare, B. M.
  • Hörandel, J. R.
  • Bonardi, A.
  • Rossetto, L.
  • Scholten, O.
  • Corstanje, Arthur
  • Rachen, J. P.
  • Schellart, P.
  • Buitink, Stijn
  • Veen, S. Ter
  • Winchen, Tobias
  • Thoudam, S.
  • Trinh, T. N. G.
Abstract

The LOFAR radio telescope is able to measure the radio emission from cosmic ray induced air showers with hundreds of individual antennas. This allows for precision testing of the emission mechanisms for the radio signal as well as determination of the depth of shower maximum $X_$, the shower observable most sensitive to the mass of the primary cosmic ray, to better than 20 g/cm$^2$. With a densely instrumented circular area of roughly 320 m$^2$, LOFAR is targeting for cosmic ray astrophysics in the energy range $10^{16}$ - $10^{18}$ eV. In this contribution we give an overview of the status, recent results, and future plans of cosmic ray detection with the LOFAR radio telescope.

Topics
  • impedance spectroscopy