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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in Cooperation with on an Cooperation-Score of 37%

Topics

Publications (3/3 displayed)

  • 2022Numerical modelling of radiative heat transfer in a polydispersion of ceramic particles under direct high-flux solar irradiation11citations
  • 2022High-temperature optical and radiative properties of alumina–silica-based ceramic materials for solar thermal applications16citations
  • 2021Optical and radiative characterisation of alumina–silica based ceramic materials for high-temperature solar thermal applications12citations

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Lipiński, Wojciech
3 / 4 shared
Kumar, Apurv
3 / 3 shared
Kim, Jin Soo
1 / 1 shared
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2022
2021

Co-Authors (by relevance)

  • Lipiński, Wojciech
  • Kumar, Apurv
  • Kim, Jin Soo
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article

Numerical modelling of radiative heat transfer in a polydispersion of ceramic particles under direct high-flux solar irradiation

  • Lipiński, Wojciech
  • Kumar, Apurv
  • Kim, Jin Soo
  • Chen, Jingjing
Abstract

<p>The effects of polydispersity on radiative and interfacial convective heat transfer are investigated in particle–gas two-phase media for solar particle receiver applications. Non-grey radiative transfer is analysed using the collision-based Monte Carlo ray-tracing method. The Mie theory is employed to calculate radiative properties of particles. The finite volume method and the explicit Euler time integration scheme are used to solve the transient energy equations for the particle and gas phases. Three alternative approaches to modelling particle properties and thermal conditions are employed: (i) a novel discrete size model, in which particle groups within discrete size intervals are assigned individual properties and temperatures locally; (ii) a lumped size model, in which integral properties and a single temperature are assigned to the particle phase locally; and (iii) a monodisperse size model, in which properties are evaluated for the Sauter mean diameter of the polydispersion and a single temperature is assigned to the particle phase locally. Strongly size-dependent radiation absorption and interfacial convective heat transfer are predicted with the discrete size model for alumina particles. Particles smaller than 27.4μm located near the aperture absorb the solar irradiation and transfer heat to the gas phase most effectively. The angular spread of the incident solar radiation is found to have a negligible effect on the overall absorption, although the most uniform thermal conditions occur for the solar irradiation with the smallest confinement angle. The overall absorptance of alumina particles is higher by 3.4% and 2.7% than that of iron (III) oxide and mullite particles, respectively. The lumped and monodisperse size models allow for reduction of the computational time at the expense of lower accuracy and limited information about particle properties and thermal conditions.</p>

Topics
  • impedance spectroscopy
  • theory
  • iron
  • interfacial
  • gas phase
  • polydispersity
  • mullite