Articolo in rivista, 2013, ENG, 10.1088/0029-5515/53/12/123002
S. Ratynskaia (1; L. Vignitchouk (1; P. Tolias (1; I. Bykov (2; H. Bergsåker (2; A. Litnovsky (3; N. den Harder (4; E. Lazzaro (5
1) Division of Space and Plasma Physics, Association EURATOM-VR, Royal Institute of Technology KTH, Sweden 2) Division of Fusion Plasma Physics, Association EURATOM-VR, Royal Institute of Technology KTH, Sweden 3) Institut fur Energieforschung-Plasmaphysik, Forschungszentrum J ¨ ulich, Association ¨ EURATOM-FZ Julich, Germany ¨ 4 FOM-Institute for Plasma Physics Rijnhuizen, Association EURATOM-FOM, The Netherlands 5) Istituto di Fisica del Plasma-CNR, Association EURATOM-ENEA-CNR, Milano, Italy
The modelling of a controlled tungsten dust injection experiment in TEXTOR by the dust dynamics code MIGRAINe is reported. The code, in addition to the standard dust-plasma interaction processes, also encompasses major mechanical aspects of dust-surface collisions. The use of analytical expressions for the restitution coefficients as functions of the dust radius and impact velocity allows us to account for the sticking and rebound phenomena that define which parts of the dust size distribution can migrate efficiently. The experiment provided unambiguous evidence of long-distance dust migration; artificially introduced tungsten dust particles were collected 120o toroidally away from the injection point, but also a selectivity in the permissible size of transported grains was observed. The main experimental results are reproduced by modelling.
Nuclear fusion (Online) 53 , pp. 642–646
Dust transport, wall reflections, tungsten
ID: 270548
Year: 2013
Type: Articolo in rivista
Creation: 2013-11-14 13:59:04.000
Last update: 2020-05-21 08:50:10.000
CNR authors
CNR institutes
EU Projects
External links
OAI-PMH: Dublin Core
OAI-PMH: Mods
OAI-PMH: RDF
DOI: 10.1088/0029-5515/53/12/123002
URL: http://iopscience.iop.org/0029-5515/53/12/123002/pdf/0029-5515_53_12_123002.pdf
External IDs
CNR OAI-PMH: oai:it.cnr:prodotti:270548
DOI: 10.1088/0029-5515/53/12/123002
Scopus: 2-s2.0-84889008281
ISI Web of Science (WOS): 000327787000004