SMuK 2023 – wissenschaftliches Programm
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P: Fachverband Plasmaphysik
P 11: Poster I
P 11.19: Poster
Mittwoch, 22. März 2023, 14:00–15:30, HSZ EG
COMPACT -- the future complex plasma facility for the ISS — •Daniel P. Mohr1, Christina A. Knapek1, Stefan Schütt1, Daniel Maier1, Andre Melzer1, Lenaic Couedel2, Adrienne Dove3, John Goree4, Uwe Konopka5, Svetlana Ratynskaia6, Markus H. Thoma7, and Hubertus M. Thomas8 for the COMPACT collaboration — 1University of Greifswald, Institute of Physics, Greifswald, Germany — 2Department of Physics & Engineering Physics, University of Saskatchewan, Saskatoon, Canada — 3Department of Physics, University of Central Florida, Orlando, Florida, USA — 4Dept. of Physics & Astronomy, The University of Iowa, Iowa City, Iiowa, USA — 5Physics Department, Auburn University, Auburn, Alabama, USA — 6Space & Plasma Physics, School of Electrical Engineering, Royal Institute of Technology (KTH), Stockholm, Sweden — 7I. Physikalisches Institut, Justus-Liebig-Universität Gießen, Gießen, Germany — 8Institut für Materialphysik im Weltraum, Deutsches Zentrum für Luft- und Raumfahrt (DLR), Köln, Germany
Complex, or dusty, plasmas consist of micrometer-sized grains injected into a low temperature noble gas discharge. The grains become charged and interact with each other via a screened Coulomb potential. On ground, gravity compresses the system and prevents the generation of larger, three-dimensional particle clouds.
The future complex plasma facility COMPACT will allow the investigation of large three-dimensional complex plasmas under microgravity conditions on the International Space Station (ISS). Its technology is mainly based on pre-studies (Ekoplasma, PlasmaLab), including a novel plasma chamber with adaptive internal geometry, a four-electrode radio-frequency system for plasma generation, and a stereoscopic particle diagnostic that allows to record 3D particle dynamics in real-time.
We will present the scientific goals of COMPACT, scientific and technology results from the pre-studies, technologies currently under discussion, and the project status.
This work is funded by DLR/BMWi (FKZ 50WM2161).