Jul 2 – 6, 2018
Žofín Palace
Europe/Prague timezone

P2.4010 Multi-diagnostics investigation of an ECR plasma confined in a simple mirror trap

Jul 3, 2018, 2:00 PM
2h
Mánes

Mánes

Speaker

Giuseppe Castro

Description

See the full Abstract at http://ocs.ciemat.es/EPS2018ABS/pdf/P2.4010.pdf Time-characterization of RF/X-ray bursts during a Cyclotron Instability in Simple Mirror and B-minimum Traps D. Mascali1, J. Angot2, G. Castro1, A. Galatà,3 S. Gammino1, M. Giarrusso1, F. Leone4,5,1, M. Mazzaglia1, R. Miracoli6, E. Naselli4,1, G. Torrisi1 1 Istituto Nazionale di Fisica Nucleare, Laboratori Nazionali del Sud, Catania, 95123 - ITALY 2 Univ. Grenoble Alpes, CNRS, Grenoble INP*, LPSC-IN2P3, 38000 Grenoble, France * Institute of Engineering Univ. Grenoble Alpes 3 Istituto Nazionale di Fisica Nucleare, Laboratori Nazionali di Legnaro, Legnaro (PD) - Italy 4 Università di Catania, Dipartimento di Fisica e Astronomia, Sezione Astrofisica, Via S. Sofia 78, I-95123 Catania, Italy 5 INAF—Osservatorio Astrofisico di Catania, Via S. Sofia 78, I-95123 Catania, Italy 6 ESS - Bilbao, Bilbao, Spain A Cyclotron-type instability has been observed at INFN-LNS on an axis-symmetric plasma trap based on a Simple Mirror configuration, where the plasma is sustained via 4 and 7 GHz Electron Cyclotron Resonance heating, and at the LPSC in Grenoble, in a B-minimum trap operating at 14 GHz. The Radio and X-ray bursts produced by the unstable plasma have been characterized in a time resolved way: a) Radio-signals detected along and across the magnetic axis have been measured in a timescale <100 ns via 80 Gs/s, 20 GHz band scope; a dedicated wavelet analysis shows the inner-plasma self-generation of waves far from the pumping frequency; b) fast Germanium detectors provide the evolution of the X-rays emitted axially and radially, allowing time-resolved spectroscopy; typical observed X-ray bursts lie in the timescales of ms or tens of ms, depending on the mirror ratio, and are emitted by the plasma few ms after the RF ones. Both RF and X-ray signals can be ranked on a temporal sequence which provides the whole characterization of the instability. Implications on laboratory plasma physics and astrophysical plasmas will be discussed.

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