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Spectroscopic investigation of liquid helium excited by a corona discharge: evidence for bubbles and 'red satellites'

Authors :
André Denat
V.M. Atrazhev
V. A. Shakhatov
K. von Haeften
Z.-L. Li
Frédéric Aitken
Nelly Bonifaci
Laboratoire de Génie Electrique de Grenoble (G2ELab)
Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS)
Department of Physics and Astronomy [Leicester]
University of Leicester
Joint Institute for High Temperatures (JIHT) and Russian Academy of Sciences
Izhorskaya St. 13
A.V. Topchiev Institute of Petrochemical Synthesis (TIPS)
Russian Academy of Sciences [Moscow] (RAS)
Institut des hautes densités d'énergie RAS
RAS
Garcia, Sylvie
Source :
European Physical Journal: Applied Physics, European Physical Journal: Applied Physics, EDP Sciences, 2009, 47 (2), pp.1-7. ⟨10.1051/epjap/2009092⟩, 11 th Int Symposium on High Pressure Low Temperature Plasma Chemistry (HAKONE XI), 11 th Int Symposium on High Pressure Low Temperature Plasma Chemistry (HAKONE XI), 2008, France. pp.550-554, European Physical Journal: Applied Physics, EDP Sciences, 2009, 47, p 22821
Publication Year :
2009
Publisher :
HAL CCSD, 2009.

Abstract

International audience; The establishment of corona discharges close to a point electrode under both negative and positive high voltage in normal liquid helium (LHe) at 4.2 K is reported. The experiments were carried out at constant temperature and pressures ranging from 0.1–10 MPa. Visible luminescence emitted from the zone close to the tip revealed lines due to excited He atoms and molecules. The molecular luminescence showed hot band emissions with vibrational levels populated up to . Rotational temperatures of 800 K were estimated showing that the excitations do not thermalise. With increasing pressure the lines shifted to shorter wavelengths and became broader. The magnitude of the increase in width deviated from what is expected from the gas phase and from classical line broadening theory and rather showed similarities to the behavior of bubbles in LHe. The detailed analysis of the rotational line intensity distribution revealed the presence of an additional radiator at the long wavelength side of molecular bands that we tentatively assign to “red satellite” emission. For corona discharges with positive tip polarities both atomic and molecular lines showed “red satellite" bands with much larger intensity than for negative polarity. The origin of the red satellite and the polarity dependence is unclear yet.

Details

Language :
English
ISSN :
12860042 and 12860050
Database :
OpenAIRE
Journal :
European Physical Journal: Applied Physics, European Physical Journal: Applied Physics, EDP Sciences, 2009, 47 (2), pp.1-7. ⟨10.1051/epjap/2009092⟩, 11 th Int Symposium on High Pressure Low Temperature Plasma Chemistry (HAKONE XI), 11 th Int Symposium on High Pressure Low Temperature Plasma Chemistry (HAKONE XI), 2008, France. pp.550-554, European Physical Journal: Applied Physics, EDP Sciences, 2009, 47, p 22821
Accession number :
edsair.doi.dedup.....e2bc4d05f39e0d239e6e6760db8b6115
Full Text :
https://doi.org/10.1051/epjap/2009092⟩