• Aucun résultat trouvé

Analyses of plasma spheroids in dusty plasma by RF discharge in argon

N/A
N/A
Protected

Academic year: 2021

Partager "Analyses of plasma spheroids in dusty plasma by RF discharge in argon"

Copied!
3
0
0

Texte intégral

(1)

HAL Id: hal-01053576

https://hal.archives-ouvertes.fr/hal-01053576

Submitted on 31 Jul 2014

HAL is a multi-disciplinary open access archive for the deposit and dissemination of sci- entific research documents, whether they are pub- lished or not. The documents may come from teaching and research institutions in France or abroad, or from public or private research centers.

L’archive ouverte pluridisciplinaire HAL, est destinée au dépôt et à la diffusion de documents scientifiques de niveau recherche, publiés ou non, émanant des établissements d’enseignement et de recherche français ou étrangers, des laboratoires publics ou privés.

Analyses of plasma spheroids in dusty plasma by RF discharge in argon

Jean-François Lagrange, Maxime Mikikian, Isabelle Géraud-Grenier, Francois Faubert, Véronique Massereau-Guilbaud

To cite this version:

Jean-François Lagrange, Maxime Mikikian, Isabelle Géraud-Grenier, Francois Faubert, Véronique Massereau-Guilbaud. Analyses of plasma spheroids in dusty plasma by RF discharge in argon. XXII Europhysics Conference on Atomic and Molecular Physics of Ionized Gases (ESCAMPIG), Jul 2014, Greifswald, Germany. pp.P2-07-05. �hal-01053576�

(2)

ESCAMPIG XXII, Greifswald, Germany, July 15-19, 2014

Analyses of plasma spheroids in dusty plasma by RF discharge in argon

J.-F. Lagrange

(*)1

, M. Mikikian

2

, I. Géraud-Grenier

1

, F. Faubert

3

, V. Massereau-Guilbaud

1

1 GREMI, UMR7344, CNRS/Univ-Orléans, F-18028 Bourges, France

2 GREMI, UMR7344, CNRS/Univ-Orléans, F-45067 Orléans, France

3 IUT de Bourges, Département Mesures Physiques, 63 avenue de Lattre de Tassigny, 18020 Bourges Cedex, France

(*) [email protected]

Plasma spheroids appear in dusty plasma by RF discharge in Argon. Their movement, quantity and velocity can be controlled by the experimental conditions such as the gas flow rate, the pressure and the RF power. Spheroids are analysed by Optical Emission Spectroscopy. They are also studied for their interactions with the particle cloud formed by hydrogenated carbon particles.

Dust particles are previously produced by PECVD in a RF capacitive discharge (13.56 MHz) under a pressure of 120 Pa in pure CH4 [1] or in a N2-CH4 gas mixture [2]. Then, RF discharges are realised in Argon. Instabilities appear in the plasma for specific experimental conditions (gas flow rate, pressure, RF power). They look like plasma glow spheroids turning along the circumference of the space between electrodes (Fig. 1). Depending on the experimental conditions, it is possible to control their speed, and also the spheroids number, which are distributed at equal distance from each other.

Studies reported this kind of instabilities [3,4], but usually they appear as two sets of spheroids turning in opposite direction of rotation: one set of spheroids turning along the circumference of the top electrode, and the other one near the bottom electrode. In our vacuum chamber, we have only one set of spheroids in the inter-electrode space, which is typically 2.5 cm.

A 2D-mapping of spheroids is performed by Optical Emission Spectroscopy. In the same time during the discharge, the particles are in levitation between the electrodes. The interaction of the plasma spheroids with the particles is studied and discussed, in particular the repulsive effect put in evidence using laser light scattering by particles, when the spheroids go into the particle cloud.

Fig. 1: Plasma spheroids in the discharge. The particle cloud is evidenced in green colour by laser light scattering.

Acknowledgments

This work was supported by the French National Agency (ANR), Project INDIGO No. ANR-11-JS09- 010-01.

RF electrode

Grounded electrode Plasma spheroids

Particle cloud

Topic number: 7

(3)

ESCAMPIG XXII, Greifswald, Germany, July 15-19, 2014

References

[1] I. Géraud-Grenier, V. Massereau-Guilbaud, and A. Plain, Surf. Coat. Technol. 187 (2004) 336- 342.

[2] J. Pereira, V. Massereau-Guilbaud, I. Géraud-Grenier, and A. Plain, J. Appl. Phys. 103 (2008) 033301-9.

[3] M. Mikikian, L. Couedel, Y. Tessier, and L. Boufendi, IEEE Trans. Plasma Sci. 39 (2011) 2748- 2749.

[4] H. Tawidian, M. Mikikian, L. Couëdel, and T. Lecas, Eur. Phys. J. Appl. Phys. 56 (2011) 24018.

Références

Documents relatifs

This work is devoted to the study of the relative permittivity in argon expanding plasma produced below a microwave discharge sustained in a quartz tube and working at 2.45 GHz..

We investigated electrostatic instabilities of FB type in the partially ionized plasma of the solar chromosphere taking into account ion and electron thermal effects, electron and

The case of Ar/CH 4 plasma is more complicated, a small increase of the electron density is observed at the very beginning of the afterglow which tends to indicate that the

These unstable phenomena are easily detected on the plasma glow emission: Regions with an enhanced emission appear stochastically or regularly at different places of the plasma..

This specific type of oscillation has been observed during the ending phase of the heartbeat instability which is characterized by an alternation of small and high amplitude

Thanks to the appearance time, the different frequencies of the instability (starting, during the long stochastic phase, and final) can also be determined as shown in figure 14

Abstract - R otating plasma spheroids are observed in a capacitively-coupled radio-frequency (ccrf) discharge containing grown dust particles.. These plasma spheroids

Plasma instabilities triggered by dust particle formation, (a) Plasma glow emission observed with a standard color camera showing striation like patterns (3 cm gap between