Radio-frequency plasma start-up at uragan-3M stellarator

V. E. Moiseenko; A. Lyssoivan; T. Wauters; M. Tripský; A. V. Lozin; R. O. Pavlichenko; M. M. Kozulya; M. B. Dreval; Yu K. Mironov; V. S. Romanov; A. Ye Kulaga; N. V. Zamanov; A. N. Shapoval; V. G. Konovalov; V. V. Chechkin; L. I. Grigor’eva; A. A. Beletskii; A. A. Kasilov; I. E. Garkusha

Radio-frequency plasma start-up at uragan-3M stellarator

V. E. Moiseenko, A. Lyssoivan, T. Wauters, M. Tripský, A. V. Lozin, R. O. Pavlichenko, M. M. Kozulya, M. B. Dreval, Yu K. Mironov, V. S. Romanov, A. Ye Kulaga, N. V. Zamanov, A. N. Shapoval, V. G. Konovalov, V. V. Chechkin, L. I. Grigor’eva, A. A. Beletskii, A. A. Kasilov, I. E. Garkusha

Laboratory for Plasma Physics

Inst. of Plasma Physics of the National Science Center kharkiv Institute of Physics and Technology

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A double frame antenna with a broad spectrum of parallel wavenumbers (with respect to the magnetic field) is used for radio-frequency (RF) plasma production in Uragan-3M stellarator type device. The delay between the start of RF pulse and the discharge development (breakdown (delay) time) is analyzed as functions of the magnetic field strength, neutral gas pressure and anode voltage of the RF generator. The reproducibility of the RF discharges is improved by the pre-ionization by the pulse of the three-half-turn antenna preceding the main RF pulse. The pre-ionization also results in shortening of the breakdown time for the frame antenna. The Langmuir probe measurements are made with two probes located at the plasma edge near and far from the double frame antenna. The measurements give rather high edge electron temperature, about 100 eV, at the initial stage of the frame antenna discharge both near and far from the antenna. The information on the plasma build-up is also given by the Hα chord measurements.

Originele taal-2	Engels
Pagina's (van-tot)	54-59
Aantal pagina's	6
Tijdschrift	Problems of Atomic Science and Technology
Volume	107
Nummer van het tijdschrift	1
Status	Gepubliceerd - 2017

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Moiseenko, V. E., Lyssoivan, A., Wauters, T., Tripský, M., Lozin, A. V., Pavlichenko, R. O., Kozulya, M. M., Dreval, M. B., Mironov, Y. K., Romanov, V. S., Kulaga, A. Y., Zamanov, N. V., Shapoval, A. N., Konovalov, V. G., Chechkin, V. V., Grigor’eva, L. I., Beletskii, A. A., Kasilov, A. A., & Garkusha, I. E. (2017). Radio-frequency plasma start-up at uragan-3M stellarator. Problems of Atomic Science and Technology, 107(1), 54-59.

@article{5563e027f52745ebbee310620cf5dca3,

title = "Radio-frequency plasma start-up at uragan-3M stellarator",

abstract = "A double frame antenna with a broad spectrum of parallel wavenumbers (with respect to the magnetic field) is used for radio-frequency (RF) plasma production in Uragan-3M stellarator type device. The delay between the start of RF pulse and the discharge development (breakdown (delay) time) is analyzed as functions of the magnetic field strength, neutral gas pressure and anode voltage of the RF generator. The reproducibility of the RF discharges is improved by the pre-ionization by the pulse of the three-half-turn antenna preceding the main RF pulse. The pre-ionization also results in shortening of the breakdown time for the frame antenna. The Langmuir probe measurements are made with two probes located at the plasma edge near and far from the double frame antenna. The measurements give rather high edge electron temperature, about 100 eV, at the initial stage of the frame antenna discharge both near and far from the antenna. The information on the plasma build-up is also given by the Hα chord measurements.",

author = "Moiseenko, {V. E.} and A. Lyssoivan and T. Wauters and M. Tripsk{\'y} and Lozin, {A. V.} and Pavlichenko, {R. O.} and Kozulya, {M. M.} and Dreval, {M. B.} and Mironov, {Yu K.} and Romanov, {V. S.} and Kulaga, {A. Ye} and Zamanov, {N. V.} and Shapoval, {A. N.} and Konovalov, {V. G.} and Chechkin, {V. V.} and Grigor{\textquoteright}eva, {L. I.} and Beletskii, {A. A.} and Kasilov, {A. A.} and Garkusha, {I. E.}",

year = "2017",

language = "English",

volume = "107",

pages = "54--59",

journal = "Problems of Atomic Science and Technology",

issn = "1682-9344",

number = "1",

}

Moiseenko, VE, Lyssoivan, A, Wauters, T, Tripský, M, Lozin, AV, Pavlichenko, RO, Kozulya, MM, Dreval, MB, Mironov, YK, Romanov, VS, Kulaga, AY, Zamanov, NV, Shapoval, AN, Konovalov, VG, Chechkin, VV, Grigor’eva, LI, Beletskii, AA, Kasilov, AA & Garkusha, IE 2017, 'Radio-frequency plasma start-up at uragan-3M stellarator', Problems of Atomic Science and Technology, vol. 107, nr. 1, blz. 54-59.

TY - JOUR

T1 - Radio-frequency plasma start-up at uragan-3M stellarator

AU - Moiseenko, V. E.

AU - Lyssoivan, A.

AU - Wauters, T.

AU - Tripský, M.

AU - Lozin, A. V.

AU - Pavlichenko, R. O.

AU - Kozulya, M. M.

AU - Dreval, M. B.

AU - Mironov, Yu K.

AU - Romanov, V. S.

AU - Kulaga, A. Ye

AU - Zamanov, N. V.

AU - Shapoval, A. N.

AU - Konovalov, V. G.

AU - Chechkin, V. V.

AU - Grigor’eva, L. I.

AU - Beletskii, A. A.

AU - Kasilov, A. A.

AU - Garkusha, I. E.

PY - 2017

Y1 - 2017

N2 - A double frame antenna with a broad spectrum of parallel wavenumbers (with respect to the magnetic field) is used for radio-frequency (RF) plasma production in Uragan-3M stellarator type device. The delay between the start of RF pulse and the discharge development (breakdown (delay) time) is analyzed as functions of the magnetic field strength, neutral gas pressure and anode voltage of the RF generator. The reproducibility of the RF discharges is improved by the pre-ionization by the pulse of the three-half-turn antenna preceding the main RF pulse. The pre-ionization also results in shortening of the breakdown time for the frame antenna. The Langmuir probe measurements are made with two probes located at the plasma edge near and far from the double frame antenna. The measurements give rather high edge electron temperature, about 100 eV, at the initial stage of the frame antenna discharge both near and far from the antenna. The information on the plasma build-up is also given by the Hα chord measurements.

AB - A double frame antenna with a broad spectrum of parallel wavenumbers (with respect to the magnetic field) is used for radio-frequency (RF) plasma production in Uragan-3M stellarator type device. The delay between the start of RF pulse and the discharge development (breakdown (delay) time) is analyzed as functions of the magnetic field strength, neutral gas pressure and anode voltage of the RF generator. The reproducibility of the RF discharges is improved by the pre-ionization by the pulse of the three-half-turn antenna preceding the main RF pulse. The pre-ionization also results in shortening of the breakdown time for the frame antenna. The Langmuir probe measurements are made with two probes located at the plasma edge near and far from the double frame antenna. The measurements give rather high edge electron temperature, about 100 eV, at the initial stage of the frame antenna discharge both near and far from the antenna. The information on the plasma build-up is also given by the Hα chord measurements.

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AN - SCOPUS:85016122250

SN - 1682-9344

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EP - 59

JO - Problems of Atomic Science and Technology

JF - Problems of Atomic Science and Technology

IS - 1

ER -

Radio-frequency plasma start-up at uragan-3M stellarator

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