2017
DOI: 10.1007/s10894-017-0135-0
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Development of a Helicon Plasma Source for Neutral Beam Injection System of the Alborz Tokamak

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Cited by 8 publications
(4 citation statements)
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“…Common features have been drawn from this mode such as azimuthal instabilities driven by radial pressure gradients, and high-beta (beta is the ratio of particle pressure to magnetic field pressure) effects [16]. Previous studies mainly employed optical camera and/or spectrometer to characterise these features after the blue-core formation [10,11,[17][18][19], however, little attention was given to the transitional behaviours from non-blue-core mode to bluecore mode. Especially, to our best knowledge, there is no measurement yet about the wave field and power absorption inside and outside the blue-core plasma column, respectively.…”
Section: Introductionmentioning
confidence: 99%
“…Common features have been drawn from this mode such as azimuthal instabilities driven by radial pressure gradients, and high-beta (beta is the ratio of particle pressure to magnetic field pressure) effects [16]. Previous studies mainly employed optical camera and/or spectrometer to characterise these features after the blue-core formation [10,11,[17][18][19], however, little attention was given to the transitional behaviours from non-blue-core mode to bluecore mode. Especially, to our best knowledge, there is no measurement yet about the wave field and power absorption inside and outside the blue-core plasma column, respectively.…”
Section: Introductionmentioning
confidence: 99%
“…In our experimental conditions, ω was ~13.56 MHz, B 0 was ~78 G, a was 1.5 cm and P was 300 W. The plasma density n e under RH helical antenna excitation was ~8× 10 18 m −3 and T e was ~12 eV, while the plasma density n e was ~2×10 18 m −3 and T e was ~11 eV under LH helical antenna excitation. The wavelength calculated by the bounded whistler wave dispersion relation (11) for RH helical antenna excitation is about 8.74 cm, whereas the calculated value for LH helical antenna excitation is about 32.95 cm. The wavelength determined by the unbounded dispersion equation (10) for whistler waves under RH helical antenna excitation is about 1.72 cm, and the wavelength of LH helical antenna excitation is about 3.34 cm.…”
Section: Exp [I (Mθmentioning
confidence: 69%
“…The blue core appears and extends from upstream of the discharge tube to downstream as the power is increased. The presence of blue core is often used to represent the helicon plasma discharge entering W mode [11,26,[32][33][34]. Boswell [8] suggested that the blue core mode discharge was a sign that the helicon plasma discharge mode had jumped to wave mode.…”
Section: Axial Distributionmentioning
confidence: 99%
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