TY - JOUR
T1 - Observation of Plasma Turbulence in a Hall Thruster Using Microwave Interferometry
AU - Yamamoto, Naoji
AU - Kuwabara, Naoya
AU - Kuwahara, Daisuke
AU - Cho, Shinatora
AU - Kosuga, Yusuke
AU - Pradalier, Guilhem Dif
N1 - Publisher Copyright:
© 2023 by the American Institute of Aeronautics and Astronautics, Inc.
PY - 2023/11
Y1 - 2023/11
N2 - To understand anomalous electron transport in a Hall thruster, plasma turbulence inside the acceleration channel was observed using a 76 GHz microwave interferometer. The dependence of the amplitude of the 100–500 kHz turbulence on magnetic flux density, and the relationships between the turbulence and other plasma instabilities and between the turbulence and the discharge current were investigated through spectral density and bicoherence analysis. The amplitude of electron number density fluctuations of the turbulence, integrating the spectral density from 100 to 500 kHz, is 1017 m−3, or almost 10% of the time-averaged electron number density. The amplitude of the turbulence decreases with increase in weak magnetic field strength (coil current less than 0.6 A) and then increases with increase in magnetic field strength. The amplitude of the turbulence has a positive relation to the discharge current, leads to anomalous electron transport inside the acceleration channel, and is coupled with ionization instability. In addition, low-frequency perturbations of several hundred hertz were observed, with a positive relation to the turbulence and coupled with both ionization instability and turbulence.
AB - To understand anomalous electron transport in a Hall thruster, plasma turbulence inside the acceleration channel was observed using a 76 GHz microwave interferometer. The dependence of the amplitude of the 100–500 kHz turbulence on magnetic flux density, and the relationships between the turbulence and other plasma instabilities and between the turbulence and the discharge current were investigated through spectral density and bicoherence analysis. The amplitude of electron number density fluctuations of the turbulence, integrating the spectral density from 100 to 500 kHz, is 1017 m−3, or almost 10% of the time-averaged electron number density. The amplitude of the turbulence decreases with increase in weak magnetic field strength (coil current less than 0.6 A) and then increases with increase in magnetic field strength. The amplitude of the turbulence has a positive relation to the discharge current, leads to anomalous electron transport inside the acceleration channel, and is coupled with ionization instability. In addition, low-frequency perturbations of several hundred hertz were observed, with a positive relation to the turbulence and coupled with both ionization instability and turbulence.
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U2 - 10.2514/1.B38711
DO - 10.2514/1.B38711
M3 - Article
AN - SCOPUS:85181987547
SN - 0748-4658
VL - 39
SP - 849
EP - 855
JO - Journal of Propulsion and Power
JF - Journal of Propulsion and Power
IS - 6
ER -