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In-vessel coils are used for plasma instability control, error field correct, RWM and ELMs suppress.
The nighttime (post-sunset) ESF structure started from F-region bottomside where positive (upward) plasma density gradients favoring for plasma instability development usually exist and grew up to 450 km into the topside.
However, for the present case, the starting altitude of the daytime irregularity structure is near/above the F-region peak (~ 360 km) where the background plasma density gradient is usually not favorable for plasma instability.
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The paper presents an overview on the power supply (PS) systems for plasma instabilities control in fusion experiments, based on active control coils.
Internal standards introduced with the sample were used to correct for plasma instabilities.
Since the plasma in Hall thrusters is far from equilibrium and is placed in a rather strong magnetic field, both features create conditions for plasma instabilities to occur.
Internal standards (Sc, Ge, and Bi) introduced with the sample were used to correct for plasma instabilities.
An internal standard (Er) introduced with the sample was used to monitor for plasma instabilities and correct for changes in sample matrix.
It is also a well-known fact that the development of the PRE is the most basic condition for the initiation of plasma instability process by Rayleigh-Taylor mechanism leading to generation of plasma bubble/spread F irregularities.
For example, active feedback control of plasma instability developed at Columbia University are guiding research on NSTX at the Princeton Plasma Physics Laboratory, on the DIII-D tokamak at General Atomics, and for the design of the next generation burning plasma experiment, ITER.
Recent studies, however, have found an unexpected high occurrence of ionospheric F-region irregularities during June solstice, when conditions are believed to be unfavorable for the development of plasma instabilities responsible for equatorial spread-F (ESF).
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