Laboratory studies of the dynamic of resonance cones formation in magnetized plasmas
- 1. Russian Academy of Sciences, Institute of Applied Physics, Nizhny Novgorod (Russian Federation)
Description
The paper is devoted to experimental studies of formation of resonance cones in magnetized plasmas by pulsed RF source in the lower-hybrid (whistler) and the upper-hybrid frequency ranges. It is shown that in both frequency ranges, resonance cones exhibit similar dynamics after switching-on the RF source: at first, wide maxima of radiation are formed in non-resonance directions, which then become narrower, with their direction approaching the resonance one. While the resonance cones are being formed, one observes a fine structure in the form of secondary radiation maxima. It is shown that the characteristic formation time of stationary resonance cones is determined by the minimal value of the group velocity of the quasi-electrostatic waves excited by the antenna. In the low-temperature plasma, this value is limited in the lower-hybrid frequency range by the spatial spectrum of the emitting antenna and in the upper-hybrid range, by the effects of spatial plasma dispersion.
Additional details
Identifiers
- DOI
- 10.1063/1.4794965;
Publishing Information
- Journal Title
- Physics of Plasmas
- Journal Volume
- 20
- Journal Issue
- 3
- Journal Page Range
- p. 032110-032110.10
- ISSN
- 1070-664X
- CODEN
- PHPAEN
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 44065472
- Subject category
- S70: PLASMA PHYSICS AND FUSION TECHNOLOGY;
- Descriptors DEI
- ANTENNAS; CONES; DISPERSIONS; FINE STRUCTURE; FREQUENCY RANGE; LOWER HYBRID CURRENT DRIVE; LOWER HYBRID HEATING; PLASMA; PULSES; RESONANCE; SPECTRA; VELOCITY; WHISTLERS
- Descriptors DEC
- ELECTRICAL EQUIPMENT; ELECTROMAGNETIC RADIATION; EQUIPMENT; HEATING; HIGH-FREQUENCY HEATING; NOISE; NON-INDUCTIVE CURRENT DRIVE; PLASMA HEATING; RADIATIONS; RADIO NOISE; RADIOWAVE RADIATION
Optional Information
- Notes
- (c) 2013 American Institute of Physics