Ion-Flow-Induced Excitation of Electrostatic Cyclotron Mode in Magnetized Dusty Plasma
- Авторлар: Bezbaruah P.1, Das N.1
- 
							Мекемелер: 
							- Department of Physics
 
- Шығарылым: Том 44, № 5 (2018)
- Беттер: 514-519
- Бөлім: Dusty Plasma
- URL: https://journal-vniispk.ru/1063-780X/article/view/186767
- DOI: https://doi.org/10.1134/S1063780X18050057
- ID: 186767
Дәйексөз келтіру
Аннотация
The stability of electrostatic cyclotron mode is investigated in a flowing magnetized dusty plasma in the presence of strong ion–neutral collisions. In the high magnetic field limit, when the dust magnetization becomes important, it is expected that the collective behavior of magnetized dust grains suspended in the near-sheath region substantially influences the dispersion properties of electrostatic modes. The growth/damping of the collective excitation is significantly controlled by such parameters as the ion–neutral collision frequency, Mach number, and magnetic field strength. In our case, the explicit dependence of the Mach number on the magnetic field and collision frequency has been taken into account and possible implications on the stability of the mode is analyzed. Streaming instability of cyclotron modes may be important to understand issues related to the interaction mechanism between dust grains and other associated phenomena like Coulomb crystallization, phase behavior, transport properties, etc., in the relatively strong magnetic field limit, which is currently accessible in the DPD (Kiel University) and MDPX (PSL, Auburn University) experiments.
Авторлар туралы
P. Bezbaruah
Department of Physics
							Хат алмасуға жауапты Автор.
							Email: pratphd@tezu.ernet.in
				                					                																			                												                	Үндістан, 							Assam, 784028						
N. Das
Department of Physics
														Email: pratphd@tezu.ernet.in
				                					                																			                												                	Үндістан, 							Assam, 784028						
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