Farley-Buneman instability in dusty space plasma
- Space Research Center, PAS, Bartycka 18A, 00-716, Warsaw (Poland)
- Institute of Terrestrial Magnetism, the Ionosphere, and Radio Wave Propagation, Academy of Sciences of the RUSSIA, IZMIRAN, 142092 Troitsk, Moscow Region (Russian Federation)
The dusty plasma and turbulent plasma properties in the vicinity of Jupiter and particularly inside the Ganymede magnetosphere can be a key parameters for understanding the plasma processes The complex system magnetic and electric field inside the Jowian magnetosphere can drive electrojet. If these currents exceed a certain critical amplitude, a streaming instability called the Farley-Buneman or a collisional two-stream instability develops. This instability grows more rapidly at shorter wavelengths and the waves propagate nearly perpendicular to the magnetic field. It is well known that even system with finite number of interacting waves can realize a turbulent state in active media. In such cases, when the number of cooperating waves remains small due to a competition of processes of their instability and attenuation, the turbulence appears in the result of their stochastic behavior. We study of nonlinear stabilization and influence of the dust component, conditions of stochasticity and the different regimes in the conditions when the number of interacting waves keeps small by the strong competition of processes wave damping and instabilities are considered.
- OSTI ID:
- 21612210
- Journal Information:
- AIP Conference Proceedings, Journal Name: AIP Conference Proceedings Journal Issue: 1 Vol. 1397; ISSN 0094-243X; ISSN APCPCS
- Country of Publication:
- United States
- Language:
- English
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Related Subjects
79 ASTRONOMY AND ASTROPHYSICS
ASTROPHYSICS
ATTENUATION
DAMPING
DUSTS
ELECTRIC FIELDS
INSTABILITY
INTERPLANETARY SPACE
JUPITER PLANET
MAGNETIC FIELDS
NONLINEAR PROBLEMS
PHYSICS
PLANETS
PLASMA
PLASMA INSTABILITY
PLASMA MICROINSTABILITIES
PLASMA WAVES
SPACE
STABILIZATION
STOCHASTIC PROCESSES
TURBULENCE
TWO-STREAM INSTABILITY