Transport Processes and Structure Formation of a Pure Electron Plasma Coupled to an External Rotating Wave

2006 ◽  
Author(s):  
Y. Soga ◽  
Y. Kiwamoto ◽  
Y. Kawai ◽  
J. Aoki
Keyword(s):  
Structure Formation ◽  
Electron Plasma ◽  
Transport Processes ◽  
Rotating Wave

Heterogeneous Transport Processes and Unexpected Structure Formation in Layered Epoxy and Epoxy-Alumina Nanocomposite Systems

2011 ◽  
Vol 87 (11) ◽  
pp. 1073-1098 ◽  
Author(s):  
M. Philipp ◽  
U. Müller ◽  
R. Sanctuary ◽  
J. C. Gaukler ◽  
C. Wehlack ◽  
...  
Keyword(s):  
Structure Formation ◽  
Transport Processes

Transport processes of a non-neutral plasma coupled to an external rotating wave

2006 ◽  
Vol 13 (5) ◽  
pp. 052105 ◽  
Author(s):  
Y. Soga ◽  
Y. Kiwamoto ◽  
N. Hashizume
Keyword(s):  
Transport Processes ◽  
Rotating Wave ◽  
Neutral Plasma

scholarly journals Stability properties of phase transition layers in the diffuse ISM revisited

2012 ◽  
Vol 10 (H16) ◽  
pp. 611-611
Author(s):  
Jennifer M. Stone ◽  
Shu-ichiro Inutsuka ◽  
Ellen G. Zweibel
Keyword(s):  
Phase Transition ◽  
Interstellar Medium ◽  
Numerical Simulations ◽  
Structure Formation ◽  
Thermal Conduction ◽  
Transport Processes ◽  
Radiative Heating ◽  
Transition Layers ◽  
Stability Properties ◽  
Scant Attention

AbstractIn a thermally bistable medium, cold, dense gas is separated from warm, rarified gas by thin phase transition layers, or fronts, in which radiative heating/cooling, thermal conduction, and convection of material are balanced. While these fronts have received only scant attention in the literature, and are not resolved by most current numerical simulations, they have been shown to have important ramifications for transport processes and structure formation in the diffuse interstellar medium. Here, we discuss calculations of their hydrodynamic and magnetohydrodynamic stability properties.

scholarly journals Solitary structure formation and self-guiding of electromagnetic beam in highly degenerate electron plasma

2021 ◽  
Vol 28 (5) ◽  
pp. 052104
Author(s):  
V. I. Berezhiani ◽  
Z. N. Osmanov ◽  
S. M. Mahajan ◽  
S. V. Mikeladze
Keyword(s):  
Structure Formation ◽  
Electron Plasma ◽  
Degenerate Electron ◽  
Electromagnetic Beam

Saturn's E, G and F rings: modulated by the plasma sheet

1984 ◽  
Vol 75 ◽  
pp. 597
Author(s):  
E. Grün ◽  
G.E. Morfill ◽  
T.V. Johnson ◽  
G.H. Schwehm
Keyword(s):  
Solar Wind ◽  
Direct Contact ◽  
Transport Processes ◽  
Time Variable ◽  
Dust Particles ◽  
Spatial Diffusion ◽  
Drag Forces ◽  
Orbit Perturbation ◽  
Time Variations ◽  
F Ring

ABSTRACTSaturn's broad E ring, the narrow G ring and the structured and apparently time variable F ring(s), contain many micron and sub-micron sized particles, which make up the “visible” component. These rings (or ring systems) are in direct contact with magnetospheric plasma. Fluctuations in the plasma density and/or mean energy, due to magnetospheric and solar wind processes, may induce stochastic charge variations on the dust particles, which in turn lead to an orbit perturbation and spatial diffusion. It is suggested that the extent of the E ring and the braided, kinky structure of certain portions of the F rings as well as possible time variations are a result of plasma induced electromagnetic perturbations and drag forces. The G ring, in this scenario, requires some form of shepherding and should be akin to the F ring in structure. Sputtering of micron-sized dust particles in the E ring by magnetospheric ions yields lifetimes of 102to 104years. This effect as well as the plasma induced transport processes require an active source for the E ring, probably Enceladus.

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