The potential around a test charge in magnetized dusty plasmas

1996 ◽  
Vol 3 (10) ◽  
pp. 3858-3860 ◽  
Author(s):  
P. K. Shukla ◽  
M. Salimullah
Keyword(s):  
Dusty Plasmas ◽  
Test Charge

Energy Loss of a Test Charge in Dusty Plasmas: Collective and Individual Particle Contributions

1999 ◽  
Vol 59 (5) ◽  
pp. 379-388 ◽  
Author(s):  
M H Nasim ◽  
Arshad M Mirza ◽  
G Murtaza ◽  
P K Shukla
Keyword(s):  
Energy Loss ◽  
Dusty Plasmas ◽  
Individual Particle ◽  
Test Charge

Energy Loss of a Test Charge in Collisional Dusty Plasmas

2000 ◽  
Vol 61 (5) ◽  
pp. 628-634 ◽  
Author(s):  
M H Nasim ◽  
Arshad M Mirza ◽  
G Murtaza ◽  
P K Shukla
Keyword(s):  
Energy Loss ◽  
Dusty Plasmas ◽  
Test Charge

scholarly journals Plasma Diagnostic Methods: Test Charge Response in Lorentzian Dusty Plasmas

2020 ◽  
Author(s):  
Shahid Ali ◽  
Yas Al-Hadeethi
Keyword(s):  
Dusty Plasmas ◽  
Diagnostic Methods ◽  
Charged Dust ◽  
Dust Grains ◽  
Plasma Diagnostic ◽  
Acoustic Oscillations ◽  
Plasma Parameters ◽  
Charge Potential ◽  
Test Charge ◽  
Electrons And Ions

Different plasma diagnostic methods are briefly discussed, and the framework of a test charge technique is effectively used as diagnostic tool for investigating interaction potentials in Lorentzian plasma, whose constituents are the superthermal electrons and ions with negatively charged dust grains. Applying the space-time Fourier transformations to the linearized coupled Vlasov-Poisson equations, a test charge potential is derived with a modified response function due to energetic ions and electrons. For a test charge moving much slower than the dust-thermal speed, there appears a short-range Debye-Hückel (DH) potential decaying exponentially with distance and a long-range far-field (FF) potential as the inverse cube of the distance from test charge. The FF potentials exhibit more localized shielding curves for low-Kappas, and smaller effective shielding length is observed in dusty plasma compared to electron-ion plasma. However, a wakefield (WF) potential is formed behind the test charge when it resonates with dust-acoustic oscillations, whereas a fast moving test charge leads to the Coulomb potential having no shielding around. It is revealed that superthermality and plasma parameters significantly alter the DH, FF, and WF potentials in space plasmas of Saturn’s E-ring, where power-law distributions can be used for energetic electrons and ions in contrast to Maxwellian dust grains.

Energy loss of a test charge in partially ionized dusty plasmas

2000 ◽  
Vol 7 (2) ◽  
pp. 762-765 ◽  
Author(s):  
M. H. Nasim ◽  
M. S. Qaisar ◽  
Arshad M. Mirza ◽  
G. Murtaza ◽  
P. K. Shukla
Keyword(s):  
Energy Loss ◽  
Dusty Plasmas ◽  
Test Charge ◽  
Partially Ionized

Shielding of a slowly moving test charge in dusty plasmas

1994 ◽  
Vol 1 (5) ◽  
pp. 1362-1363 ◽  
Author(s):  
P. K. Shukla
Keyword(s):  
Dusty Plasmas ◽  
Test Charge

Dusty plasmas

2004 ◽  
Vol 174 (5) ◽  
pp. 495 ◽  
Author(s):  
Vladimir E. Fortov ◽  
Aleksei G. Khrapak ◽  
Sergei A. Khrapak ◽  
Vladimir I. Molotkov ◽  
Oleg F. Petrov
Keyword(s):  
Dusty Plasmas

Acoustic Modes of Multi-Ion Dusty Plasmas

2020 ◽  
Vol 76 (9) ◽  
pp. 824-828
Author(s):  
N. Ahmad ◽  
Majeed Ur Rehman ◽  
M. N. S. Qureshi ◽  
Y. Al-Hadeethi ◽  
A. A. Abid ◽  
...  
Keyword(s):  
Dusty Plasmas ◽  
Acoustic Modes
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