scholarly journals Ion acoustic instability triggered by finite amplitude polarized waves in the solar wind

2005 ◽  
Vol 110 (A6) ◽  
Author(s):  
L. Gomberoff
Keyword(s):  
Solar Wind ◽  
Finite Amplitude ◽  
Acoustic Instability ◽  
Polarized Waves ◽  
Ion Acoustic

Ion acoustic instability in the presence of plasma turbulence in the solar wind

Solar Physics ◽  
1982 ◽  
Vol 79 (1) ◽  
pp. 187-194
Author(s):  
P. Revathy ◽  
S. R. Prabhakaran Nayar
Keyword(s):  
Solar Wind ◽  
Plasma Turbulence ◽  
Acoustic Instability ◽  
Ion Acoustic

Solar wind heating by heat conduction driven ion acoustic instability

Solar Physics ◽  
1977 ◽  
Vol 52 (2) ◽  
pp. 471-475 ◽  
Author(s):  
P. Revathy ◽  
G. S. Lakhina
Keyword(s):  
Solar Wind ◽  
Heat Conduction ◽  
Acoustic Instability ◽  
Ion Acoustic

Solitary waves in a dusty adiabatic electronegative plasma

2010 ◽  
Vol 76 (3-4) ◽  
pp. 409-418 ◽  
Author(s):  
A. A. MAMUN ◽  
K. S. ASHRAFI ◽  
M. G. M. ANOWAR
Keyword(s):  
Solitary Waves ◽  
Vries Equation ◽  
Negative Ions ◽  
Finite Amplitude ◽  
Reductive Perturbation Method ◽  
Charged Dust ◽  
Electronegative Plasma ◽  
Ion Acoustic ◽  
Basic Features ◽  
Electronegative Plasmas

AbstractThe dust ion-acoustic solitary waves (SWs) in an unmagnetized dusty adiabatic electronegative plasma containing inertialess adiabatic electrons, inertial single charged adiabatic positive and negative ions, and stationary arbitrarily (positively and negatively) charged dust have been theoretically studied. The reductive perturbation method has been employed to derive the Korteweg-de Vries equation which admits an SW solution. The combined effects of the adiabaticity of plasma particles, inertia of positive or negative ions, and presence of positively or negatively charged dust, which are found to significantly modify the basic features of small but finite-amplitude dust-ion-acoustic SWs, are explicitly examined. The implications of our results in space and laboratory dusty electronegative plasmas are briefly discussed.

Coupling of electrostatic ion cyclotron and ion acoustic waves in the solar wind

2016 ◽  
Vol 23 (8) ◽  
pp. 082901 ◽  
Author(s):  
T. Sreeraj ◽  
S. V. Singh ◽  
G. S. Lakhina
Keyword(s):  
Solar Wind ◽  
Acoustic Waves ◽  
Ion Acoustic Waves ◽  
Ion Acoustic ◽  
Ion Cyclotron

Ion acoustic waves in the solar wind

1978 ◽  
Vol 83 (A1) ◽  
pp. 58-74 ◽  
Author(s):  
D. A. Gurnett ◽  
L. A. Frank
Keyword(s):  
Solar Wind ◽  
Acoustic Waves ◽  
Ion Acoustic Waves ◽  
Ion Acoustic

A linear and quasi-linear investigation of the crossfield current-driven ion-acoustic instability

1982 ◽  
Vol 28 (2) ◽  
pp. 267-279 ◽  
Author(s):  
R. Bharuthram ◽  
M. A. Hellberg
Keyword(s):  
Linear Growth ◽  
Velocity Distribution Function ◽  
Linear Growth Rate ◽  
Particle Diffusion ◽  
Anomalous Resistivity ◽  
Heating Rates ◽  
Ion Heating ◽  
Acoustic Instability ◽  
Ion Acoustic ◽  
Drift Instability

The linear growth rate of the crossfield current-driven ion-acoustic instability is obtained for any equilibrium particle velocity distribution function of the type . Quasi-linear theory is then used to investigate the saturation of the instability. Several associated features, namely, particle diffusion in velocity space, anomalous resistivity, energy distribution and electron and ion heating rates are evaluated for a Maxwellian distribution. Finally, a brief comparison is made with the heating rates associated with the electron cyclotron drift instability.

scholarly journals Brief Communication: The double layer in the separatrix region during magnetic reconnection

2015 ◽  
Vol 22 (2) ◽  
pp. 167-171
Author(s):  
J. Guo ◽  
B. Yu
Keyword(s):  
Electron Beam ◽  
Magnetic Reconnection ◽  
Double Layer ◽  
Particle In Cell ◽  
Acoustic Instability ◽  
Ion Acoustic ◽  
Evolution Stage ◽  
Spatial Size ◽  
Electron Holes ◽  
Observation Results

Abstract. With two-dimensional (2-D) particle-in-cell (PIC) simulations we investigate the evolution of the double layer (DL) driven by magnetic reconnection. Our results show that an electron beam can be generated in the separatrix region as magnetic reconnection proceeds. This electron beam could trigger the ion-acoustic instability; as a result, a DL accompanied with electron holes (EHs) can be found during the nonlinear evolution stage of this instability. The spatial size of the DL is about 10 Debye lengths. This DL propagates along the magnetic field at a velocity of about the ion-acoustic speed, which is consistent with the observation results.

scholarly journals First-year ion-acoustic wave observations in the solar wind by the RPW/TDS instrument on board Solar Orbiter

2021 ◽  
Author(s):  
D. Písa ◽  
J. Souček ◽  
O. Santolík ◽  
M. Hanzelka ◽  
G. Nicolaou ◽  
...  
Keyword(s):  
Solar Wind ◽  
Acoustic Wave ◽  
First Year ◽  
Ion Acoustic Wave ◽  
Ion Acoustic
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