Gyrokinetic investigations on entropy modes in dipole magnetic field confined plasmas with an anisotropic temperature

2019 ◽  
Vol 26 (3) ◽  
pp. 032113 ◽  
Author(s):  
Liang Qian ◽  
Zhibin Wang ◽  
Xiaogang Wang
Keyword(s):  
Magnetic Field ◽  
Confined Plasmas ◽  
Anisotropic Temperature ◽  
Dipole Magnetic Field

Particle balance in a steady state plasma in a dipole magnetic field

2019 ◽  
Vol 1 (4) ◽  
pp. 045005 ◽  
Author(s):  
Anuj Ram Baitha ◽  
Ayesha Nanda ◽  
Sargam Hunjan ◽  
Sudeep Bhattacharjee
Keyword(s):  
Magnetic Field ◽  
Steady State ◽  
Dipole Magnetic Field ◽  
Particle Balance ◽  
State Plasma

scholarly journals Spin-down rate and inferred dipole magnetic field of the soft gamma-ray repeater SGR 1627-41

2009 ◽  
Vol 399 (1) ◽  
pp. L44-L48 ◽  
Author(s):  
P. Esposito ◽  
M. Burgay ◽  
A. Possenti ◽  
R. Turolla ◽  
S. Zane ◽  
...  
Keyword(s):  
Magnetic Field ◽  
Gamma Ray ◽  
Dipole Magnetic Field

scholarly journals Modeling ULF waves in a compressed dipole magnetic field

2010 ◽  
Vol 115 (A10) ◽  
pp. n/a-n/a ◽  
Author(s):  
A. W. Degeling ◽  
R. Rankin ◽  
K. Kabin ◽  
I. J. Rae ◽  
F. R. Fenrich
Keyword(s):  
Magnetic Field ◽  
Ulf Waves ◽  
Dipole Magnetic Field

scholarly journals Radio Emission Model of a 'Typical' Pulsar

1987 ◽  
Vol 40 (6) ◽  
pp. 755 ◽  
Author(s):  
AZ Kazbegi ◽  
GZ Machabeli ◽  
G Melikidze
Keyword(s):  
Magnetic Field ◽  
Electromagnetic Waves ◽  
Emission Model ◽  
Radio Waves ◽  
Resonance Case ◽  
Pulsar Magnetosphere ◽  
Pulsar Emission ◽  
Dipole Magnetic Field ◽  
New Type ◽  
The Magnetic Field

The generation of radio waves in the plasma of the pulsar magnetosphere is considered taking into account the inhomogeneity of the dipole magnetic field. It is shown that the growth rate of the instability of the electromagnetic waves calculated in the non-resonance case turns out to be of the order of 1/ TO (where TO is the time of plasma escape from the light cylinder). However, the generation of electromagnetic waves from a new type Cherenkov resonance is possible, occurring when the particles have transverse velocities caused by the drift due to the inhomogeneity of the magnetic field. Estimates show that the development of this type of instability is possible only for pulsars with ages which exceed 104 yr. We make an attempt to explain some peculiarities of 'typical' pulsar emission on the basis of the model developed.

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