The effects of nonuniform magnetic field strength on density flux and test particle transport in drift wave turbulence

2009 ◽  
Vol 16 (7) ◽  
pp. 072306 ◽  
Author(s):  
J. M. Dewhurst ◽  
B. Hnat ◽  
R. O. Dendy
Keyword(s):  
Magnetic Field ◽  
Field Strength ◽  
Magnetic Field Strength ◽  
Test Particle ◽  
Particle Transport ◽  
Nonuniform Magnetic Field ◽  
Wave Turbulence ◽  
Drift Wave Turbulence ◽  
Drift Wave

scholarly journals Experimental observation of drift wave turbulence in an inhomogeneous six-pole cusp magnetic field of MPD

2018 ◽  
Vol 25 (11) ◽  
pp. 112114 ◽  
Author(s):  
A. D. Patel ◽  
M. Sharma ◽  
R. Ganesh ◽  
N. Ramasubramanian ◽  
P. K. Chattopadhyay
Keyword(s):  
Magnetic Field ◽  
Experimental Observation ◽  
Wave Turbulence ◽  
Drift Wave Turbulence ◽  
Drift Wave ◽  
Cusp Magnetic Field

On the Configuration of the Magnetic Field of β CrB

1976 ◽  
Vol 32 ◽  
pp. 613-622
Author(s):  
I.A. Aslanov ◽  
Yu.S. Rustamov
Keyword(s):  
Magnetic Field ◽  
Field Strength ◽  
Radial Velocity ◽  
Magnetic Field Strength ◽  
Complex Shape ◽  
Rotation Period ◽  
Field Variation ◽  
Magnetic Field Variation ◽  
Secular Variations ◽  
The Magnetic Field

SummaryMeasurements of the radial velocities and magnetic field strength of β CrB were carried out. It is shown that there is a variability with the rotation period different for various elements. The curve of the magnetic field variation measured from lines of 5 different elements: FeI, CrI, CrII, TiII, ScII and CaI has a complex shape specific for each element. This may be due to the presence of magnetic spots on the stellar surface. A comparison with the radial velocity curves suggests the presence of a least 4 spots of Ti and Cr coinciding with magnetic spots. A change of the magnetic field with optical depth is shown. The curve of the Heffvariation with the rotation period is given. A possibility of secular variations of the magnetic field is shown.

Sign in / Sign up

Export Citation Format

Share Document