Study of MHD dynamo effect at the outlet from plasma accelerator in the presence of longitudinal magnetic field

2020 ◽  
Vol 60 (3) ◽  
pp. e201900174
Author(s):  
Andrei N. Kozlov

2008 ◽  
Vol 74 (2) ◽  
pp. 261-286 ◽  
Author(s):  
ANDREY N. KOZLOV

AbstractThe analytic and numerical approaches to the investigation of the two-dimensional steady-state plasma flows are analyzed and compared with reference to a plasma accelerator channel in the presence of a longitudinal magnetic field. The present study continues a cycle of research into the plasma flows in the coaxial channels with the traditional azimuthal magnetic field. The additional longitudinal field opens new possibilities for controlling the dynamic processes and achieving the transonic flows. The research is based on the magnetohydrodynamic equations.



2019 ◽  
Vol 2019 (2) ◽  
pp. 19-21
Author(s):  
A.D. Razmyshlyaev ◽  
◽  
M.V. Ageeva ◽  
E.V. Lavrova ◽  
◽  
...  






2021 ◽  
Vol 1975 (1) ◽  
pp. 012037
Author(s):  
Y Kinoshita ◽  
T Yonenaka ◽  
Y Ichiki ◽  
T Akasaka ◽  
E S Otabe ◽  
...  


2013 ◽  
Vol 9 (S302) ◽  
pp. 381-382
Author(s):  
V. Butkovskaya ◽  
S. Plachinda ◽  
D. Baklanova ◽  
V. Butkovskyi

AbstractWe present the results of the spectropolarimetric study of the classical Cepheid η Aql in 2002, 2004, 2010, and 2012. The longitudinal magnetic field of η Aql was found to be variable with the pulsation cycle of 7.176726 day. The amplitude, phase, and mean value of the field vary from year to year presumably due to stellar rotation or dynamo mechanisms.



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