Ramp rate instability of multifilamentary superconductors due to longitudinal magnetic field

1997 ◽  
Vol 7 (2) ◽  
pp. 235-238 ◽  
Author(s):  
N. Banno ◽  
N. Amemiya ◽  
K. Kajikawa ◽  
H. Tateishi
Keyword(s):  
Magnetic Field ◽  
Longitudinal Magnetic Field ◽  
Ramp Rate ◽  
Multifilamentary Superconductors

Refinement of metal structure in arc surfacing under the effect of longitudinal magnetic field

2019 ◽  
Vol 2019 (2) ◽  
pp. 19-21
Author(s):  
A.D. Razmyshlyaev ◽  
◽  
M.V. Ageeva ◽  
E.V. Lavrova ◽  
◽  
...  
Keyword(s):  
Magnetic Field ◽  
Longitudinal Magnetic Field ◽  
Metal Structure

scholarly journals Design and evaluation of 10-kA class superconducting DC power cable based on longitudinal magnetic field effect

2021 ◽  
Vol 1975 (1) ◽  
pp. 012037
Author(s):  
Y Kinoshita ◽  
T Yonenaka ◽  
Y Ichiki ◽  
T Akasaka ◽  
E S Otabe ◽  
...  
Keyword(s):  
Magnetic Field ◽  
Field Effect ◽  
Longitudinal Magnetic Field ◽  
Magnetic Field Effect ◽  
Power Cable ◽  
Dc Power

scholarly journals Magnetic field of the classical Cepheid η Aql: new results

2013 ◽  
Vol 9 (S302) ◽  
pp. 381-382
Author(s):  
V. Butkovskaya ◽  
S. Plachinda ◽  
D. Baklanova ◽  
V. Butkovskyi
Keyword(s):  
Magnetic Field ◽  
Longitudinal Magnetic Field ◽  
Mean Value ◽  
Stellar Rotation ◽  
Classical Cepheid ◽  
Pulsation Cycle

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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