Hysteresis losses of multifilament superconductors in superimposed dc and ac magnetic fields

Cryogenics ◽  
1981 ◽  
Vol 21 (10) ◽  
pp. 593-597 ◽  
Author(s):  
K. Kwasnitza ◽  
P. Bruzzone
2002 ◽  
Vol 372-376 ◽  
pp. 1739-1742
Author(s):  
A. Rastogi ◽  
H. Yamasaki ◽  
Y. Iijima ◽  
K. Kakimoto ◽  
K. Takeda

2008 ◽  
Vol 468 (15-20) ◽  
pp. 1714-1717 ◽  
Author(s):  
M. Suenaga ◽  
M. Iwakuma ◽  
T. Sueyoshi ◽  
T. Izumi ◽  
M. Mimura ◽  
...  

2008 ◽  
Vol 97 ◽  
pp. 012025 ◽  
Author(s):  
M Suenaga ◽  
M Iwakuma ◽  
T Sueyoshi ◽  
T Izumi ◽  
M Mimura ◽  
...  

2014 ◽  
Vol 506 ◽  
pp. 133-137 ◽  
Author(s):  
N. Magnusson ◽  
A.B. Abrahamsen ◽  
D. Liu ◽  
M. Runde ◽  
H. Polinder

Author(s):  
Muyong Kim ◽  
Heeyeon Park ◽  
Chan Kim ◽  
Sang-Kook Park ◽  
H.-C. Ri

1994 ◽  
Vol 144 ◽  
pp. 559-564
Author(s):  
P. Ambrož ◽  
J. Sýkora

AbstractWe were successful in observing the solar corona during five solar eclipses (1973-1991). For the eclipse days the coronal magnetic field was calculated by extrapolation from the photosphere. Comparison of the observed and calculated coronal structures is carried out and some peculiarities of this comparison, related to the different phases of the solar cycle, are presented.


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