Solar prominence model based on eigenvalue solutions. II - Filaments in the vertical magnetic fields

1989 ◽  
Vol 336 ◽  
pp. 1041 ◽  
Author(s):  
Vladimir A. Osherovich
2020 ◽  
Vol 10 (1) ◽  
Author(s):  
Anang Dadhich ◽  
Enric Pardo

Abstract Superconducting stacks and bulks can act as very strong magnets (more than 17 T), but they lose their magnetization in the presence of alternating (or ripple) transverse magnetic fields, due to the dynamic magneto-resistance. This demagnetization is a major concern for applications requiring high run times, such as motors and generators, where ripple fields are of high amplitude and frequency. We have developed a numerical model based on dynamic magneto-resistance that is much faster than the conventional Power-Law-resistivity model, enabling us to simulate high number of cycles with the same accuracy. We simulate demagnetization behavior of superconducting stacks made of 10–100 tapes for up to 2 million cycles of applied ripple field. We found that for high number of cycles, the trapped field reaches non-zero stationary values for both superconducting bulks and stacks; as long as the ripple field amplitudes are below the parallel penetration field, being determined by the penetration field for a single tape in stacks. Bulks keep substantial stationary values for much higher ripple field amplitudes than the stacks, being relevant for high number of cycles. However, for low number of cycles, stacks lose much less magnetization as compared to bulks.


1993 ◽  
Vol 141 ◽  
pp. 138-142
Author(s):  
G. S. Choe ◽  
L. C. Lee

AbstractNumerical simulations of solar prominence formation are presented employing photospheric horizontal motions as boundary conditions. Three different combinations of magnetic field configurations and footpoint motions are considered: (1) a bipolar arcade with a footpoint shear, (2) an arcade exposed to a shearing and converging motion, (3) two adjacent arcades undergoing a shearing and converging motion. In each case, it is found that the dynamic evolution of magnetic fields can force the plasma into a thermal instability leading to the formation of a prominence.


1997 ◽  
Vol 11 (26n27) ◽  
pp. 1133-1151 ◽  
Author(s):  
V. M. Svistunov ◽  
T. Aomine ◽  
T. Fukami ◽  
T. Yamamoto ◽  
A. I. D'Yachenko

Models describing the appearance of an abnormal hysteresis in the critical current of granular superconductors are analyzed. It has been revealed that the most suitable for High T c Superconductors ( H T c S ) is a model based on an irreversibility of the grain surface current that determines the critical current of the Josephson weak links or depairing current of narrow superconducting part in ( H T c S ) oxides. This leads to the irreversibility phenomena in ( H T c S ) at the high magnetic fields H≫ H c1 .


Sign in / Sign up

Export Citation Format

Share Document