Effects of transverse magnetic field upon the temperature distribution, cross-section shape, and profile of a cross-flow arc

1970 ◽  
Author(s):  
A. BAKER
1960 ◽  
Vol 7 (2) ◽  
pp. 287-301 ◽  
Author(s):  
Joseph L. Neuringer

The possibility exists of directly using the plasma, resulting from a controlled fusion reaction, to generate electricity by electromagnetic induction. Two special cases of a more general problem are considered here: (1)the extraction of optimum power from the steady one-dimensional flow of an incompressible inviscid plasma across a uniform transverse magnetic field in an externally loaded channel of arbitrarily varying cross-section, and (2) the extraction of optimum power from the steady one-dimensional flow of a compressible inviscid plasma across a uniform transverse magnetic field in a channel of uniform cross-section. In each case, the magnitude of the required external loading at optimum power operation is determined as a function of the parameters which characterize the hydromagnetic interaction. Also determined are the magnitudes of the terminal voltate, power, fluid mechanical to electrical conversion efficiency, and the variation of the fluid dynamical variables along the channel at optimum power.


AIAA Journal ◽  
1971 ◽  
Vol 9 (8) ◽  
pp. 1441-1446 ◽  
Author(s):  
DAVID M. BENENSON ◽  
A. J. BAKER

2007 ◽  
Vol 25 (7) ◽  
pp. 1471-1476 ◽  
Author(s):  
Y. C. Zhang ◽  
Z. X. Liu ◽  
C. Shen ◽  
A. Fazakerley ◽  
M. Dunlop ◽  
...  

Abstract. We investigate the magnetic structure of a small earthward-moving flux rope observed by Cluster in the near-Earth plasma sheet through application of the Grad-Shafranov (GS) technique to reconstruct the transverse magnetic field distribution perpendicular to the flux rope axis at X=−14.75 RE. We find that the principal axis of the flux rope lies approximately along the dawn-dusk direction and that the diameter of the flux rope is about 1.5 RE. There is a strong duskward core magnetic field in the center of the flux rope. According to the AE index, there is no obvious substorm associated with the magnetic flux rope. Recent studies indicate that the formation of the flux rope in the plasma sheet can be understood in terms of simultaneous reconnection at multiple X-line points in the near-tail. The distribution of the transverse magnetic field on the cross section is the asymmetric circles, which requires that the reconnections at multiple X-line points occur. So our results also provide additional evidence for the occurrence of multiple-X line reconnection in the magnetotail.


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