Measurement of the Hall Dynamo Effect during Magnetic Reconnection in a High-Temperature Plasma

2004 ◽  
Vol 93 (4) ◽  
Author(s):  
W. X. Ding ◽  
D. L. Brower ◽  
D. Craig ◽  
B. H. Deng ◽  
G. Fiksel ◽  
...  
2011 ◽  
Vol 107 (6) ◽  
Author(s):  
R. M. Magee ◽  
D. J. Den Hartog ◽  
S. T. A. Kumar ◽  
A. F. Almagri ◽  
B. E. Chapman ◽  
...  

1981 ◽  
Vol 9 (3) ◽  
pp. 237-252 ◽  
Author(s):  
Mitsuo MAEDA ◽  
Katsunori MURAOKA ◽  
Makoto HAMAMOTO ◽  
Masanori AKAZAKI ◽  
Yasushi MIYAZOE

1985 ◽  
Vol 85 ◽  
pp. 365-368
Author(s):  
S. Ibadov

AbstractThe intensity of solar X-radiation scattered by a comet is calculated and compared to the proper X-radiation of the comet due to impacts of cometary and interplanetary dust particles. Detection of X-radiation of dusty comets at small heliocentric distances (R ≤ 1 a.u.) is found to be an indicator of high-temperature plasma generation as result of grain collisions.


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