scholarly journals Fast Magnetic Reconnection in Laser-Produced Plasma Bubbles

2011 ◽  
Vol 106 (21) ◽  
Author(s):  
W. Fox ◽  
A. Bhattacharjee ◽  
K. Germaschewski
2018 ◽  
Vol 25 (9) ◽  
pp. 093105 ◽  
Author(s):  
K. V. Lezhnin ◽  
W. Fox ◽  
J. Matteucci ◽  
D. B. Schaeffer ◽  
A. Bhattacharjee ◽  
...  

2017 ◽  
Vol 24 (10) ◽  
pp. 102101 ◽  
Author(s):  
Kai Huang ◽  
Quanming Lu ◽  
Can Huang ◽  
Quanli Dong ◽  
Huanyu Wang ◽  
...  

2012 ◽  
Vol 86 (5) ◽  
Author(s):  
M. J. Rosenberg ◽  
J. S. Ross ◽  
C. K. Li ◽  
R. P. J. Town ◽  
F. H. Séguin ◽  
...  

2017 ◽  
Vol 24 (4) ◽  
pp. 041406 ◽  
Author(s):  
Kai Huang ◽  
Can Huang ◽  
Quanli Dong ◽  
Quanming Lu ◽  
San Lu ◽  
...  

2014 ◽  
Vol 113 (10) ◽  
Author(s):  
G. Fiksel ◽  
W. Fox ◽  
A. Bhattacharjee ◽  
D. H. Barnak ◽  
P.-Y. Chang ◽  
...  

2012 ◽  
Vol 78 (4) ◽  
pp. 497-500 ◽  
Author(s):  
Q.-L. DONG ◽  
D.-W. YUAN ◽  
S.-J. WANG ◽  
Y. T. LI ◽  
X. LIU ◽  
...  

AbstractThe magnetic reconnection (MR) configuration was constructed by using two approaching laser-produced plasma bubbles. The characteristics of the MR current sheet were investigated. The driving energy of the laser pulse affects the type of the current sheet. The experiments present “Y-type” and “X-type” current sheets for larger and smaller driving energy, respectively. The energetic electrons were found to be well-collimated. The formation and ejection of plasmoid from the “Y-type” current sheet was expected to enhance the number of accelerated electrons.


2019 ◽  
Vol 15 (S354) ◽  
pp. 189-194
Author(s):  
J. B. Climent ◽  
J. C. Guirado ◽  
R. Azulay ◽  
J. M. Marcaide

AbstractWe report the results of three VLBI observations of the pre-main-sequence star AB Doradus A at 8.4 GHz. With almost three years between consecutive observations, we found a complex structure at the expected position of this star for all epochs. Maps at epochs 2007 and 2010 show a double core-halo morphology while the 2013 map reveals three emission peaks with separations between 5 and 18 stellar radii. Furthermore, all maps show a clear variation of the source structure within the observing time. We consider a number of hypothesis in order to explain such observations, mainly: magnetic reconnection in loops on the polar cap, a more general loop scenario and a close companion to AB Dor A.


2006 ◽  
Vol 133 ◽  
pp. 525-527
Author(s):  
V. S. Belyaev ◽  
A. Ya. Faenov ◽  
A. I. Magunov ◽  
A. P. Matafonov ◽  
T. A. Pikuz ◽  
...  

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