scholarly journals Electron dynamics in collisionless magnetic reconnection

2011 ◽  
Vol 56 (12) ◽  
pp. 1174-1181 ◽  
Author(s):  
QuanMing Lu ◽  
RongSheng Wang ◽  
JinLin Xie ◽  
Can Huang ◽  
San Lu ◽  
...  
2015 ◽  
Vol 22 (9) ◽  
pp. 092901 ◽  
Author(s):  
E. Cazzola ◽  
M. E. Innocenti ◽  
S. Markidis ◽  
M. V. Goldman ◽  
D. L. Newman ◽  
...  

2014 ◽  
Vol 112 (21) ◽  
Author(s):  
D. B. Graham ◽  
Yu. V. Khotyaintsev ◽  
A. Vaivads ◽  
M. André ◽  
A. N. Fazakerley

2018 ◽  
Vol 9 (1) ◽  
Author(s):  
Y. Kuramitsu ◽  
T. Moritaka ◽  
Y. Sakawa ◽  
T. Morita ◽  
T. Sano ◽  
...  

2013 ◽  
Vol 118 (12) ◽  
pp. 7703-7713 ◽  
Author(s):  
T. Nagai ◽  
S. Zenitani ◽  
I. Shinohara ◽  
R. Nakamura ◽  
M. Fujimoto ◽  
...  

2017 ◽  
Vol 122 (7) ◽  
pp. 7396-7413 ◽  
Author(s):  
Seiji Zenitani ◽  
Hiroshi Hasegawa ◽  
Tsugunobu Nagai

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.


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