scholarly journals Relativistic electron production during driven magnetic reconnection

2006 ◽  
Vol 33 (13) ◽  
Author(s):  
P. L. Pritchett
Keyword(s):  
Magnetic Reconnection ◽  
Relativistic Electron ◽  
Electron Production

The global efficiency of relativistic electron production in the Earth's magnetosphere

2001 ◽  
Vol 106 (A9) ◽  
pp. 19169-19178 ◽  
Author(s):  
D. N. Baker ◽  
S. G. Kanekal ◽  
J. B. Blake ◽  
T. I. Pulkkinen
Keyword(s):  
Relativistic Electron ◽  
Earth’S Magnetosphere ◽  
Global Efficiency ◽  
Electron Production ◽  
Earth's Magnetosphere

scholarly journals Relativistic-electron-driven magnetic reconnection in the laboratory

2018 ◽  
Vol 98 (4) ◽  
Author(s):  
A. E. Raymond ◽  
C. F. Dong ◽  
A. McKelvey ◽  
C. Zulick ◽  
N. Alexander ◽  
...  
Keyword(s):  
Magnetic Reconnection ◽  
Relativistic Electron

scholarly journals Relativistic electron production in the ORMAK device

1973 ◽  
Author(s):  
D. A. Spong ◽  
J. F. Clarke ◽  
J. A. Rome
Keyword(s):  
Relativistic Electron ◽  
Electron Production

Relativistic electron production in solar flare

1995 ◽  
Author(s):  
P. N. Okeke ◽  
K. Ohki
Keyword(s):  
Solar Flare ◽  
Relativistic Electron ◽  
Electron Production

A large rotating structure around AB Doradus A at VLBI scale

2019 ◽  
Vol 15 (S354) ◽  
pp. 189-194
Author(s):  
J. B. Climent ◽  
J. C. Guirado ◽  
R. Azulay ◽  
J. M. Marcaide
Keyword(s):  
Magnetic Reconnection ◽  
Main Sequence ◽  
Complex Structure ◽  
Main Sequence Star ◽  
Polar Cap ◽  
Vlbi Observations ◽  
Rotating Structure ◽  
Source Structure ◽  
Expected Position

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.

Magnetic reconnection in solar flares

2010 ◽  
Vol 180 (9) ◽  
pp. 997 ◽  
Author(s):  
B.V. Somov
Keyword(s):  
Magnetic Reconnection ◽  
Solar Flares

Experimental Investigation of Ion Mass Dependency of Magnetic Reconnection Outflow by using High Precision Ion Doppler Spectroscopy

2014 ◽  
Vol 134 (5) ◽  
pp. 352-353
Author(s):  
Hirotaka Oka ◽  
Hiroshi Tanabe ◽  
Masanobu Annoura ◽  
Michiaki Inomoto ◽  
Yasushi Ono
Keyword(s):  
Experimental Investigation ◽  
Magnetic Reconnection ◽  
High Precision ◽  
Doppler Spectroscopy
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