The Radio Signature of Magnetic Reconnection for the M-Class Flare of 2004 November 1

2007 ◽  
Vol 672 (2) ◽  
pp. L131-L134 ◽  
Author(s):  
Guangli Huang ◽  
Haisheng Ji ◽  
Guiping Wu
Keyword(s):  
Magnetic Reconnection ◽  
Radio Signature ◽  
Class Flare

scholarly journals A Two-step Magnetic Reconnection in a Confined X-class Flare in Solar Active Region 12673

2019 ◽  
Vol 870 (2) ◽  
pp. 97 ◽  
Author(s):  
Peng Zou ◽  
Chaowei Jiang ◽  
Xueshang Feng ◽  
Pingbing Zuo ◽  
Yi Wang ◽  
...  
Keyword(s):  
Active Region ◽  
Magnetic Reconnection ◽  
Solar Active Region ◽  
Class Flare

scholarly journals Magnetic Reconnection Rates and Energy Release in a Confined X-class Flare

Solar Physics ◽  
2015 ◽  
Vol 290 (10) ◽  
pp. 2923-2942 ◽  
Author(s):  
A. M. Veronig ◽  
W. Polanec
Keyword(s):  
Magnetic Reconnection ◽  
Energy Release ◽  
Class Flare

scholarly journals Signatures of magnetic reconnection during the evolutionary phases of a prominence eruption and associated X1.8 flare

2013 ◽  
Vol 8 (S300) ◽  
pp. 424-425
Author(s):  
Bhuwan Joshi ◽  
Upendra Kushwaha ◽  
KyungSuk Cho ◽  
Astrid Veronig
Keyword(s):  
Active Region ◽  
Magnetic Reconnection ◽  
Current Sheet ◽  
Morphological Evolution ◽  
Flare Activity ◽  
Active Region Noaa ◽  
Triggering Mechanism ◽  
Filament Eruption ◽  
Multi Wavelength ◽  
Class Flare

AbstractIn this paper, we present RHESSI and TRACE observations of multiple flare activity that occurred in the active region NOAA 10656 on 2004 August 18. Out of four successive flares, there were three events of class-C while the final event was a major X1.8 solar eruptive flare. During localized C-class flares, the filament undergoes slow yet crucial morphological evolution. The filament eruption is accompanied with an X1.8 flare during which multiple HXR bursts are observed up to 100–300 keV energies. From the location, timing, strength, and spectrum of HXR emission, we conclude that the prominence eruption is driven by the distinct events of magnetic reconnection occurring in the current sheet below the erupting prominence. These multi-wavelength observations also provide evidence for tether-cutting reconnection as the triggering mechanism for filament eruption and associated X-class flare.

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 Plasmas

2000 ◽  
Author(s):  
Dieter Biskamp
Keyword(s):  
Magnetic Reconnection

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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