scholarly journals Solar Active Region and Quiet‐Sun Extreme‐Ultraviolet Spectra from SERTS‐95

1998 ◽  
Vol 119 (2) ◽  
pp. 255-276 ◽  
Author(s):  
Jeffrey W. Brosius ◽  
Joseph M. Davila ◽  
Roger J. Thomas
1996 ◽  
Vol 106 ◽  
pp. 143 ◽  
Author(s):  
Jeffrey W. Brosius ◽  
Joseph M. Davila ◽  
Roger J. Thomas ◽  
Brunella C. Monsignori-Fossi

2003 ◽  
Vol 346 (1) ◽  
pp. 58-62 ◽  
Author(s):  
F. P. Keenan ◽  
A. C. Katsiyannis ◽  
R. H. G. Reid ◽  
A. K. Pradhan ◽  
H. L. Zhang ◽  
...  

2000 ◽  
Vol 543 (2) ◽  
pp. 1016-1026 ◽  
Author(s):  
Jeffrey W. Brosius ◽  
Roger J. Thomas ◽  
Joseph M. Davila ◽  
Enrico Landi

2002 ◽  
Vol 566 (1) ◽  
pp. 521-527 ◽  
Author(s):  
F. P. Keenan ◽  
A. C. Katsiyannis ◽  
R. S. I. Ryans ◽  
R. H. G. Reid ◽  
H. L. Zhang ◽  
...  

2015 ◽  
Vol 11 (S320) ◽  
pp. 185-190
Author(s):  
Bin Zhang ◽  
Jun Zhang ◽  
Shuhong Yang ◽  
Ting Li ◽  
Yuzong Zhang ◽  
...  

AbstractUsing the Solar Dynamics Observatory observations, we study the evolution of an emerging active region (EAR) and its reconnection with the quiet Sun. The EAR continuously interacts with the surrounding quiet region, and dark ribbons at the boundary of the EAR and the quiet Sun are observed. The extreme-ultraviolet observations show that the regions swept by the dark ribbons are brightened and the temperature increases. These results reveal that there exists an uninterrupted magnetic reconnection between the EAR and the quiet region and the released energy heats the corona of the quiet Sun. The dark ribbons are suggested to correspond to the interface of the reconnected fields and the undisturbed ones. The dark ribbon propagates outward, and this phenomenon is considered as a dark wave.


2002 ◽  
Vol 574 (1) ◽  
pp. 453-466 ◽  
Author(s):  
Jeffrey W. Brosius ◽  
Enrico Landi ◽  
John W. Cook ◽  
Jeffrey S. Newmark ◽  
N. Gopalswamy ◽  
...  

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