Measurements of Three‐dimensional Coronal Magnetic Fields from Coordinated Extreme‐Ultraviolet and Radio Observations of a Solar Active Region Sunspot

2002 ◽  
Vol 574 (1) ◽  
pp. 453-466 ◽  
Author(s):  
Jeffrey W. Brosius ◽  
Enrico Landi ◽  
John W. Cook ◽  
Jeffrey S. Newmark ◽  
N. Gopalswamy ◽  
...  
2013 ◽  
Vol 8 (S300) ◽  
pp. 479-480
Author(s):  
Jie Zhao ◽  
Hui Li ◽  
Etienne Pariat ◽  
Brigitte Schmieder ◽  
Yang Guo ◽  
...  

AbstractWith the cylindrical equal area (CEA) projection data from the Helioseismic and Magnetic Imager (HMI) onboard the Solar Dynamics Observatory (SDO), we reconstructed the three-dimensional (3D) magnetic fields in the corona, using a non-linear force-free field (NLFFF) extrapolation method every 12 minutes during five days, to calculate the squashing degree factor Q in the volume. The results show that this AR has an hyperbolic flux tube (HFT) configuration, a typical topology of quadrupole, which is stable even during the two large flares (M6.6 and X2.2 class flares).


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 531 (2) ◽  
pp. 1129-1149 ◽  
Author(s):  
Markus J. Aschwanden ◽  
David Alexander ◽  
Neal Hurlburt ◽  
Jeffrey S. Newmark ◽  
Werner M. Neupert ◽  
...  

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 ◽  
...  

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