A deep learning method to estimate magnetic fields in solar active regions from photospheric continuum images

Xianyong Bai(Chinese Academy of Sciences), Kaifan Ji(Chinese Academy of Sciences), Jie Jiang(Beihang University), Hui Liu(Chinese Academy of Sciences), Yuanyong Deng(Chinese Academy of Sciences), Jiangtao Su(Chinese Academy of Sciences), Jingjing Guo(Chinese Academy of Sciences), Tao Feng(Sichuan University), Yi Bi(Hefei University of Technology), Zhenyu Jin(Chinese Academy of Sciences), Wenda Cao(New Jersey Institute of Technology)
Astronomy and Astrophysics
July 9, 2021
10.1051/0004-6361/202140374
Cited by 6

Related Papers

ON A CORONAL BLOWOUT JET: THE FIRST OBSERVATION OF A SIMULTANEOUSLY PRODUCED BUBBLE-LIKE CME AND A JET-LIKE CME IN A SOLAR EVENT
|The Astrophysical Journal|2012|205
Advanced Space-based Solar Observatory (ASO-S): an overview
|Research in Astronomy and Astrophysics|2019|182
Magnetic Flux Cancellation Associated with the Major Solar Event on 2000 July 14
|The Astrophysical Journal|2001|148
Orientation of the Magnetic Fields in Interplanetary Flux Ropes and Solar Filaments
|The Astrophysical Journal|2001|138
FORMATION OF A DOUBLE-DECKER MAGNETIC FLUX ROPE IN THE SIGMOIDAL SOLAR ACTIVE REGION 11520
|The Astrophysical Journal|2014|133