Decay of the coronal magnetic field can release sufficient energy to power a solar flare GD Fleishman, DE Gary, B Chen, N Kuroda, S Yu, GM Nita Science 367 (6475), 278-280, 2020 | 113 | 2020 |
Element abundances: a new diagnostic for the solar wind JM Laming, A Vourlidas, C Korendyke, D Chua, SR Cranmer, YK Ko, ... The Astrophysical Journal 879 (2), 124, 2019 | 72 | 2019 |
Three-dimensional forward-fit modeling of the hard X-ray and microwave emissions of the 2015 June 22 M6. 5 Flare N Kuroda, DE Gary, H Wang, GD Fleishman, GM Nita, J Jing The Astrophysical Journal 852 (1), 32, 2018 | 30 | 2018 |
Revealing the evolution of non-thermal electrons in solar flares using 3D modeling GD Fleishman, GM Nita, N Kuroda, S Jia, K Tong, RR Wen, Z Zhizhuo The Astrophysical Journal 859 (1), 17, 2018 | 16 | 2018 |
Evolution of flare-accelerated electrons quantified by spatially resolved analysis N Kuroda, GD Fleishman, DE Gary, GM Nita, B Chen, S Yu Frontiers in Astronomy and Space Sciences 7, 22, 2020 | 8 | 2020 |
Observation of the 2011-02-15 X2. 2 Flare in the Hard X-Ray and Microwave N Kuroda, H Wang, DE Gary The Astrophysical Journal 807 (2), 124, 2015 | 4 | 2015 |