Publications of K. E. Yang


A list of publications authored or co-authored by K. E. Yang, derived from the SAO/NASA Astrophysics Data System (ADS). The number in brackets after each title indicates the number of citations that the paper has received.

Orcid ID: 0000-0002-7663-7652

List of publications ordered by citations
Number of papers: 29 (refereed: 29)
No. of citations: 688
First author papers: 7 (refereed: 7)

2025

  1. Spectropolarimetric Inversion in Four Dimensions with Deep Learning (SPIn4D). II. A Physics-informed Machine Learning Method for 3D Solar Photosphere Reconstruction [0]
    Yang, Kai E., Sun, Xudong, Tarr, Lucas A., Liu, Jiayi, Sadowski, Peter, Dodds, S. Curt, Rempel, Matthias, Jaeggli, Sarah A., Schad, Thomas A., Cunnyngham, Ian, Glaser, Yannik & Wolniewicz, Linnea, ApJ, 995, 146
  2. Analyzing the Morphology of Late-phase Stellar Flares from G-, K-, and M-type Stars [3]
    Yudovich, Denise G., Yang, Kai E. & Sun, Xudong, ApJ, 984, 186

2024

  1. Stellar flares are far-ultraviolet luminous [23]
    Berger, Vera L., Hinkle, Jason T., Tucker, Michael A., Shappee, Benjamin J., van Saders, Jennifer L., Huber, Daniel, Reep, Jeffrey W., Sun, Xudong & Yang, Kai E., MNRAS, 532, 4436
  2. Superflare rate variability on M dwarfs [4]
    Crowley, James, Wheatland, Michael S. & Yang, Kai, MNRAS, 530, 457
  3. Spectropolarimetric Inversion in Four Dimensions with Deep Learning (SPIn4D). I. Overview, Magnetohydrodynamic Modeling, and Stokes Profile Synthesis [7]
    Yang, Kai E., Tarr, Lucas A., Rempel, Matthias, Dodds, S. Curt, Jaeggli, Sarah A., Sadowski, Peter, Schad, Thomas A., Cunnyngham, Ian, Liu, Jiayi, Glaser, Yannik & Sun, Xudong, ApJ, 976, 204

2023

  1. Data-constrained Magnetohydrodynamic Simulation of an Intermediate Solar Filament Eruption [8]
    Guo, Yang, Guo, Jinhan, Ni, Yiwei, Ding, M. D., Chen, P. F., Xia, Chun, Keppens, Rony & Yang, Kai E., ApJ, 958, 25
  2. Investigating Pre-eruptive Magnetic Properties at the Footprints of Erupting Magnetic Flux Ropes [14]
    Wang, Wensi, Qiu, Jiong, Liu, Rui, Zhu, Chunming, Yang, Kai E., Hu, Qiang & Wang, Yuming, ApJ, 943, 80
  3. A Possible Mechanism for the "Late Phase" in Stellar White-light Flares [17]
    Yang, Kai E., Sun, Xudong, Kerr, Graham S. & Hudson, Hugh S., ApJ, 959, 54

2022

  1. Observed Rate Variations in Superflaring G-type Stars [7]
    Crowley, James, Wheatland, Michael S. & Yang, Kai, ApJ, 941, 193

2020

  1. Reconstructing Highly-twisted Magnetic Fields [2]
    Demcsak, Victor M., Wheatland, Michael S., Mastrano, Alpha & Yang, Kai E., Solar Physics, 295, 116
  2. Self-consistent Nonlinear Force-Free Field Reconstruction from Weighted Boundary Conditions [5]
    Mastrano, A., Yang, K. E. & Wheatland, M. S., Solar Physics, 295, 97
  3. Relative Magnetic Helicity Based on a Periodic Potential Field [4]
    Yang, Kai E., Wheatland, Michael S. & Gilchrist, Stuart A., ApJ, 894, 151

2019

  1. Evolution of a Magnetic Flux Rope toward Eruption [33]
    Wang, Wensi, Zhu, Chunming, Qiu, Jiong, Liu, Rui, Yang, Kai E. & Hu, Qiang, ApJ, 871, 25

2018

  1. Extremely Large Extreme-ultraviolet Late Phase Powered by Intense Early Heating in a Non-eruptive Solar Flare [21]
    Dai, Yu, Ding, Mingde, Zong, Weiguo & Yang, Kai E., ApJ, 863, 124
  2. Observationally quantified reconnection providing a viable mechanism for active region coronal heating [13]
    Yang, Kai E., Longcope, Dana W., Ding, M. D. & Guo, Yang, Nature Communications, 9, 692

2017

  1. A reexamination of a filament oscillation event on 2013 March 15 [7]
    Chen, Jialin, Xie, Wenbin, Zhou, Yuhao, Yang, Kai, Ouyang, Yu & Chen, P. F., Astrophysics and Space Science, 362, 165
  2. A circular white-light flare with impulsive and gradual white-light kernels [38]
    Hao, Q., Yang, K., Cheng, X., Guo, Y., Fang, C., Ding, M. D., Chen, P. F. & Li, Z., Nature Communications, 8, 2202
  3. Homologous Circular-ribbon Flares Driven by Twisted Flux Emergence [43]
    Xu, Z., Yang, K., Guo, Y., Zhao, J., Zhao, Z. J. & Kashapova, L., ApJ, 851, 30
  4. Interaction of Two Filaments in a Long Filament Channel Associated with Twin Coronal Mass Ejections [24]
    Zheng, Ruisheng, Zhang, Qingmin, Chen, Yao, Wang, Bing, Du, Guohui, Li, Chuanyang & Yang, Kai, ApJ, 836, 160
  5. Magnetic Separatrix as the Source Region of the Plasma Supply for an Active-region Filament [16]
    Zou, P., Fang, C., Chen, P. F., Yang, K. & Cao, Wenda, ApJ, 836, 122

2016

  1. Bidirectional Outflows as Evidence of Magnetic Reconnection Leading to a Solar Microflare [17]
    Hong, Jie, Ding, M. D., Li, Ying, Yang, Kai, Cheng, Xin, Chen, Feng, Fang, Cheng & Cao, Wenda, ApJ, 820, L17
  2. Slipping Magnetic Reconnection of Flux-rope Structures as a Precursor to an Eruptive X-class Solar Flare [32]
    Li, Ting, Yang, Kai, Hou, Yijun & Zhang, Jun, ApJ, 830, 152
  3. Observations of an X-shaped Ribbon Flare in the Sun and Its Three-dimensional Magnetic Reconnection [17]
    Li, Y., Qiu, J., Longcope, D. W., Ding, M. D. & Yang, K., ApJ, 823, L13
  4. Observation of Magnetic Reconnection at a 3D Null Point Associated with a Solar Eruption [10]
    Sun, J. Q., Zhang, J., Yang, K., Cheng, X. & Ding, M. D., ApJ, 830, L4
  5. Observing the release of twist by magnetic reconnection in a solar filament eruption [153]
    Xue, Zhike, Yan, Xiaoli, Cheng, Xin, Yang, Liheng, Su, Yingna, Kliem, Bernhard, Zhang, Jun, Liu, Zhong, Bi, Yi, Xiang, Yongyuan, Yang, Kai & Zhao, Li, Nature Communications, 7, 11837
  6. Quantifying the Topology and Evolution of a Magnetic Flux Rope Associated with Multi-flare Activities [28]
    Yang, Kai, Guo, Yang & Ding, M. D., ApJ, 824, 148
  7. Material Supply and Magnetic Configuration of an Active Region Filament [28]
    Zou, P., Fang, C., Chen, P. F., Yang, K., Hao, Q. & Cao, Wenda, ApJ, 831, 123

2015

  1. Is Flux Rope a Necessary Condition for the Progenitor of Coronal Mass Ejections? [36]
    Ouyang, Y., Yang, K. & Chen, P. F., ApJ, 815, 72
  2. On the 2012 October 23 Circular Ribbon Flare: Emission Features and Magnetic Topology [78]
    Yang, Kai, Guo, Yang & Ding, M. D., ApJ, 806, 171


Created on Wed Apr 8 04:30:09 2026.