First-authored, refereed papers of W. Su, ordered by citations
A list of first-authored, refereed publications of W. Su, derived from the SAO/NASA Astrophysics Data System (ADS) and ordered by the numbers of citations. Publications above the horizontal line count towards the h-index.
Orcid ID: 0000-0002-6613-957X
Number of papers: 7
No. of citations: 131
| 45
| A Type II Radio Burst without a Coronal Mass Ejection
Su, W., Cheng, X., Ding, M. D., Chen, P. F. & Sun, J. Q., 2015, ApJ, 804, 88
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| 31
| Period Increase and Amplitude Distribution of Kink Oscillation of Coronal Loop
Su, W., Guo, Y., Erdélyi, R., Ning, Z. J., Ding, M. D., Cheng, X. & Tan, B. L., 2018, Scientific Reports, 8, 4471
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| 18
| Investigating the Conditions of the Formation of a Type II Radio Burst on 2014 January 8
Su, W., Cheng, X., Ding, M. D., Chen, P. F., Ning, Z. J. & Ji, H. S., 2016, ApJ, 830, 70
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| 17
| Analyses of residual accelerations for TianQin based on the global MHD simulation
Su, Wei, Wang, Yan, Zhou, Ze-Bing, Bai, Yan-Zheng, Guo, Yang, Zhou, Chen, Lee, Tom, Wang, Ming, Zhou, Ming-Yue, Shi, Tong, Yin, Hang & Zhang, Bu-Tian, 2020, Classical and Quantum Gravity, 37, 185017
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| 11
| Analyses of Laser Propagation Noises for TianQin Gravitational Wave Observatory Based on the Global Magnetosphere MHD Simulations
Su, Wei, Wang, Yan, Zhou, Chen, Lu, Lingfeng, Zhou, Ze-Bing, Li, T. M., Shi, Tong, Hu, Xin-Chun, Zhou, Ming-Yue, Wang, Ming, Yeh, Hsien-Chi, Wang, Han & Chen, P. F., 2021, ApJ, 914, 139
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| 7
| Quantifying the Magnetic Structure of a Coronal Shock Producing a Type II Radio Burst
Su, W., Li, T. M., Cheng, X., Feng, L., Zhang, P. J., Chen, P. F., Ding, M. D., Chen, L. J., Guo, Y., Wang, Y., Li, D. & Zhang, L. Y., 2022, ApJ, 929, 175
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| 2
| Evaluating residual acceleration noise for the TianQin gravitational waves observatory with an empirical magnetic field model
Su, Wei, Zhou, Ze-Bing, Wang, Yan, Zhou, Chen, Chen, P. F., Hong, Wei, Peng, J. H., Yang, Yun & Ni, Y. W., 2023, Physical Review D, 108, 103030
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Created on Wed Jan 22 04:30:40 2025.
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