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Oxygen vacancies and local amorphization introduced by high fluence neutron irradiation in β-Ga2O3 power diodes 期刊论文
APPLIED PHYSICS LETTERS, 2023, 卷号: 123
作者:  Liu, Jinyang;  Han, Zhao;  Ren, Lei;  Yang, Xiao;  Xu, Guangwei
收藏  |  浏览/下载：9/0  |  提交时间：2023/11/10
Estimating energy release performance of oxidizer-activated aluminum fuel particles under ultrafast stimulus 期刊论文
DEFENCE TECHNOLOGY, 2023, 卷号: 23, 页码: 92-99
作者:  Li, Yaru;  Ren, Hui;  Wu, Xinzhou;  Wang, Huixin;  Yu XL(余西龙)
收藏  |  浏览/下载：10/0  |  提交时间：2023/06/15
Determination method of high fluence rate for D-T neutron source with long counter 期刊论文
RADIATION MEASUREMENTS, 2021, 卷号: 148
作者:  Li, Yanan;  Li, Taosheng;  Wang, Ying;  Hong, Bing;  Wang, Feipeng
收藏  |  浏览/下载：16/0  |  提交时间：2021/11/15
Detection of two bright radio bursts from magnetar SGR 1935 + 2154 期刊论文
Nature Astronomy, 2021, 卷号: 5, 页码: 414
作者:  Kirsten, F.;  Snelders, M. P.;  Jenkins, M.;  Nimmo, K.;  van den Eijnden, J.
收藏  |  浏览/下载：41/0  |  提交时间：2021/11/18
Astrophysics - High Energy Astrophysical Phenomena  Abstract: Fast radio bursts are millisecond-duration, bright radio signals (fluence 0.1-100 Jy ms) emitted from extragalactic sources of unknown physical origin. The recent CHIME/FRB and STARE2 detection of an extremely bright (fluence ~MJy ms) radio burst from the Galactic magnetar SGR 1935+2154 supports the hypothesis that (at least some) fast radio bursts are emitted by magnetars at cosmological distances. In follow-up observations totalling 522.7 h on source, we detect two bright radio bursts with fluences of 112 ± 22 Jy ms and 24 ± 5 Jy ms, respectively. Both bursts appear to be affected by interstellar scattering and we measure significant linear and circular polarization for the fainter burst. The bursts are separated in time by ~1.4 s, suggesting a non-Poissonian, clustered emission processsimilar to those seen in some repeating fast radio bursts. Together with the burst reported by CHIME/FRB and STARE2, as well as a much fainter burst seen by FAST (fluence 60 mJy ms), our observations demonstrate that SGR 1935+2154 can produce bursts with apparent energies spanning roughly seven orders of magnitude, and that the burst rate is comparable across this range. This raises the question of whether these four bursts arise from similar physical processes, and whether the fast radio burst population distribution extends to very low energies (~1030 erg, isotropic equivalent).  
Konus-Wind observation of GRB 200412B GCN
2020
作者:  Ridnaia, A;  Golenetskii, S;  Aptekar, R;  Frederiks, D;  Ulanov, M
收藏  |  浏览/下载：46/0  |  提交时间：2020/05/20
Konus-Wind observation of GRB 200125B GCN
2020
作者:  Svinkin, D;  Golenetskii, S;  Aptekar, R;  Frederiks, D;  Ulanov, M
收藏  |  浏览/下载：15/0  |  提交时间：2020/05/20
Konus-Wind observation of GRB 190531B GCN
2019
作者:  Svinkin, D;  Golenetskii, S;  Aptekar, R;  Frederiks, D;  Ulanov, M
收藏  |  浏览/下载：13/0  |  提交时间：2020/05/20
Heavy-ion and pulsed-laser single event effects in 130-nm CMOS-based thin/thick gate oxide anti-fuse PROMs 期刊论文
NUCLEAR SCIENCE AND TECHNIQUES, 2019, 卷号: 30, 期号: 5, 页码: 11
作者:  Zhao, Pei-Xiong;  Geng, Chao;  Zhang, Zhan-Gang;  Liu, Jie;  Li, Xiao-Yuan
收藏  |  浏览/下载：59/0  |  提交时间：2019/11/10
GREENBURST: A commensal Fast Radio Burst search back-end for the Green Bank Telescope 期刊论文
PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF AUSTRALIA, 2019, 卷号: 36, 页码: e032
作者:  Surnis, Mayuresh P.;  Agarwal, D.;  Lorimer, D. R.;  Pei, X.;  Foster, G.
收藏  |  浏览/下载：30/0  |  提交时间：2019/10/29

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