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Chinese Academy of Sciences Institutional Repositories Grid
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浏览/检索结果: 共50条,第1-10条 帮助

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A Novel Method for Recognizing Space Radiation Sources Based on Multi-Scale Residual Prototype Learning Network 期刊论文  OAI收割
SENSORS, 2023, 卷号: 23, 期号: 10, 页码: 25
作者:  
Liu, Pengfei;  Guo, Lishu;  Zhao, Hang;  Shang, Peng;  Chu, Ziyue
  |  收藏  |  浏览/下载:16/0  |  提交时间:2023/12/13
A framework of correcting the angular effect of land surface temperature on evapotranspiration estimation in single-source energy balance models 期刊论文  OAI收割
REMOTE SENSING OF ENVIRONMENT, 2022, 卷号: 283, 页码: 18
作者:  
Jiang, Yazhen;  Tang, Ronglin;  Li, Zhao-Liang
  |  收藏  |  浏览/下载:32/0  |  提交时间:2022/12/09
A framework of correcting the angular effect of land surface temperature on evapotranspiration estimation in single-source energy balance models 期刊论文  OAI收割
REMOTE SENSING OF ENVIRONMENT, 2022, 卷号: 283, 页码: 18
作者:  
Jiang, Yazhen;  Tang, Ronglin;  Li, Zhao-Liang
  |  收藏  |  浏览/下载:24/0  |  提交时间:2022/12/09
Thermal features and heat transfer enhancement of a Casson fluid across a porous stretching/shrinking sheet: Analysis of dual solutions 期刊论文  OAI收割
CASE STUDIES IN THERMAL ENGINEERING, 2021, 卷号: 28, 页码: 12
作者:  
Khan, M. Riaz;  Elkotb, Mohamed Abdelghany;  Matoog, R. T.;  Alshehri, Nawal A.;  Abdelmohimen, Mostafa A. H.
  |  收藏  |  浏览/下载:31/0  |  提交时间:2022/04/02
Applied Superconductivity and Electromagnetic Devices-Large-Scale Applications and Availability 期刊论文  OAI收割
IEEE TRANSACTIONS ON APPLIED SUPERCONDUCTIVITY, 2021, 卷号: 31, 期号: 8, 页码: 17
作者:  
Zhou, Qian;  Wu, Wei;  Mei, Enming;  Sun, Liangting;  Zhang, Guoshu
  |  收藏  |  浏览/下载:77/0  |  提交时间:2021/12/13
Unsteady Convective MHD Flow and Heat Transfer of a Viscous Nanofluid across a Porous Stretching/Shrinking Surface: Existence of Multiple Solutions 期刊论文  OAI收割
CRYSTALS, 2021, 卷号: 11, 期号: 11, 页码: 11
作者:  
Alshehri, Nawal A.;  Abidi, Awatef;  Khan, Muhammad Riaz;  Reddy, Yanala Dharmendar;  Rasheed, Saim
  |  收藏  |  浏览/下载:25/0  |  提交时间:2022/04/02
Unsteady radiative slip flow of MHD Casson fluid over a permeable stretched surface subject to a non-uniform heat source 期刊论文  OAI收割
CASE STUDIES IN THERMAL ENGINEERING, 2021, 卷号: 26, 页码: 10
作者:  
Zhou, Jian-Cun;  Abidi, Awatef;  Shi, Qiu-Hong;  Khan, M. Riaz;  Rehman, Aysha
  |  收藏  |  浏览/下载:28/0  |  提交时间:2022/04/02
3D modeling of multi-radiation source semi-airborne transient electromagnetic response 期刊论文  OAI收割
CHINESE JOURNAL OF GEOPHYSICS-CHINESE EDITION, 2021, 卷号: 64, 期号: 2, 页码: 716-723
作者:  
Li Xiu;  Hu WeiMing;  Xue GuoQiang
  |  收藏  |  浏览/下载:35/0  |  提交时间:2021/10/09
Combined carrier phase and code phase passive radiation source localisation method 期刊论文  OAI收割
IET RADAR SONAR AND NAVIGATION, 2020, 卷号: 14, 期号: 1, 页码: 147-155
作者:  
  |  收藏  |  浏览/下载:20/0  |  提交时间:2020/11/09
No pulsed radio emission during a bursting phase of a Galactic magnetar 期刊论文  OAI收割
Nature, 2020, 卷号: 587, 页码: 63-65
作者:  
HXMT
  |  收藏  |  浏览/下载:44/0  |  提交时间:2022/02/08
Astrophysics - High Energy Astrophysical Phenomena  Abstract: Fast radio bursts (FRBs) are millisecond-duration radio transients of unknown physical origin observed at extragalactic distances1-3. It has long been speculated that magnetars are the engine powering repeating bursts from FRB sources4-13, but no convincing evidence has been collected so far14. Recently, the Galactic magnetar SRG 1935+2154 entered an active phase by emitting intense soft íray bursts15. One FRB-like event with two peaks (FRB 200428) and a luminosity slightly lower than the faintest extragalactic FRBs was detected from the source, in association with a soft íray/hard-X-ray flare18-21. Here we report an eight-hour targeted radio observational campaign comprising four sessions and assisted by multi-wavelength (optical and hard-X-ray) data. During the third session, 29 soft-íray repeater (SGR) bursts were detected in íray energies. Throughout the observing period, we detected no single dispersed pulsed emission coincident with the arrivals of SGR bursts, but unfortunately we were not observing when the FRB was detected. The non-detection places a fluence upper limit that is eight orders of magnitude lower than the fluence of FRB 200428. Our results suggest that FRB-SGR burst associations are rare. FRBs may be highly relativistic and geometrically beamed, or FRB-like events associated with SGR bursts may have narrow spectra and characteristic frequencies outside the observed band. It is also possible that the physical conditions required to achieve coherent radiation in SGR bursts are difficult to satisfy, and that only under extreme conditions could an FRB be associated with an SGR burst.