supported by the National Basic Research Program of China (973 Program) (Grant No. 2015CB452804);the National Natural Science Foundation of China (Grant Nos. 41575064, 41875079, 91637102, 41475036, 91437215 and 41575047);the Basic Research Fund of CAMS (Grant No. 2017Y010)
Convective burst(CB) characteristics at distinct stages of a rapidly intensified Typhoon Mujigae(2015), are investigated based on a 72-h simulation. The spatial features show that almost all CB elements develop in the...
supported by the National Basic Research Program of China(973 Program,Grant No.2014CB845800);China Postdoctoral Science Foundation(Grant No.2017M612233);the National Natural Science Foundation of China(Grant Nos.11422325 and 11373022);the Excellent Youth Foundation of Jiangsu Province(BK 20140016)
X-ray flares are the most common phenomena in the afterglow phase of gamma-ray bursts (GRBs) in the Swift era, and are known as a canonical component in X-ray afterglows. In this work, we constrain the Lorentz facto...
Supported by National Basic Research Program of Ministry of Science and Technology of China(2011CB811401);the National Major Scientific Equipment Research and Development Project(ZDYZ2009-3);National Natural Science Foundation of China(11211120147,11221063,11273030,11103044,11103039,11373039)
Two groups of microwave type U and Reverse-Slope(RS)bursts after the Soft X-Ray(SXR)maximum were observed with the 2.6~3.8GHz spectrometer of Chinese Solar Broadband Radio Spectrometers(SBRS/Huairou)on 15 February 201...
supported by the National Natural Science Foundation of China(Grant Nos.50925104,11132006,51231005 and 51321003);the National Basic Research Program of China("973"Program)(Grant Nos.2010CB631003 and 2012CB619402);the support from the"111"Project of China(Grant No.B06025);JL also acknowledges the support by US National Science Foundation(Grant Nos.DMR-1240933 and DMR-1120901)
Mechanical tests on small-volume materials show that in addition to the usual attributes of strength and ductility, the controlla- bility of deformation would be crucial for the purpose of precise plastic shaping. In ...
supported by the National Natural Science Foundation of China(Grant Nos.40931054,41174141 and 40904042);the National Basic Research Program of China("973"Project)(Grant No.2011CB811404);Specialized Research Fund for State Key Laboratories of China(Grant No.KP201104)
In an attempt to study the flow bursts in the Earth's plasma sheet we select an event that took place on August 7, 2004 in the expansion phase of a substorm, using data from the geomagnetic index, solar wind data, pl...
supported by the National Basic Research Program of China("973" Project)(Grant Nos.2012CB957801,2011CB811405);the National Natural Science Foundation of China(Grant Nos.41274155,40904036);the Public Science and Technology Research Funds Projects of Ocean,State Oceanic Administration of China(Grant No.201005017);the Specialized Research Fund for State Key Laboratories
Particle bursts (PBs), the phenomena characterized by short-term increases of particle counting rates (CRs), were observed by space-borne radiation belt particle detectors. With the electron CR data obtained by Na...
the National Basic Research Program of China (Grant No. 2009CB824800);the National Natural Science Foundation of China (Grant Nos. 11025313 and 11203008);the Special Foundation for Distinguished Expert Program of Guangxi;the Guangxi Natural Science Foundation (Grant No. 2013GXNSFFA019001) and Contract No.2011-135
A systematical analysis of the spectral lags in different episodes within a gamma-ray burst (GRB) for the BATSE GRB sample is given. The identified episodes are usually a single pulse with mixing of small fluctuations...
supported by the National Natural Science Foundation of China(Grant Nos. 11033002 and J1210039);the National Basic Research Program of China (973 Program, Grant No. 2009CB824800)
The afterglow of GRB 081029 showed unusual behavior, with a signifi- cant rebrightening being observed at the optical wavelength at about 3000 s after the burst. One possible explanation is that the rebrightening resu...
supported by the National Basic Research Program of China (973 program, Grant Nos. 2012CB821800 and 2009CB824800);the National Natural Science Foundation of China(Grant Nos. 11225314, 11103026 and 10935001)
We analyze the emission plateaus in the X-ray afterglow light curves of gamma-ray bursts (GRBs) and those in the optical light curves of type Ⅱ plateau su- pernovae (SNe Ⅱ-P) in order to study whether they have ...
Supported by the National Natural Science Foundation of China;supported by the National Basic Research Programof China (973 Program,2009CB824800);the China Postdoctoral Science Foundation funded project(No. 20110490590);the National Natural Science Foundation of China (Grant No. 111030262);the Foundation for the Authors of National Excellent Doctoral Dissertations of China
Observations imply that long "y-ray bursts (GRBs) originate from the explo- sions of massive stars, therefore they may occur in the molecular clouds where their progenitors were born. We show that the prompt optica...