supported by the National Natural Science Foundation of China(Grant Nos.42322408,42188101,41974211,and 42074202);the Key Research Program of Frontier Sciences,Chinese Academy of Sciences(Grant No.QYZDJ-SSW-JSC028);the Strategic Priority Program on Space Science,Chinese Academy of Sciences(Grant Nos.XDA15052500,XDA15350201,and XDA15014800);supported by the Youth Innovation Promotion Association of the Chinese Academy of Sciences(Grant No.Y202045)。
Astronomical imaging technologies are basic tools for the exploration of the universe,providing basic data for the research of astronomy and space physics.The Soft X-ray Imager(SXI)carried by the Solar wind Magnetosph...
funding and support from the United Kingdom Space Agency(UKSA);the European Space Agency(ESA);funded and supported through the ESA PRODEX scheme;funded through PRODEX PEA 4000123238;the Research Council of Norway grant 223252;funded by Spanish MCIN/AEI/10.13039/501100011033 grant PID2019-107061GB-C61;funding and support from the Chinese Academy of Sciences(CAS);funding and support from the National Aeronautics and Space Administration(NASA)。
The Soft X-ray Imager(SXI)is part of the scientific payload of the Solar wind Magnetosphere Ionosphere Link Explorer(SMILE)mission.SMILE is a joint science mission between the European Space Agency(ESA)and the Chinese...
Throughout the SMILE mission the satellite will be bombarded by radiation which gradually damages the focal plane devices and degrades their performance.In order to understand the changes of the CCD370s within the sof...
support from the UK Space Agency under Grant Number ST/T002964/1;partly supported by the International Space Science Institute(ISSI)in Bern,through ISSI International Team Project Number 523(“Imaging the Invisible:Unveiling the Global Structure of Earth’s Dynamic Magnetosphere”)。
The Solar wind Magnetosphere Ionosphere Link Explorer(SMILE)Soft X-ray Imager(SXI)will shine a spotlight on magnetopause dynamics during magnetic reconnection.We simulate an event with a southward interplanetary magne...
supported by the Youth Science and Technology Innovation Foundation of NSSC;the International Partnership Program of Chinese Academy of Sciences(183311KYSB20200003);the National Natural Science Foundation of China(41831073 and 42004138);the Open Research Project of Large Research Infrastructures of CAS–“Study on the interaction between low/mid-latitude atmosphere and ionosphere based on the Chinese Meridian Project”。
Branching structure(BS)is a very important phenomenon in the evolution of equatorial plasma bubbles(EPBs),the mechanism of which is widely studied from observation and from simulation.However,occurrence characteristic...
the National Science Foundation of China(41327802,41774152 and 41674155);in part by Youth Innovation Promotion Association of the Chinese Academy of Sciences(2017258);the Strategic Priority Program on Space Science,Chinese Academy of Sciences,Grant No.XDA15350203。
New observations of auroras based on the wide-field aurora imager(WAI)onboard Fengyun-3D(FY-3D)satellite are exhibited in this paper.Validity of the WAI data is analyzed by comparing auroral boundaries derived from WA...