Z.Y.acknowledges the National Natural Science Foundation of China(Grant No.42074211).
Magnetic reconnection and dipolarization are crucial processes driving magnetospheric dynamics,including particle energization,mass circulation,and auroral processes,among others.Recent studies have revealed that thes...
Sun acknowledges the support from the National Natural Science Foundation of China through grants(No.s 42322408,42188101,and 42074202).
The SMILE(Solar wind Magnetosphere Ionosphere Link Explorer)project(http://www.nssc.cas.cn/smile/,https://www.cosmos.esa.int/web/smile/mission)is a joint spacecraft mission of the European Space Agency(ESA)and the Chi...
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...
the European Research Council for starting grant 200141-QuESpace,with which the Vlasiator model was developed;consolidator grant 682068-PRESTISSIMO awarded for further development of Vlasiator and its use in scientific investigations;Academy of Finland grant numbers 338629-AERGELC’H,339756-KIMCHI,336805-FORESAIL,and 335554-ICT-SUNVAC;The Academy of Finland also supported this work through the PROFI4 grant(grant number 3189131);support from the NASA grants,80NSSC20K1670 and 80MSFC20C0019;the NASA GSFC FY23 IRAD;HIF funds。
Solar wind charge exchange produces emissions in the soft X-ray energy range which can enable the study of near-Earth space regions such as the magnetopause,the magnetosheath and the polar cusps by remote sensing tech...
Solar Wind Charge eXchange X-ray(SWCX) emission in the heliosphere and Ea rth’s exosphere is a hard to avoid signal in soft Xray obse rvations of astrophysical targets.On the other hand,the X-ray imaging possibilitie...
supported by NNSFC grants 42322408,42188101 and 42074202;the Strategic Pioneer Program on Space Science,CAS Grant nos.XDA15350201;in part by the Research Fund from the Chinese Academy of Sciences;the Specialized Research Fund for State Key Laboratories of China.;supported by the Young Elite Scientists Sponsorship Program(CAST-Y202045);supported by Royal Society grant DHFR1211068。
Solar wind charge exchange(SWCX)is the process of solar wind high-valence ions exchanging charges with neutral components and generating soft X-rays.Recently,detecting the SWCX emission from the magnetosphere is propo...
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...
support from the United Kingdom Space Agency(UKSA);the Science and Technology Facilities Council(STFC)under Grant No.ST/T002085/1。
The Soft X-ray Imager(SXI)on board the Solar wind Magnetosphere Ionosphere Link Explorer(SMILE)spacecraft will be able to view the Earth’s magnetosheath in soft X-rays.Simulated images of the X-ray emission visible f...
To determine the cause(s)of perturbations seen in dayside equatorial ground magnetograms,we conducted a systematic survey of simultaneous ground-based and geosynchronous satellite-based observations during the 90-day ...
supported by Royal Society grant DHFR1211068;funded by UKSA;STFC;STFC grant ST/M001083/1;funded by STFC grant ST/W00089X/1;supported by NERC grant NE/W003309/1(E3d);funded by NERC grant NE/V000748/1;support from NERC grants NE/V015133/1,NE/R016038/1(BAS magnetometers),and grants NE/R01700X/1 and NE/R015848/1(EISCAT);supported by NERC grant NE/T000937/1;NSFC grants 42174208 and 41821003;supported by the Research Council of Norway grant 223252;PRODEX arrangement 4000123238 from the European Space Agency;support of the AUTUMN East-West magnetometer network by the Canadian Space Agency;supported by NASA’s Heliophysics U.S.Participating Investigator Program;support from grant NSF AGS 2027210;supported by grant Dnr:2020-00106 from the Swedish National Space Agency;supported by the German Research Foundation(DFG)under number KR 4375/2-1 within SPP"Dynamic Earth"。
The joint European Space Agency and Chinese Academy of Sciences Solar wind Magnetosphere Ionosphere Link Explorer(SMILE)mission will explore global dynamics of the magnetosphere under varying solar wind and interplane...