相关期刊:《Journal of High Energy Physics, Gravitation and Cosmology》《Science China Earth Sciences》《Communications in Nonlinear Science and Numerical Simulation》《Science China Mathematics》更多>>
In this study, we examined variability of sun-related energies, auroral electrojet current, ring current, and magnetopause current during solar cycles 23 and 24. The study revealed a dependence of sun-related energies...
supported by the National Natural Science Foundation of China(Grant Nos.42030203,42004132,42074195,and 42074183).
The magnetopause is the boundary between the Earth’s magnetic field and the interplanetary magnetic field(IMF),located where the supersonic solar wind and magnetospheric pressure are in balance.Although empirical mod...
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 National Natural Science Foundation of China(NNSFC)grants 42074202,42274196;Strategic Priority Research Program of Chinese Academy of Sciences grant XDB41000000;ISSI-BJ International Team Interaction between magnetic reconnection and turbulence:From the Sun to the Earth。
Earth’s magnetopause is a thin boundary separating the shocked solar wind plasma from the magnetospheric plasmas,and it is also the boundary of the solar wind energy transport to the magnetosphere.Soft X-ray imaging ...
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...
supported by NASA(Grant Nos.80NSSC19K0844,80NSSC20K1670,80MSFC20C0019,and 80GSFC21M0002);support from NASA Goddard Space Flight Center internal funding programs(HIF,Internal Scientist Funding Model,and Internal Research and Development)。
The Lunar Environment heliospheric X-ray Imager(LEXI)and Solar wind Magnetosphere Ionosphere Link Explorer(SMILE)missions will image the Earth’s dayside magneto pause and cusps in soft X-rays after their respective l...
supported by NASA Goddard Space Flight Center through Cooperative Agreement 80NSSC21M0180 to Catholic University;Partnership for Heliophysics and Space Environment Research(PHaSER);the NASA Heliophysics United States Participating Investigator Program under Grant WBS516741.01.24.01.03(DS);support from the NASA grants 80NSSC19K0844,80NSSC20K1670,and 80MSFC20C0019;the NASA GSFC internal fundings(HIF,ISFM,and IRAD)。
Variability in the location and shape of the dayside magnetopause is attributed to magnetic reconnection,a fundamental process that enables the transfer of mass,energy,and momentum from the solar wind into the magneto...
support from the European Space Agency(ESA)PRODEX(PROgramme de Développement d’Expériences scientifiques)Project mission(No.PEA4000134960);Partial funding was provided by the Romanian Ministry of Research,Innovation and Digitalization under Romanian National Core Program LAPLAS VII(Contract No.30N/2023);the Belgian Solar-Terrestrial Centre of Excellence;supported by the project Belgian Research Action through Interdisciplinary Networks(BRAIN-BE)2.0(Grant No.B2/223/P1/PLATINUM)funded by the Belgian Office for Research(BELSPO);partially supported by a grant from the Romanian Ministry of Education and Research(CNCS-UEFISCDI,Project No.PN-III-P1-1.1TE-2021-0102)。
We derived the properties of the terrestrial magnetopause(MP)from two modeling approaches,one global–fluid,the other local–kinetic,and compared the results with data collected in situ by the Magnetospheric Multiscal...
supported by the National Natural Science Foundation of China(Grant Nos.41731070,41974211,42074202,41774173);the Key Research Program of Frontier Sciences CAS(Grant No.QYZDJ-SSW-JSC028);the Strategic Pioneer Program on Space Science,CAS(Grant Nos.XDA15052500,XDA15350201);supported by the Youth Innovation Promotion Association of CAS(Grant No.Y202045)。
Imaging techniques provide essential information in astronomical and space physics studies.The Soft X-ray Imager(SXI)will obtain images of the Earth’s magnetosphere via the solar wind charge exchange process in a glo...