supported by the National Natural Science Foundation of China(Grant No.42225405);Shutao YAO was supported by the National Natural Science Foundation of China(Grant No.42104153);the National Natural Science Foundation of Shandong Province(Grant No.ZR2021QD097);the China Postdoctoral Science Foundation(Grant No.2021M701975);supported by the International Space Science Institute(ISSI)in Bern,through ISSI International Team Project(Grant Nos.#517,#555);financial support from the Canadian Space Agency。
Magnetic holes at the ion-to-electron kinetic scale(KSMHs)are one of the extremely small intermittent structures generated in turbulent magnetized plasmas.In recent years,the explorations of KSMHs have made substantia...
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 ...
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...
supported by the NSF grant AGS-1928883;the NASA grants,80NSSC20K1670 and 80MSFC20C0019;support from NASA GSFC IRAD;HIF;ISFM funds。
Lunar Environment heliospheric X-ray Imager(LEXI)and Solar wind−Magnetosphere−Ionosphere Link Explorer(SMILE)will observe magnetosheath and its boundary motion in soft X-rays for understanding magnetopause reconnectio...
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 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)。
Following our earlier work on tomographic reconstruction of the magnetosheath soft X-ray emissions with superposed epoch analysis of many images recorded from a single spacecraft we now explore the instantaneous recon...
financial support from CNES via its Sun-Heliosphere-Magnetosphere(SHM)program;support from NASA grant#80NSSC20K1709。
While we eagerly anticipate SMILE’s(Solar wind Magnetosphere Ionosphere Link Explorer)unprecedented X-ray observations of the Earth’s magnetosheath and the initiation of a new era of magnetospheric research,it seems...
Z.Y.acknowledges the National Natural Science Foundation of China(Grant No.42074211);the Key Research Program of the Institute of Geology&Geophysics,Chinese Academy of Sciences(Grant No.IGGCAS-201904).
A mirror mode wave is a fundamental magnetic structure in the planetary space environment that is persistently compressed by solar wind,especially in the magnetosheath.Mirror modes have been widely identified in the m...
supported by the Shenzhen Science and Technology Research Program (JCYJ20210324121412034);the Guangdong Basic and Applied Basic Research Foundation (2022A1515011698);supported by the NASA (National Aeronautics and Space Administration) Mars Exploration Program
In-flight calibration of the ze ro offset is crucial for ensuring high-precision measure ment of the spaceborne fluxgate magnetomete r.Tianwen-1 is China’s first Mars mission,and its orbiter will re main out of the s...
FAPESP for PhD fellowship support(projects 2016/10794-2 and 2017/00516-8);the CNPq agency(projects PQ-300969/2020-1,PQ-301542/2021-0)for their support;the Brazilian FAPESP(2018/21657-1);CNPq(PQ-301883/2019-0)agencies for financial support;supported by CNPq agency contract number(PQ-305692/2018-6);FAPEG agency contract number 2012.1026.7000905;supported by German Space Agency grant 50QM1703.
Planetary magnetosheaths are characterized by high plasma wave and turbulence activity.The Martian magnetosheath is no exception;both upstream and locally generated plasma waves have been observed in the region betwee...