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Analysis of the joint detection capability of the SMILE satellite and EISCAT-3D radar 被引量:1

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摘要 The Solar wind Magnetosphere Ionosphere Link Explorer(SMILE)satellite is a small magnetosphere–ionosphere link explorer developed cooperatively between China and Europe.It pioneers the use of X-ray imaging technology to perform large-scale imaging of the Earth’s magnetosheath and polar cusp regions.It uses a high-precision ultraviolet imager to image the overall configuration of the aurora and monitor changes in the source of solar wind in real time,using in situ detection instruments to improve human understanding of the relationship between solar activity and changes in the Earth’s magnetic field.The SMILE satellite is scheduled to launch in 2025.The European Incoherent Scatter Sciences Association(EISCAT)-3D radar is a new generation of European incoherent scatter radar constructed by EISCAT and is the most advanced ground-based ionospheric experimental device in the high-latitude polar region.It has multibeam and multidirectional quasi-real-time three-dimensional(3D)imaging capabilities,continuous monitoring and operation capabilities,and multiple-baseline interferometry capabilities.Joint detection by the SMILE satellite and the EISCAT-3D radar is of great significance for revealing the coupling process of the solar wind–magnetosphere–ionosphere.Therefore,we performed an analysis of the joint detection capability of the SMILE satellite and EISCAT-3D,analyzed the period during which the two can perform joint detection,and defined the key scientific problems that can be solved by joint detection.In addition,we developed Web-based software to search for and visualize the joint detection period of the SMILE satellite and EISCAT-3D radar,which lays the foundation for subsequent joint detection experiments and scientific research.
出处 《Earth and Planetary Physics》 EI CSCD 2024年第1期299-306,共8页 地球与行星物理(英文版)
基金 supported by the Stable-Support Scientific Project of the China Research Institute of Radio-wave Propagation(Grant No.A13XXXXWXX) the National Natural Science Foundation of China(Grant Nos.42174210,4207202,and 42188101) the Strategic Pioneer Program on Space Science,Chinese Academy of Sciences(Grant No.XDA15014800)。
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  • 1J.A.Carter,M.Dunlop,C.Forsyth,K.Oksavik,E.Donovon,A.Kavanagh,S.E.Milan,T.Sergienko,R.C.Fear,D.G.Sibeck,M.Connors,T.Yeoman,X.Tan,M.G.G.T.Taylor,K.McWilliams,J.Gjerloev,R.Barnes,D.D.Billet,G.Chisham,A.Dimmock,M.P.Freeman,D.-S.Han,M.D.Hartinger,S.-Y.W.Hsieh,Z.-J.Hu,M.K.James,L.Juusola,K.Kauristie,E.A.Kronberg,M.Lester,J.Manuel,J.Matzka,I.McCrea,Y.Miyoshi,J.Rae,L.Ren,F.Sigernes,E.Spanswick,K.Sterne,A.Steuwer,T.Sun,M.-T.Walach,B.Walsh,C.Wang,J.Weygand,J.Wild,J.Yan,J.Zhang,Q.-H.Zhang.Ground-based and additional science support for SMILE[J].Earth and Planetary Physics,2024,8(1):275-298. 被引量:2
  • 2丁宗华,代连东,董明玉,许正文,吴健.非相干散射雷达进展:从传统体制到EISCAT 3D[J].地球物理学进展,2014,29(5):2376-2381. 被引量:17

二级参考文献21

  • 1Anita A, Ian M. 2012. EISCAT 3D science case[Z]. EISCAT 3D preparatory phase project WP3, Kiruna, Sweden. 被引量:1
  • 2Bauer P, Waldteufel P, Vialle C. 1974. The French quadristatic incoherent scatter facility[J]. Radio Sci., 9(2): 77-83. 被引量:1
  • 3Bowles K L. 1958. Observation of vertical incidence scatter from the ionosphere at 41 Mc/sec[J]. Phys. Rev. Lett., 1: 454-455, doi/10. 1103/ PhysRevLett. 1. 454. 被引量:1
  • 4Craig H. 2013. Report about the EISCAT Scientific Association and EISCAT 3D ESFRI Preparatory Phase Project[R]. Kiruna, Sweden. 被引量:1
  • 5Derek M, Ian M. 2009. Final report of the EISCAT 3D design study[R]. EISCAT Scientific Association, Kiruna, Sweden. 被引量:1
  • 6Emelyanov L Y, Zhivolup T G. 2013. History of the development of IS radars and founding of the Institute of Ionosphere in Ukraine[J]. Hist. Geo Space Sci., 4: 7-17, doi: 10. 5194/hgss-4-7-2013. 被引量:1
  • 7Esa T. 2009. EISCAT 3D: our windows to Geo-space environment[Z]. EISCAT Scientific Association, Kiruna, Sweden. 被引量:1
  • 8Evans J V. 1969. Theory and practice of ionosphere study by Thomson scatter radar[J]. Proceedings of the IEEE, 57(4): 496-530. 被引量:1
  • 9Evans J V. 1970. Millstone Hill Thomson scatter results for 1965[J]. Planetary and Space Science, 18(8): 1225-1253. 被引量:1
  • 10Farley D T. 1991. Early incoherent scatter observations at Jicamarca[J]. J. Atmos. Terr. Phys., 53(8): 665-675. 被引量:1

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