Data Sources

Part of the Springer Theses book series (Springer Theses)


Since 1980s, several important science programs were proposed to address the fundamental physical processes of the sun, its interaction with Earth and the solar system, which include International Solar-Terrestrial Physics (ISTP) Program, Living With a Star (LWS) Program, and Solar Terrestrial Probes (STP) Program. ISTP is an international cooperation program led by NASA, ESA as well as ISAS, and its primary missions include ACE, Wind, SOHO, Geotail, Cluster, GOES, LANL, etc. LWS and STP are two strategic programs of NASA in the new century. The primary missions in the LWS Program are SDO, Van Allen Probes, BARREL, Solar Probe Plus, Solar Orbiter, etc. And the primary missions in the STP Program are TIMED, MMS, Solar-B, STEREO, etc.


  1. 1.
    Escoubet CP, Fehringer M, Goldstein M (2001) Introduction the cluster mission. Ann Geophys 19(10/12):1197–1200ADSCrossRefGoogle Scholar
  2. 2.
    Rème H et al (2001) First multispacecraft ion measurements in and near the Earth’s magnetosphere with the identical Cluster ion spectrometry (CIS) experiment. Ann Geophys 19:1303–1354ADSCrossRefGoogle Scholar
  3. 3.
    Balogh A et al (1997) The cluster magnetic field investigation. Space Sci Rev 79:65–91ADSCrossRefGoogle Scholar
  4. 4.
    Gustafsson G et al (2001) First results of electric field and density observations by Cluster EFW based on initial months of operation. Ann Geophys 19(10/12):1219–1240ADSCrossRefGoogle Scholar
  5. 5.
    Ren J, Zong Q, Zhou X, Zhang H, Fu S, Wang Y, Liu YC-M (2016b) Statistics of the field-aligned currents at the high-latitude energetic electron boundaries in the nightside: Cluster observation. J Geophys Res 121(3):1979–1989. Scholar
  6. 6.
    Mauk B, Fox NJ, Kanekal S, Kessel R, Sibeck D, Ukhorskiy A (2013) Science objectives and rationale for the Radiation Belt Storm Probes Mission. Space Sci Rev 179(1–4):3–27. Scholar
  7. 7.
    Funsten H et al (2013) Helium, Oxygen, Proton, and Electron (HOPE) mass spectrometer for the radiation belt storm probes mission. Space Sci Rev 179(1–4):423–484.,214-013-9968-7ADSCrossRefGoogle Scholar
  8. 8.
    Kletzing C et al (2013) The electric and magnetic field instrument suite and integrated science (EMFISIS) on RBSP. Space Sci Rev 179:127–181.,214-013-9993-6ADSCrossRefGoogle Scholar
  9. 9.
    Wygant J et al (2000) Polar spacecraft based comparisons of intense electric fields and Poynting flux near and within the plasma sheet-tail lobe boundary to UVI images: an energy source for the aurora. J Geophys Res 105(A8):18675–18692. Scholar

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© Springer Nature Singapore Pte Ltd. 2019

Authors and Affiliations

  1. 1.School of Earth and Space SciencesPeking UniversityBeijingChina

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