Skip to main content
Log in

Shrinkage of magnetosphere observed by TC-1 satellite during the high-speed solar wind stream

  • Published:
Science in China Series E: Technological Sciences Aims and scope Submit manuscript

Abstract

During the interval 06:14–07:30 UT on August 24, 2005, since the Earth’s magnetopause was suddenly compressed by the persistent high-speed solar wind stream with the southward component of the interplanetary magnetic field (IMF), the magnetopause moved inward for about 3.1 RE. Meanwhile, TC-1 satellite shifted from northern plasma sheet to the northern lobe/mantle region, although it kept inward flying during the interval 06:00–07:30UT. The shift of TC-1 from the plasma sheet to the lobe/mantle is caused by the simultaneous inward displacements of the plasma sheet and near-Earth lobe/mantle region, and their inward movement velocity is larger than the inward motion velocity of TC-1. The joint inward displacements of the magnetopause, the lobe/mantle region and the plasma sheet indicate that the whole magnetosphere shrinks inward due to the magnetospheric compression by the high-speed solar wind stream, and the magnetospheric ions are attached to the magnetic field lines (i.e. ‘frozen’ in magnetic field) and move inward in the shrinking process of magnetosphere. The large shrinkage of magnetosphere indicates that the near-Earth magnetotail compression caused by the strong solar wind dynamic pressure is much larger than its thickening caused by the southward component of the IMF, and the locations of magnetospheric regions with different plasmas vary remarkably with the variation of the solar wind dynamic pressure.

This is a preview of subscription content, log in via an institution to check access.

Access this article

Price excludes VAT (USA)
Tax calculation will be finalised during checkout.

Instant access to the full article PDF.

Similar content being viewed by others

References

  1. Gosling J T, McComas D J, Phillips J L, et al. Geomagnetic activity associated with Earth passage of interplanetary shock disturbances and coronal mass ejections. J Geophys Res, 1991, 96(A5): 7831–7839

    Article  Google Scholar 

  2. Tsurutani B T, Gonzalez W D, Gonzalez A L C, et al. Interplanetary origin of geomagnetic activity in the declining phase of the solar cycle. J Geophys Res, 1995, 100(A11): 21717–21733

    Article  Google Scholar 

  3. Kamide Y, Baumjohann W, Daglis I A, et al. Current understanding of geomagnetic storms: Storm-substorm relationship. J Geophys Res, 1998, 103(A3): 17705–17728

    Article  Google Scholar 

  4. Gonzalez W D, Tsurutani B T, Cluade A L, Interplanetary origin of geomagnetic storms. Space Sci Rev, 1999, 88: 529–562

    Article  Google Scholar 

  5. Richardson I, Cliver E, Cane H. Sources of geomagnetic storms for solar minimum and maximum conditions during 1972–2000. Geophys Res Lett, 2001, 28: 2567–2572

    Article  Google Scholar 

  6. Lyatsky W, Tan A. Solar wind disturbances responsible for geomagnetic storms. J Geophys Res, 2003, 108(A3): 1134, doi:10.1029/2001JA005057

    Article  Google Scholar 

  7. Li L Y, Cao J B, Zhou G C. Relation between the variation of geomagnetospheric relativistic electron flux and storm/substorm. Chin J Geophys, 2006, 49(1): 9–15

    Google Scholar 

  8. Wilken B, Zong Q G, Doke T, et al. Substorm activity on January 11, 1994: Geotail observations in the distant tail during the leading phase of a corotating interaction region. J Geophys Res, 1998, 103(A8): 17671–17689

    Article  Google Scholar 

  9. Zong Q G, Wilken B. Layered structure of energetic oxygen ions in the dayside magnetosheath. Geophys Res Lett, 1998, 25(22): 4121–4124

    Article  Google Scholar 

  10. Wilken B, Goertz C K, Baker D N, et al. The SSC on July 29, 1977 and its propagation within the magnetosphere. J Geophys Res, 1982, 87: 5901–5910

    Article  Google Scholar 

  11. Russell C T, Zhou X W, Chi P J, et al. Sudden compression of the outer magnetosphere associated with an ionospheric mass ejection. Geophys Res Lett, 1999, 26: 2343–2346

    Article  Google Scholar 

  12. Russell C T, Le G, Chi P J, et al. The extreme compression of the magnetosphere on May 4, 19978, as observed by the Polar spacecraft. Advances in Space Res, 2000, 25: 1369–1375

    Article  Google Scholar 

  13. Andréeová K, Přech L. Propagation of interplanetary shocks into the Earth’s magnetosphere. Advances in Space Res, 2007, 40: 1871–1880

    Article  Google Scholar 

  14. Carr C, Brown P, Zhang T L, et al. The Double Star magnetic field investigation: instrument design, performance and highlights of the first year’s observations. Ann Geophys, 2005, 23: 2713–2732

    Google Scholar 

  15. Rème H, Dandouras I, Aoustin C, et al. The HIA instrument on board the Tan Ce 1 Double Star near-equatorial spacecraft and its first results. Ann Geophys, 2005, 23: 2757–2774

    Article  Google Scholar 

  16. Kokubun S, Yamamoto T, Acuna M, et al. The Geotail magnetic field experiment. J Geomagn Geoelectr, 1994, 46: 7–21

    Google Scholar 

  17. Frank L A, Ackerson K L, Paterson W R, et al. The comprehensive plasma instrumentation (CPI) for the Geotail spacecraft. J Geomag Geoelectr, 1994, 46: 23–37

    Google Scholar 

  18. Shue J H, Song P, Russell C T, et al. Magnetopause location under extreme solar wind conditions. J Geophys Res, 1998, 103(A8): 17691–17700

    Article  Google Scholar 

  19. Rosenbauer H, Gruwldt H, Montgomery M D, et al. Heos 2 plasma observations in the distant polar magnetosphere: the plasma mantle. J Geophys Res, 1975, 80(19): 2723–2737

    Article  Google Scholar 

  20. Gosling J T, Baker D N, Bame S J, et al. Plasma entry into the distant tail lobes: ISEE 3. Geophys Res Lett, 1984, 11(10): 1078–1081

    Article  Google Scholar 

  21. Taguchi S, Kishida H, Mukai T, et al. Low-latitude plasma mantle in the near-Earth magnetosphere: Geotail observations. J Geophys Res, 2001, 106(A2): 1949–1954

    Article  Google Scholar 

  22. Maezawa K, Hori T. The distant magnetotail: Its structure, IMF dependence, and Thermal properties. In: Nishida A, et al. eds. New Perspectives on the Earth’s magnetotail. Washington D. C.: American Geophysical Union, 2000. 1–19

    Google Scholar 

  23. Seki K, Hirahara M, Terasawa T, et al. Statistical properties and possible supply mechanisms of tailward cold O+ beams in the lobe/mantle regions. J Geophys Res, 1998, 103: 4477–4490

    Article  Google Scholar 

  24. Taguchi S, Kiyohara M, Mukai T, et al. Convection enhancements in the low-latitude lobe for substorm onset. J Geophys Res, 2001, 106(A3): 3943–3952

    Article  Google Scholar 

  25. Hardy D A, Freeman J W, Hills H K. Double-peaked ion spectra in the lobe plasma: Evidence for massive ions? J Geophys Res, 1977, 82(35): 5529–5540

    Article  Google Scholar 

  26. Seki K, Hirahara M, Terasawa T, et al. Properties of He+ beams observed by Geotail in the lobe/mantle regions: Comparison with O+ beams. J Geophys Res, 1999, 104: 6973–6985

    Article  Google Scholar 

  27. Zong Q G, Wilken B, Woch J, et al. Energetic oxygen ion bursts in the distant magnetotail as a product of intense substorms: Three case studies. J Geophys Res, 1998, 103(A9): 20339–20363

    Article  Google Scholar 

Download references

Author information

Authors and Affiliations

Authors

Corresponding author

Correspondence to LiuYuan Li.

Additional information

Supported by the National Natural Science Foundation of China (Grant Nos. 40604018, 40523006), CSSAR (Grant No. O72114AA4S), Scientific Research Start-up Foundation for President Prize of CAS, 973 Program of China (Grant No. 2006CB806305) and the Specialized Research Fund for State Key Laboratories

Rights and permissions

Reprints and permissions

About this article

Cite this article

Li, L., Cao, J., Zhou, G. et al. Shrinkage of magnetosphere observed by TC-1 satellite during the high-speed solar wind stream. Sci. China Ser. E-Technol. Sci. 51, 1695–1703 (2008). https://doi.org/10.1007/s11431-008-0258-7

Download citation

  • Received:

  • Accepted:

  • Published:

  • Issue Date:

  • DOI: https://doi.org/10.1007/s11431-008-0258-7

Keywords

Navigation