Skip to main content
Log in

Structures of magnetic null points in reconnection diffusion region: Cluster observations

  • Articles
  • Geophysics
  • Published:
Chinese Science Bulletin

Abstract

Magnetic reconnection is a very important and fundamental plasma process in transferring energy from magnetic field into plasma. Previous theory, numerical simulations and observations mostly concentrate on 2-dimensional (2D) model; however, magnetic reconnection is a 3-dimensional (3D) nonlinear process in nature. The properties of reconnection in 3D and its associated singular structure have not been resolved completely. Here we investigate the structures and characteristics of null points inside the reconnection diffusion region by introducing the discretized Poincaré index through Gauss integral and using magnetic field data with high resolution from the four satellites of Cluster mission. We estimate the velocity and trajectory of null points by calculating its position in different times, and compare and discuss the observations with different reconnection models with null points based on characteristics of electric current around null points.

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. Lau Y T, Finn J M. Three-dimensional kinematic reconnection in the presence of field nulls and closed field lines. Astrophys J, 1990, 350: 672–691

    Article  Google Scholar 

  2. Parnell C E, Smith J M, Neukirch T et al., The structure of three-dimensional magnetic neutral points. Phys Plasmas, 1996, 3(3): 759–770

    Article  CAS  Google Scholar 

  3. Priest E R, Titov V S. Magnetic reconnection at three-dimensional null points. Phil Trans R Soc Lond A, 1996, 354(1721): 2951–2992

    Article  Google Scholar 

  4. Wang H, Wang J X. Two-dimensional magnetic singular points and flares in solar active regions. Astron Astrophys, 1996, 313: 285–296

    Google Scholar 

  5. Zhao H, Wang J, Zhang J, et al. A new method of identifying 3D null points in solar vector magnetic fields. Chin J Astron Astrophys. 2005, 5: 443–447

    Article  Google Scholar 

  6. Cai D S, Li Y T, Ichikawai T, et al., Visualization and criticality of magnetotail field topology in a three-dimensional particle simulation. Earth Planets Space 53, 2001: 1011–1019

    Google Scholar 

  7. Dorelli J C, Bhattacharjee A, Raeder J. Separator reconnection at Earth’s dayside magnetopause under generic northward interplanetary magnetic field conditions. J Geophys Res, 2007, 112, doi: 10.1029/2006JA011877

  8. Greene J. Locating three-dimensional roots by a bisection method. J Comput Phys, 1992, 98: 194–198

    Article  Google Scholar 

  9. Xiao C J, Wang X G, Pu Z Y, et al. In situ evidence for the structure of the magnetic null in a 3D reconnection event in the Earth’s magnetotail. Nat Phys, 2006, 2: 478–483

    Article  CAS  Google Scholar 

  10. Xiao C J, Wang X G, Pu Z Y et al., Satellite observations of separator-line geometry of three-dimensional magnetic reconnection. Nat Phys, 2007, 3: 609

    Article  CAS  Google Scholar 

  11. Greene J. Geometrical properties of three-dimensional reconnecting magnetic fields with nulls. J Geophys Res, 1988, 93: 8583–8590

    Article  Google Scholar 

  12. Garth C, Tricoche X, Scheuermann G. Tracking of vector field singularities in unstructured 3D time-dependent datasets. In Proceedings of IEEE Visualization, 2004, 329–336

  13. Deng X H, Matsumoto H, Kojima H, et al. GEOTAIL encounter with reconnection diffusion region in the Earth’s magnetotail: evidence of multiple X-lines collisionless reconnection. J Geophys Res, Vol. 109, A05206, doi:10.1029/2003JA010031, 2004

  14. Pritchett P L. Geospace environment modeling magnetic reconnection challenge: simulation with a full particle electromagnetic code. J Geophys Res, 2001, 106: 3783–3798

    Article  Google Scholar 

  15. Runov A, Nakamura R, Baumjohann W, et al. Current sheet structure near magnetic X-line observed by Cluster. Geophys Res Lett, 2003, 30, doi: 10.1029/2002GL016730

  16. Oieroset M, Phan T D, Fujimoto M, et al. In situ detection of collisionless reconnection in the Earth’s magnetotail. Nature, 2001. 412–414

  17. Harvey C C. In Analysis Methods for Multi-Spacecraft Data. 1998 (ESA Publications Division, Noordwijk): 307–322

    Google Scholar 

  18. Chanteur G. In Analysis Methods for Multi-Spacecraft Data. 1998 (ESA Publications Division, Noordwijk): 349–369

    Google Scholar 

  19. Khurana K K, Kepko G L, Kivelson M G, et al. Accurate determination of magnetic field gradients from four-point vector measurements-II: use of natural constraints on vector data obtained from four spinning spacecraft. IEEE Trans Magn, 1996, 32: 5193–5205

    Article  Google Scholar 

  20. Priest E R, Horning G, Pontin D I. On the nature of three-dimensional magnetic reconnection. J Geophys Res, 108, 2003, doi: 10.1029/2002JA009812

  21. Pontin D I, Horing G, Priest E R. Kinematic reconnection at a magnetic null point: spine-aligned current. Geophys Astrophy Flu Dynam, 2004, 98: 407–428

    Article  Google Scholar 

Download references

Author information

Authors and Affiliations

Authors

Corresponding author

Correspondence to XiaoHua Deng.

Additional information

Supported by the National Natural Science Foundation of China (Grant Nos. 40390153, 40574073, 40574074, 40640420563) and the Outstanding Young Scientists Founding of China (Grant No. 40325012)

About this article

Cite this article

Hu, Y., Deng, X., Zhou, M. et al. Structures of magnetic null points in reconnection diffusion region: Cluster observations. Chin. Sci. Bull. 53, 1880–1886 (2008). https://doi.org/10.1007/s11434-008-0173-0

Download citation

  • Received:

  • Accepted:

  • Published:

  • Issue Date:

  • DOI: https://doi.org/10.1007/s11434-008-0173-0

Keywords

Navigation