Hostname: page-component-cd9895bd7-mkpzs Total loading time: 0 Render date: 2024-12-28T13:32:29.906Z Has data issue: false hasContentIssue false
  • English
  • Français

Self-organized field structures in electron-depleted multi-ion dusty plasma

Published online by Cambridge University Press:  17 March 2015

M. Iqbal ,
S. M. Gondal ,
A. Shuaib  and
Qurat-ul-ain
M. Iqbal*
Affiliation:
Department of Physics, University of Engineering and Technology, Lahore 54890, Pakistan
S. M. Gondal
Affiliation:
Department of Physics, University of Engineering and Technology, Lahore 54890, Pakistan
A. Shuaib
Affiliation:
Department of Physics, University of Engineering and Technology, Lahore 54890, Pakistan
Qurat-ul-ain
Affiliation:
Key Laboratory for Laser Plasmas (MOE) & Department of Physics and Astronomy, Shanghai Jiao Tong University, Shanghai 200240, China
*
†Email address for correspondence: [email protected]
Get access Rights & Permissions [Opens in a new window]

Abstract

It is shown that there exists a strong interaction between the magnetic and kinetic aspects of a multi-ion plasma. The interaction appears as a system of simultaneous equations which show the alignment of vortices to flows and satisfy the Beltrami condition. Solving these equations lead to a non-force-free magnetic field which can be cast as a superposition of three multiscale force-free magnetic field configurations. It is the consequence of different Beltrami parameters of positive and negative ion fluids. It is also shown that self-organized paramagnetic and diamagnetic field structures could be created by varying the vorticities and flows of ion fluids.

Type
Research Article
Information
Journal of Plasma Physics , Volume 81 , Issue 3 , June 2015 , 905810319
Check for updates
Copyright
Copyright © Cambridge University Press 2015 

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

References

REFERENCES

Brinca, A. L. and Tsurutani, B. T. 1987 Astron. Astrophys. 187, 311.Google Scholar
Burlaga, L.et al. 1998 J. Geophys. Res. 103, 277.CrossRefGoogle Scholar
Chaizy, P.et al. 1991 Nature 349, 393.CrossRefGoogle Scholar
Chandrasekhar, S. and Kendall, P. C. 1957 Astrophys. J. 126, 457.CrossRefGoogle Scholar
El-Tantawy, S. A. and Moslem, W. M. 2012 Astrophys. Space Sci. 337, 219.CrossRefGoogle Scholar
Hultqvist, B., Øieroset, M., Paschmann, G. and Treumann, R. 1999 Magnetospheric Plasma Sources and Losses. Dordrecht: Kluwer.CrossRefGoogle Scholar
Iqbal, M. 2014 J. Plasma Phys. 80, 59.CrossRefGoogle Scholar
Iqbal, M., Berezhiani, V. I. and Yoshida, Z. 2008 Phys. Plasmas 15, 032905.CrossRefGoogle Scholar
Iqbal, M. and Shukla, P. K. 2012 Phys. Plasmas 19, 033517CrossRefGoogle Scholar
Kim, E.-H., Johnson, J. R., Lee, D.-H. and Pyo, Y. S. 2013 Earth Planets Space 65, 447.CrossRefGoogle Scholar
Liang, P. E., Wilks, S. C. and Tabak, M. 1998 Phys. Rev. Lett. 81, 4887.CrossRefGoogle Scholar
Mahajan, S. M. and Yoshida, Z. 1998 Phys. Rev. Lett. 81, 4863.CrossRefGoogle Scholar
Mamun, A. A., Cairns, R. A. and Shukla, P. K. 1996 Phys. Plasmas 3, 702.CrossRefGoogle Scholar
Ohsaki, S. and Yoshida, Z. 2005 Phys. Plasmas 12, 064505.CrossRefGoogle Scholar
Oohara, W., Date, D. and Hatakeyama, R. 2005 Phys. Rev. Lett. 95, 175003.CrossRefGoogle Scholar
Oohara, W. and Hatakeyama, R. 2003 Phys. Rev. Lett. 91, 205005.CrossRefGoogle Scholar
Oohara, W. and Hatakeyama, R. 2007 Phys. Plasmas 14, 055704.CrossRefGoogle Scholar
Schwenn, R. and Marsch, E. 1990 Physics of the Inner Helioshere: Large Scale Phenomena. Berlin: Springer.Google Scholar
Shemansky, D. E. and Hall, D. T. 1992 J. Geophys. Res. 97, 4143.CrossRefGoogle Scholar
Stasiewics, K. 2004 Phys. Rev. Lett. 12 125004.CrossRefGoogle Scholar
Shukla, P. K. and Mahajan, S. M. 2004 Phys. Lett. A 328, 185.CrossRefGoogle Scholar
Taylor, J. B. 1974 Phys. Rev. Lett. 33, 1139.CrossRefGoogle Scholar
Tribeche, M., Younasi, S. and Zerguini, T. H. 2008 Can. J. Phys. 86, 975.CrossRefGoogle Scholar
Tsytovich, V. N., Sato, N. and Morfill, G. E. 2003 New J. Phys. 5, 43.CrossRefGoogle Scholar
Yoshida, Z. and Giga, Y. 1990 Math. Z. 204, 235.CrossRefGoogle Scholar
Yoshida, Z. and Mahajan, S. M. 1999 J. Math. Phys. 40, 5080.CrossRefGoogle Scholar
Zurbuchen, T. H.et al. 2008 Science 321, 90.CrossRefGoogle Scholar