Cylindrical Shock Waves in Space Superthermal Fluids
Article
First Online:
- 11 Downloads
Abstract
The three-dimensional Burgers equation is used to count the effects of the spectral index parameter κ, the ion, the negative (positive) kinematics viscosity coefficients of negatively (positively) charged grains on the dissipation of cylindrical shocks. The obtained results may useful for both laboratory and space applications of plasmas.
Keywords
Dust plasmas Cylindrical Burgers Dust cylindrical ion acoustic shocksPreview
Unable to display preview. Download preview PDF.
Notes
Acknowledgments
This project was supported by the deanship of scientific research at Prince Sattam Bin Abdulaziz University under the research project No. 10259/01/2019.
References
- [1]P. K. Shukla and A. Mamun, Introduction to Dusty Plasma Physics (CRC Press, Philadelphia, 2015).CrossRefGoogle Scholar
- [2]F. Verheest, Waves in Dusty Space Plasmas (kluver Academic publishers, Dordrecht, 2000).CrossRefGoogle Scholar
- [3]F. Melandsø and P. K. Shukla, Planet. Space Sci. 43, 635 (1995).ADSCrossRefGoogle Scholar
- [4]A. Barkan, R. L. Merlino and N. D’angelo, Phys. Plasmas 2, 3563 (1995).ADSCrossRefGoogle Scholar
- [5]N. Rao, P. Shukla and M.Y. Yu, Planet. Space Sci. 38, 543 (1990).ADSCrossRefGoogle Scholar
- [6]A. Barkan, N. D’angelo and R. Merlino, Planet. Space Sci. 44, 239 (1996).ADSCrossRefGoogle Scholar
- [7]P. Shukla and V. Silin, Physica Scripta 45, 508 (1992).ADSCrossRefGoogle Scholar
- [8]F. Melandsø, Phys. Plasmas 3, 3890 (1996).ADSCrossRefGoogle Scholar
- [9]C. Thompson, A. Barkan, N. D’angelo and R. Merlino, Phys. Plasmas 4, 2331 (1997).ADSCrossRefGoogle Scholar
- [10]A. Mamun, R. Cairns and P. Shukla, Phys. Plasmas 3, 2610 (1996).ADSCrossRefGoogle Scholar
- [11]B. Sahu and M. Tribeche, Astrophys. Space Sci. 338, 259 (2012).ADSCrossRefGoogle Scholar
- [12]D. Summers and R.M. Thorne, Phys. Fluids B: Plasma Phys. 3, 1835 (1991).CrossRefGoogle Scholar
- [13]M. Alam, M. Masud and A. Mamun, Chin. Phys. B 22, 115202 (2013).ADSCrossRefGoogle Scholar
- [14]M. Hossen, L. Nahar, S. Sultana and A. Mamun, High Energ. Dens. Phys. 13, 13 (2014).ADSCrossRefGoogle Scholar
- [15]M. Uddin, M. Alam and A. Mamun, Phys. Plasmas 22, 062111 (2015).ADSCrossRefGoogle Scholar
- [16]S. Popel, V. Tsytovich and M. Yu, Astrophys. Space Sci. 256, 107 (1997).ADSCrossRefGoogle Scholar
- [17]A. Rahman, A. Mamun and S. K. Alam, Astrophys. Space Sci. 315, 243 (2008).ADSCrossRefGoogle Scholar
- [18]S. Zaghbeer et al., J. Plasma Phys. 80, 517 (2014).ADSCrossRefGoogle Scholar
- [19]H. Abdelwahed and E. El-Shewy, Commun. Theor. Phys. 67, 90 (2017).ADSCrossRefGoogle Scholar
- [20]S. El-Labany, E. El-Shewy, H. A. El-Razek and A. A. El-Rahman, Commun. Theor. Phys. 70, 325 (2018).ADSCrossRefGoogle Scholar
- [21]E. El-Shewy and A. A. El-Rahman, Phys. Scr. 93, 115202 (2018).ADSCrossRefGoogle Scholar
- [22]H. G. Abdelwahed, Zeitschrift fu¨r Naturforschung A 73, 905 (2018).ADSCrossRefGoogle Scholar
- [23]M. Y. Wu, H. Wu, Q. M. Lu and B. S. Xue, Chinese Phys. Lett. 27, 95201 (2010).CrossRefGoogle Scholar
- [24]H. Abdelwahed, E. El-Shewy, A. Mahmoud, Chinese Phys. Lett. 34, 035202 (2017).ADSCrossRefGoogle Scholar
- [25]T. Taniuti and C. C. Wei, J. Phys. Soc. Jpn 24, 941 (1968).ADSCrossRefGoogle Scholar
- [26]S. Popel et al., Phys. Plasmas 12, 054501 (2005).ADSCrossRefGoogle Scholar
Copyright information
© The Korean Physical Society 2019