On the shock wave structures in anisotropy magnetoplasmas

Author:

Albalawi Wedad1,Hammad Ma’mon Abu2,Khalid Muhammad3ORCID,Kabir Abdul4,Tiofack C. G. L.5ORCID,El-Tantawy S. A.67ORCID

Affiliation:

1. Department of Mathematical Sciences, College of Science, Princess Nourah bint Abdulrahman University 1 , P.O. Box 84428, Riyadh 11671, Saudi Arabia

2. Department of Mathematics, Al-Zaytoonah University of Jordan 2 , Amman 11733, Jordan

3. Department of Physics, Government Post Graduate College Swabi 3 , Swabi 23431, Khyber Pakhtunkhwa, Pakistan

4. GNSS Research Lab National Center of GIS & Space Applications Department of Space Science Institute of Space Technology 4 , Islamabad, Pakistan

5. Faculty of Sciences, University of Maroua 5 , P.O. Box 814, Maroua, Cameroon

6. Department of Physics, Faculty of Science, Port Said University 6 , Port Said 42521, Egypt

7. Research Center for Physics (RCP), Department of Physics, Faculty of Science and Arts, Al-Mikhwah, Al-Baha University 7 , Al-Baha 1988, Saudi Arabia

Abstract

In this work, the propagation of nonlinear electrostatic shock wave structures in an anisotropy pressure magnetoplasma composed of warm inertial ions and inertia-less Maxwellian electrons is reported. For this purpose, the technique of reductive perturbation is applied for reducing fluid equations of the current model to the Korteweg–de Vries Burgers (KdVB) equation with a second-order dissipative term and the KdVB–Kuramoto (KBK) equation with both second- and fourth-order dissipative terms. The impact of various plasma parameters, including the parallel ion pressure, perpendicular ion pressure, and dissipation parameter, on the significant characteristics of the shock wave profile is examined and discussed. In addition, a comparison between the profiles of KdVB shocks and KdVB–Kuramoto shocks is reported. We expect that KBK shock wave amplitudes become larger than the KdVB ones by taking the fourth-order dissipative into consideration. Thus, the results of the KBK equation may treat the difference between the theoretical and laboratory results or satellite observations.

Funder

Princess Nourah Bint Abdulrahman University

Al-Zaytoonah University of Jordan

Publisher

AIP Publishing

Subject

General Physics and Astronomy

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