This paper is published in Volume-3, Issue-1, 2017
Area
Shock Wave
Author
Dr. Rohitashw Kumar, Arvind Kumar
Org/Univ
Babu Ram Singh Bhai Singh Memorial Degree College, Babrala, Uttar Pradesh, India
Keywords
Self-similar motion, Monochromatic radiation and Magneto-gas dynamic shock wave.
Citations
IEEE
Dr. Rohitashw Kumar, Arvind Kumar. Propagation of Spherical Shock Wave in A Non-Uniform Medium Under the Monochromatic Radiation and Gravitation, International Journal of Advance Research, Ideas and Innovations in Technology, www.IJARIIT.com.
APA
Dr. Rohitashw Kumar, Arvind Kumar (2017). Propagation of Spherical Shock Wave in A Non-Uniform Medium Under the Monochromatic Radiation and Gravitation. International Journal of Advance Research, Ideas and Innovations in Technology, 3(1) www.IJARIIT.com.
MLA
Dr. Rohitashw Kumar, Arvind Kumar. "Propagation of Spherical Shock Wave in A Non-Uniform Medium Under the Monochromatic Radiation and Gravitation." International Journal of Advance Research, Ideas and Innovations in Technology 3.1 (2017). www.IJARIIT.com.
Dr. Rohitashw Kumar, Arvind Kumar. Propagation of Spherical Shock Wave in A Non-Uniform Medium Under the Monochromatic Radiation and Gravitation, International Journal of Advance Research, Ideas and Innovations in Technology, www.IJARIIT.com.
APA
Dr. Rohitashw Kumar, Arvind Kumar (2017). Propagation of Spherical Shock Wave in A Non-Uniform Medium Under the Monochromatic Radiation and Gravitation. International Journal of Advance Research, Ideas and Innovations in Technology, 3(1) www.IJARIIT.com.
MLA
Dr. Rohitashw Kumar, Arvind Kumar. "Propagation of Spherical Shock Wave in A Non-Uniform Medium Under the Monochromatic Radiation and Gravitation." International Journal of Advance Research, Ideas and Innovations in Technology 3.1 (2017). www.IJARIIT.com.
Abstract
A self-similar, theoretical model of propagation of spherical shock wave in a magneto-gas dynamics rotating non-uniform atmosphere in the presence of monochromatic radiation and gravitation, is considered. The result discussed depends upon the variation of flow variables behind the shock, which is represented by graphically. A special case is considered in present and absence of gravitation along with rotation to observe the influence of gravitation.
