Add to ORKGThe dynamics and structure of the magnetosheath and the magnetopause, a new theory of MHD shock wave...
It is well-known that interplanetary magnetic clouds can cause strong geomagnetic storms due to the...
Magnetopause and bow shock boundaries from IMP-2 satellite and operations of plasma detecto
The Sun often ejects large quantities of magnetic field embedded plasma called magnetic clouds. Thes...
Structure of plane magnetohydrodynamic shock wave in rarefied fully ionized plasm
Shock tube experiments to determine interaction of hypersonic flow with magnetic fiel
Structure of interplanetary shock waves formed by interaction of geomagnetic field and solar wind - ...
Abstract. In various space plasma environments, like the solar corona, Earth’s magnetopause or in th...
Magnetohydrodynamic flow model for interaction of solar wind and geomagnetic fiel
We investigate three-dimensional (3-D) bow shocks in a highly collisional magnetized aluminium plasm...
Solar wind and geomagnetic field interaction in terms of continuum theory of fluid flo
A key parameter in determining the flow of the solar wind around the magnetosphere is the Alfven Mac...
We present an ideal MHD theory to describe for the first time the “magnetic barrier” (or “depletion ...
Context. The transition of the magnetic field from the ambient magnetic field to the eject...
The one-dimensional magnetohydrodynamics of shocked flows subjected to significant mass loading are ...
The dynamics and structure of the magnetosheath and the magnetopause, a new theory of MHD shock wave...
It is well-known that interplanetary magnetic clouds can cause strong geomagnetic storms due to the...
Magnetopause and bow shock boundaries from IMP-2 satellite and operations of plasma detecto
The Sun often ejects large quantities of magnetic field embedded plasma called magnetic clouds. Thes...
Structure of plane magnetohydrodynamic shock wave in rarefied fully ionized plasm
Shock tube experiments to determine interaction of hypersonic flow with magnetic fiel
Structure of interplanetary shock waves formed by interaction of geomagnetic field and solar wind - ...
Abstract. In various space plasma environments, like the solar corona, Earth’s magnetopause or in th...
Magnetohydrodynamic flow model for interaction of solar wind and geomagnetic fiel
We investigate three-dimensional (3-D) bow shocks in a highly collisional magnetized aluminium plasm...
Solar wind and geomagnetic field interaction in terms of continuum theory of fluid flo
A key parameter in determining the flow of the solar wind around the magnetosphere is the Alfven Mac...
We present an ideal MHD theory to describe for the first time the “magnetic barrier” (or “depletion ...
Context. The transition of the magnetic field from the ambient magnetic field to the eject...
The one-dimensional magnetohydrodynamics of shocked flows subjected to significant mass loading are ...
The dynamics and structure of the magnetosheath and the magnetopause, a new theory of MHD shock wave...
It is well-known that interplanetary magnetic clouds can cause strong geomagnetic storms due to the...
Magnetopause and bow shock boundaries from IMP-2 satellite and operations of plasma detecto