Gravitational Instability of Rotating Viscoelastic Partially Ionized Plasma in the Presence of an Oblique Magnetic Field and Hall Current
Figure 5
Variation of , given by (14), with the wavenumber for different values of magnetic field in direction when โgmโcmโ1โsecโ2, โmHโcmโ1, โsecโ1, โradโsecโ1, โgmโcmโ1โsecโ1, โgmโcmโ3, โcm2โsecโ1 and .