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In present paper, field aligned whistler mode waves are analyzed, in the presence of DC field in background plasma having relativistic distribution function in the magnetosphere of Uranus.

Along with the real parts of the effective refractive index functions for the O- and X-mode waves, the swelling factors for both characteristic mode waves are also calculated.

As is well known, whistler mode waves are electromagnetic waves in a magnetized plasma that propagate through the magnetosphere at frequencies below the electron-cyclotron frequency and electron plasma frequency.

In order to maximize the soundproofing ability, the selection of size and placement of input and output openings in such a way that would minimize the effects of higher-order mode waves are considered in details.

The shear Alfven mode has magnetic field guided energy which forms standing field line resonances (FLRs) between conjugate ionospheres while the boundaries for fast mode waves are still unclear although the fast mode turning point as a boundary appears to be undisputed.

On the edge of the Io wake, mirror mode waves were seen where the pickup ion contribution to the pressure anisotropy is sufficient to overcome the instability threshold.

Volwerk et al. (2008a, b) also conclude that the mirror mode waves detected in the Venus magnetosheath have periods between 5 and 15 s, and the probability to observe the mirror mode waves is higher at the dayside magnetosheath and is lower in the nightside magnetosheath.

As to the theoretical study, TEC oscillations observed after the 2011 off the Pacific coast of Tohoku Earthquake and FACs in the ionosphere generated by acoustic mode waves were well reproduced with numerical simulations by Matsumura et al. (2011) and by Zettergren and Snively (2013), respectively.

The team spotted a quadrapolar magnetic field which theorists think can only occur when whistler-mode waves are generated.

While normal-mode waves are characterized by dispersion relations associating frequencies with wavevectors and may be sustained for a long time, non-normal-mode waves are not strictly constrained to dispersion relations and may have a relatively shorter lifetime.

In the present study, we assumed that whistler-mode waves are excited by energetic electrons generated in the associated flare.