At an altitude of 1000-2000 km in the Venusian upper ionospheric region, the plasma is
composed of H+ ions, O+ ions, and solar wind (SW) protons with electrons distributed …

This investigation presents the study of dust kinetic Alfvén wave solitons (DKAWSs) and
quasi-periodic waves in a polarized dusty plasma comprising inertial dust, Cairns–Tsallis …

Motivated by the observations of dust-ion-acoustic waves (DIAWs) on the dark side of lunar
triggered by the interaction between the Earth's magnetosphere and lunar dust particles, we …

Electrostatic solitary waves (ESWs) in the Venusian ionosphere that are impinged by the
solar wind are investigated using a homogeneous, collisionless, and magnetized …

The aim is to state the properties of ion acoustic solitary waves in course of collision and
extract characteristics of the daughter wave in a magnetized electron–ion plasma. The …

Observations suggest that at altitudes of 1000–2000 km the interaction between the solar
wind and Venus' ionospheric plasma leads to ion-acoustic waves (IAWs) formation. For …

Formation of super rogue ion-acoustic wave is suggested as a physical catalyst for the
photochemical reaction to form the Venusian ionosphere and its mantle. Based on the …

Motivated by the recent Magnetospheric Multiscale (MMS) observations of oblique electron
acoustic waves, we addressed the generation mechanism of the observed waves by utilizing …

The origin of the solitary waves in the Earth's magnetosphere and the solar wind, particularly
close to the magnetic reconnection (MR) regions, is still an open question. For that purpose …

Space observations show that Venus suffers significant atmospheric erosion caused by the
solar wind forcing. Plasma acceleration is found to be one of the main mechanisms …