Excitations of Distorted Magnetosonic Lump Waves by Orbital Charged Space Debris Objects in Ionospheric Plasma

We consider the forced Kadomtsev-Petviashvili I (KPI) equation derived in a recent work on magnetosonic waves excited by space debris objects of Acharya et al. [Adv. Space Res. 69, 4045–4057 (2022)] for further analysis in this work. For first time, we have derived a special exact distorted lump wave solution of the forced KPI equation for a specific localized form of the forcing function. The reason for choosing such a typical forcing function has been discussed in detail in the context of orbital motions of charged space debris objects in ionospheric plasma. Such exotic magnetosonic lump wave structures showing characteristic distortions resulted by orbital charged space debris objects can have potential implications in their indirect detection methods.