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Padma Kant Shukla

Researcher at Ruhr University Bochum

Publications -  1235
Citations -  37828

Padma Kant Shukla is an academic researcher from Ruhr University Bochum. The author has contributed to research in topics: Plasma & Electron. The author has an hindex of 84, co-authored 1232 publications receiving 35521 citations. Previous affiliations of Padma Kant Shukla include University of California, San Diego & University of KwaZulu-Natal.

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Theory of ion holes associated with electron-acoustic vortices

TL;DR: In this paper, a unified theory of ion holes and electron-acoustic vortices is presented, coupled with the hydrodynamic equations for electrons via the Poisson equation, and a novel type of nonlinear structures is found, which has the form of a quasi two-dimensional density rarefaction that is spatially localized by the ion trapping in the negative potential.
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Theoretical interpretation of drift wave type fluctuations at the plasmapause

TL;DR: In this paper, it was shown that an electrostatic pump near the upper hybrid resonance frequency can induce a new macroscopic parametric instability, which could be one of the candidates for the excitation of the low-frequency drift wave type fluctuations at the plasmapause.
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Modulational instability of dust-lattice waves in a plasma crystal

TL;DR: A nonlinear Schrodinger equation for the propagation of a dust-lattice wave in a one-dimensional chain of a plasma crystal is derived by using the Krylov-Bogoliubov-Mitropolsky (KBM) perturbation technique.
Proceedings ArticleDOI

Cylindrical nonlinear Schrödinger equation versus cylindrical Korteweg‐de Vries equation

TL;DR: In this article, a correspondence between the family of cylindrical nonlinear Schrodinger (cNLS) equations and the one of Cylindrical Korteweg-de Vries (cKdV) equations is constructed.
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Solar coronal heating by plasma waves

TL;DR: In this article, the plasma particle heating based on the kinetic theory of wave-particle interactions involving kinetic Alfven waves and lower-hybrid drift modes is presented, where the collisionless solar corona is ideal for supporting kinetic wave-plasma interactions.