P
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.
Journal ArticleDOI
Theoretical interpretation of drift wave type fluctuations at the plasmapause
Padma Kant Shukla,S. Bujarbarua +1 more
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.