Abstract
A charged body moving in a plasma can excite a variety of linear and nonlinear waves in the form of trailing wakes, fore-wake shocks, and precursor solitons. These structures can further interact with the background plasma to create secondary effects that can serve as signatures of the passage of the charged body. Using particle-in-cell simulations, we carry out a basic investigation of the dynamics of a plasma system that is being traversed by an energetic charged body. Using two different shapes of this charged source, namely, an idealized infinite length planar source and a two-dimensional thin rectangular source, we examine the differences in the nature of the excited wave structures and their consequent impact on the background plasma. Our simulations reveal interesting features such as the dependence of the precursor speeds on the total charge on the driving source, local particle trapping, and energization of the trapped particles in various regions along the traversal path leading to the formation of energetic charged beamlets. Our basic findings could find practical applications such as in analyzing the trajectories of charged objects like space debris orbiting in the ionosphere.
Original language | English |
---|---|
Article number | 025207 |
Journal | Physical Review E - Statistical, Nonlinear, and Soft Matter Physics |
Volume | 107 |
Issue number | 2 |
DOIs | |
State | Published - Feb 2023 |
Funding
This paper has been coauthored by employees of UT-Battelle, LLC, under Contract No. DE-AC05-00OR22725 with the U.S. Department of Energy (DOE). The U.S. government retains and the publisher, by accepting the paper for publication, acknowledges that the U.S. government retains a nonexclusive, paid-up, irrevocable, worldwide license to publish or reproduce the published form of this paper, or allow others to do so, for U.S. government purposes. DOE will provide public access to these results of federally sponsored research in accordance with the DOE Public Access Plan . A.S. acknowledges AOARD for their research Grant No. FA2386-18-1-4022 and the Indian National Science Academy for support as an INSA Honorary Scientist. The authors would like to acknowledge the OSIRIS Consortium, consisting of UCLA and IST (Lisbon, Portugal), for providing access to the OSIRIS4.0 framework, which is the work supported by NSF No. ACI-1339893. The simulations for the work described in this paper were performed on Antya, an IPR Linux cluster in India.