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Madhurjya P. Bora

Publications and source records attributed to Madhurjya P. Bora.

13 recordsLinked to original sources

Plasma localization of charged debris

We investigate whether the plasma disturbances generated by a charged debris object can be used to infer its position without directly sampling the object or its immediate sheath. A one-dimensional open-boundary electrostatic particle-in-cell (PIC) framework is used to model a continuously flowing electron-ion plasma containing an initially uncharged debris object. The debris charges self-consistently and produces an ion-ion counter-streaming instability (IICSI), which is sustained and reaches a statistically stationary state. A matching simulation without debris provides a controlled background against which debris-induced changes in different plasma fields are identified. The precursor and wake are examined through their spatial extent, fluctuation power, and frequency--wavenumber spectra. Weak-form sparse regression is then used as a supporting tool to recover reduced fluid and kinetic residuals and to learn an empirical relation connecting the precursor and wake disturbance envelopes to the equilibrium plasma flow, debris charge, and distance from the source. The predictive capability is examined by successively treating each simulation as an independent case. For each evaluation, the model is constructed from the remaining simulations, while the excluded simulation is used only to infer the debris position from its plasma response. For the idealized cold-ion regime considered here, the procedure successfully localizes the debris in transonic and supersonic flows, whereas the subsonic cases remain unresolved. These results demonstrate that debris-induced plasma disturbances possess a learnable spatial structure and provide a proof-of-principle route toward future remote localization using more realistic multidimensional models; they do not constitute an operational debris-detection scheme.

physics.plasm-ph↗

Thermal instability and multiphase dynamics in the ISM with polybaric pressure effects

In this work, we have carried out a two-dimensional (2D) simulation of thermal instability (TI) in interstellar matter (ISM), considering it to be a weakly ionised inviscid plasma with radiation loss. We carry out the simulation using our multi-fluid flux-corrected transport (mFCT) code, which incorporates a background magnetic field and anisotropic pressure. The anisotropic pressure is modelled with a polybaric pressure model. The findings of our analysis are consistent with the contemporary status of knowledge about the multiphase nature of the ISM, with volume and mass fractions of the various components of the ISM, that is, warm, cold, and unstable neutral matter (UNM) in the ranges reported by various numerical and observational analyses. Though the strength of the background magnetic field only marginally affects the overall evolution, the ratio of the parallel and perpendicular pressures can considerably alter the mass and volume fractions of the three phases, which can affect the overall evolution of the TI in the long run.

physics.plasm-ph↗

External charged debris in a flowing plasma : charge fluctuation induced complexity

In this work, we investigate the response of a flowing e-i plasma to embedded external charged debris, focusing on the periodic debris charge fluctuations that can trigger complex phenomena such as chaos and nonlinear Landau damping. We employ both kinetic and fluid simulations to analyse the plasma response to the time-dependent debris charge. Our findings indicate that the nature of the nonlinear response can be considerably different for fluctuating positively charged external debris from negatively charged debris. The simulations show that the debris charge fluctuation causes damping of the ion-acoustic wave as the debris velocity nears the ion-acoustic speed through nonlinear Landau damping and wave-wave interactions. We also present a theoretical framework to support the simulation findings. Our findings provide critical insights into debris-plasma interactions, which may be useful in applications involving space debris management.

physics.plasm-ph↗

Exploring nonlinearities in a positive ion-negative ion (PINI) plasma: can other processes mimic debris-induced effects?

In this work, an analysis of nonlinear waves and structures induced by an external charged debris in a positive ion-negative ion (PINI) plasma is presented. The results obtained are compared with findings from available experiments involving PINI plasma. The process of formation of different nonlinear structures is examined theoretically through a forced Korteweg-de Vries (fKdV) equation, which is also verified with a multi-fluid flux-corrected transport simulation code mFCT. Various processes which are responsible for different nonlinear waves and structures excited by differently charged external debris are pointed out. This work also points out the similarities in different nonlinear structures {excited} by an external charged debris and the underlying processes (this work) and those {observed experimentally through processes that do not involve any external debris.

physics.plasm-ph↗

External charge perturbation in a flowing plasma and electrostatic turbulence

In this work, an 1D electrostatic hybrid-Particle-in-Cell-Monte-Carlo-Collisionh-PIC-MCC) code is used to study the response of a plasma to a moving, external, charged perturbation (debris). We show that the so-called pinned solitons can form only under certain specific conditions through a turbulent regime of the ion-ion counter-streaming electrostatic instability (IICSI). In fact, the pinned solitons are manifestation of the ion phase-space vortices formed around the debris. The simulation shows that the pinned solitons can form only when the debris charge density exceeds a certain value causing the counter-streaming ion velocity to exceed a critical velocity, pushing the instability to a turbulent regime. The effect of debris velocity is also essential for the appearance of pinned soliton as when the debris velocity increases, it causes the widening of the phase space vortices causing well-separated pinned solitons, which merge to form one single soliton when debris velocity reduces to zero. In the opposite extreme, when debris velocity becomes highly supersonic, the vortices are widened up to a limit causing the pinned solitons to disappear altogether. We further show the existence of a Kolmogorov-type energy cascade scaling for this electrostatic turbulence.

physics.plasm-ph↗

Fast-moving electrostatic solitons in a plasma with turbulence heating

In this work, it is shown that electrostatic solitons in a plasma with turbulent heating of the electrons through an accelerating electric field can form with very high velocities, reaching up to several order of magnitudes larger than the equilibrium ion-sound speed. The possible parameter regime, where this work may be relevant, can be found in the so-called "dead zones" of a protoplanetary disk. Though these zones are stable to magnetorotational instability, the resultant turbulence can in fact heat the electrons making them follow a highly non- Maxwellian velocity distribution. We show that these fast-moving solitons can reach very high velocities. With electron velocity distribution described by the Davydov distribution function, we argue that these solitons can be an effective mechanism for energy equilibration in such a situation through soliton decay and radiation.

physics.plasm-ph↗

Counting the uncounted : estimating the unaccounted COVID-19 infections in India

Undetected infectious populations have played a major role in the COVID-19 outbreak across the globe and estimation of this undetected class is a major concern in understanding the actual size of the COVID-19 infections. Due to the asymptomatic nature of some infections, many cases have gone undetected. Also, despite carrying COVID-19 symptoms, most of the infected population kept the infections hidden and stayed unreported, especially in a country like India. Based on these factors, we have added an undetected compartment to the already developed SEIR model [48] to estimate these uncounted infections. In this article, we have applied Physics Informed Neural Network (PINN) to estimate the undetected infectious populations in the 20 worst-affected Indian states as well as India as a whole. The analysis has been carried out for the first as well as second surge of COVID-19 infections in India. A ratio of the active undetected infectious to the active detected infectious population is calculated through the PINN analysis which gives a picture of the real size of the pandemic in India. The rate at which symptomatic infectious population goes undetected and are never reported is also estimated using the PINN method. Toward the end, an artificial neural network (ANN) based forecasting scenario of the pandemic in India is presented. The prediction is found to be reliable as the training of the neural network has been carried out using the unique features, obtained from the state-wide analysis of the newly proposed model as well as from the PINN analysis.

q-bio.PE↗

Response of a dusty plasma system to external charge perturbations

The excitation of nonlinear wave structures in a dusty plasma caused by a moving external charge perturbation is examined in this work, which uses a 1-D flux corrected transport simulation. The plasma responds uniquely to different nature of the moving charge, depending on which, for small amplitude perturbations, pinned envelope solitons are generated and electrostatic dispersive ion-acoustic shock waves are formed for a large amplitude perturbation. The presence of dust particles is found to suppress the formation of dispersive shocks at low velocity of the external charge debris. The results are also investigated theoretically as a solution to the generalized Gross-Piteavskii equation, which broadly supports the simulation results.

physics.plasm-ph↗

Driven dust-charge fluctuation and chaotic ion dynamics in the plasma sheath and pre-sheath regions

Possible existence of chaotic oscillations in ion dynamics in the sheath and pre-sheath regions of a dusty plasma, induced by externally driven dust-charge fluctuation, is presented in this work. In a complex plasma, dust charge fluctuation occurs continuously with time due to the variation of electron and ions current flowing into the dust particles. In most of the works related to dust-charge fluctuation, theoretically it is assumed that the average dust-charge fluctuation follows the the plasma perturbation, while in reality, the dust-charge fluctuation is a semi-random phenomena, fluctuating about some average value. The very cause of dust-charge fluctuation in a dusty plasma also points to the fact that these fluctuations can be driven externally by changing electron and ion currents to the dust particles. With the help of a \emph{hybrid}-Particle in Cell-Monte Carlo (\emph{h}-PIC-MCC) code in this work, we use the plasma sheath as a candidate for driving the dust-charge fluctuation by periodically exposing the sheath-side wall to UV radiation, causing photoemission of electrons, which in turn drive the dust-charge fluctuation. We show that this \emph{driven} dust-charge fluctuation can induce a chaotic response in the ion dynamics in the sheath and the pre-sheath regions.

physics.plasm-ph↗

Nonlinear model of the firefly flash

A low dimensional nonlinear model based on the basic lighting mechanism of a firefly is proposed. The basic assumption is that the firefly lighting cycle can be thought to be a nonlinear oscillator with a robust periodic cycle. We base our hypothesis on the well known light producing reactions involving enzymes, common to many insect species, including the fireflies. We compare our numerical findings with the available experimental results which correctly predicts the reaction rates of the underlying chemical reactions. Toward the end, a time-delay effect is introduced for possible explanation of appearance of multiple-peak light pulses, especially when the ambient temperature becomes low.

nlin.CD↗

Thermal instability of an expanding dusty plasma with equilibrium cooling

We present an analysis of radiation induced instabilities in an expanding plasma with considerable presence of dust particles and equilibrium cooling. We have shown that the equilibrium expansion and cooling destabilize the radiation condensation modes and the presence of dust particles enhances this effect. We have examined our results in the context of ionized, dusty-plasma environments such as those found in planetary nebulae (PNe). We show that due to the non-static equilibrium and finite equilibrium cooling, small-scale localized structures formed out of thermal instability, become transient, which agrees with the observational results. The dust-charge fluctuation is found to heavily suppress these instabilities, though in view of non-availability of convincing experimental data, a definitive conclusion could not be made.

physics.plasm-ph↗

Sawtooth disruptions and limit cycle oscillations

A minimal (low-dimensional) dynamical model of the sawtooth oscillations is presented. It is assumed that the sawtooth is triggered by a thermal instability which causes the plasma temperature in the central part of the plasma to drop suddenly, leading to the sawtooth crash. It is shown that this model possesses an isolated limit cycle which exhibits relaxation oscillation, in the appropriate parameter regime, which is the typical characteristics of sawtooth oscillations. It is further shown that the invariant manifold of the model is actually the slow manifold of the relaxation oscillation.

nlin.CD↗

Thermal instability of an optically thin dusty plasma

We investigate the role of thermal instability, arising from radiative cooling of an optically thin, dusty plasma, by linear stability analysis. The corresponding isobaric stability condition for condensation mode is found to be modified significantly by the degree of ionization and concentration of finite sized, relatively heavy, and negatively charged dust particles. It has been shown that though the fundamental wave mode is similar in nature to the one in absence of dust particles, a new dust-wave mode can propagate in such a plasma. It is conjectured that the presence of negatively charged dust particles may considerably affect the stability of various astrophysical structures against thermal instability, which can not be explained with the help of gravitational instability.

physics.plasm-ph↗