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Aeronautics and Aerospace Open Access Journal

Research Article Volume 2 Issue 5

A note on modeling a void generation and contraction in complex plasma

OV Kravchenko,1 OA Azarova2

1Scientific and Technological Center of Unique Instrumentation of RAS, Russia
2Dorodnicyn Computing Centre, Federal Research Center, "Computer Science and Control" of RAS, Russia

Correspondence: Olga A Azarova, Dorodnicyn Computing Centre, Federal Research Center, "Computer Science and Control" of RAS, Vavilova str. 40, Russia, Moscow , Tel 74991350002

Received: August 24, 2018 | Published: September 26, 2018

Citation: Kravchenko OV, Azarova OA. A note on modeling a void generation and contraction in complex plasma. Aeron Aero Open Access J. 2018;2(5):283-285. DOI: 10.15406/aaoaj.2018.02.00062

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Abstract

An empty region (void) has been observed in many experiments on complex (dusty) plasma in particular which were taken place at the International Space Station. Here the known model of Avinash, Bhattacharjee and Hu of formation of void in complex plasma is considered to provide simulations of voids evolution from initially unstable flow mode. The model has been transformed into the divergent form. The MUSCL scheme of the second approximation order in space and in time has been applied for the hydrodynamic part of the model and a MINMOD limiter has been used for obtaining monotonic solution. As a result the dynamics of void’s growth and its partial contraction to the center have been obtained at the final stage of the void evolution.

Keywords: dusty plasma, complex plasma void, numerical methods, MUSCL scheme, plasma simulation

Nomenclature

nd, ne                       = densities of dust and electrons components

vd, vi                        = velocities of dust and ions components

E = electric field currency

Fd                            = ion-drag force

D0                            = diffusion coefficient

t, x, y                       = time and spatial variables

a, b                         = fit parameters of ion-drag force approximation

µ                             = coefficient of ions mobility

α0                            = friction coefficient

τd, τi                         = coefficients of normalized temperature for dust and ion

species

ni                             = amount of the grid points in the x-direction

Index “0” refers to the initial parameters

Introduction

Recently a field connected with the research of complex plasma is widely investigated.1‒3 One of the first complex plasma patterns containing a domain which is free of dust particles (void) was observed in the course of the experiments on the board of the International Space Station3. Afterwards similar patterns were found at the laboratory conditions.4‒6 To describe such a pattern formation the model of Avinash, Bhattacharjee and Hu was introduced.7,8 In this model the evolution of the dynamics of a single symmetric void from an equilibrium state is described by electro-hydrodynamic equations which take into account the effect of an ion attraction force as a nonlinear function of the speed of ions. The algorithm for modeling the appearance of complex plasma void by means of the model has been presented for the case of cylindrical geometry of the electrical field8. Also, generation of a single symmetric void and concentric symmetrical voids in unmoving flows of low-temperature complex plasma has been obtained.9,10 A study of generation of both voids in moving flows11 and unmoving media was presented.12 Recently the Lax’s scheme with re-calculation11 and the complex conservative difference scheme13 have been used for the hydrodynamic part of the model. At the same time, the MUSCL scheme is a widely using tool in hydrodynamic14 and plasma simulations.15 This paper is devoted to the MUSCL scheme application to a void evolution with respect to the contraction process. The simulations are based on the algorithm with using a predictor-corrector procedure for obtaining the second approximation order in space and in time and a MINMOD limiter is used for obtaining monotonic solution. Presented results can be used in research of dusty plasma dynamics under the conditions of microgravity which may associate with the conditions in space.

Model

Modeling is based on the model Avinash et al.8 Governing equations considered in dimensionless form with respect to the normalizing parameters8 have been applied:

, v d t + v d v d x = F d E α 0 v d τ d n d n d x MathType@MTEF@5@5@+= feaagKart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaqcfaieaaaaaa aaa8qadaWcaaGcpaqaaKqzGeWdbiabgkGi2kaadAhajuaGpaWaaSba aSqaaKqzadWdbiaadsgaaSWdaeqaaaGcbaqcLbsapeGaeyOaIyRaam iDaaaacqGHRaWkcaWG2bqcfa4damaaBaaaleaajugWa8qacaWGKbaa l8aabeaajuaGpeWaaSaaaOWdaeaajugib8qacqGHciITcaWG2bqcfa 4damaaBaaaleaajugWa8qacaWGKbaal8aabeaaaOqaaKqzGeWdbiab gkGi2kaadIhaaaGaeyypa0JaamOraKqba+aadaWgaaWcbaqcLbmape GaamizaaWcpaqabaqcLbsapeGaeyOeI0IaamyraiabgkHiTiabeg7a HLqba+aadaWgaaWcbaqcLbmapeGaaGimaaWcpaqabaqcLbsapeGaam ODaKqba+aadaWgaaWcbaqcLbmapeGaamizaaWcpaqabaqcLbsapeGa eyOeI0scfa4aaSaaaOWdaeaajugib8qacqaHepaDjuaGpaWaaSbaaS qaaKqzadWdbiaadsgaaSWdaeqaaaGcbaqcLbsapeGaamOBaKqba+aa daWgaaWcbaqcLbmapeGaamizaaWcpaqabaaaaKqba+qadaWcaaGcpa qaaKqzGeWdbiabgkGi2kaad6gajuaGpaWaaSbaaSqaaKqzadWdbiaa dsgaaSWdaeqaaaGcbaqcLbsapeGaeyOaIyRaamiEaaaaaaa@760B@    (1)

, n d t  = ( n d v d ) x + D 0 2 n d x 2 MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaqcfaieaaaaaa aaa8qadaWcaaGcpaqaaKqzGeWdbiabgkGi2kaad6gajuaGpaWaaSba aSqaaKqzadWdbiaadsgaaSWdaeqaaaGcbaqcLbsapeGaeyOaIyRaam iDaaaapaGaafiiaiaqb2dapeGaeyOeI0scfa4aaSaaaOWdaeaajugi b8qacqGHciITcaGGOaGaamOBaKqba+aadaWgaaWcbaqcLbmapeGaam izaaWcpaqabaqcLbsapeGaamODaKqba+aadaWgaaWcbaqcLbmapeGa amizaaWcpaqabaqcLbsapeGaaiykaaGcpaqaaKqzGeWdbiabgkGi2k aadIhaaaGaey4kaSIaamiraKqba+aadaWgaaWcbaqcLbmapeGaaGim aaWcpaqabaqcfa4dbmaalaaak8aabaqcLbsapeGaeyOaIyBcfa4dam aaCaaaleqabaqcLbmapeGaaGOmaaaajugibiaad6gajuaGpaWaaSba aSqaaKqzadWdbiaadsgaaSWdaeqaaaGcbaqcLbsapeGaeyOaIyRaam iEaKqba+aadaahaaWcbeqaaKqzadWdbiaaikdaaaaaaaaa@67A9@      (2)

, d n e dx = n e E τ i MathType@MTEF@5@5@+= feaagKart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaqcfa4aaSaaaO qaaKqzGeGaamizaiaad6gajuaGdaWgaaWcbaqcLbmacaWGLbaaleqa aaGcbaqcLbsacaWGKbGaamiEaaaacqGH9aqpcqGHsisljuaGdaWcaa GcbaqcLbsacaWGUbqcfa4aaSbaaSqaaKqzadGaamyzaaWcbeaajugi biaadweaaOqaaKqzGeGaeqiXdqxcfa4aaSbaaSqaaKqzadGaamyAaa Wcbeaaaaaaaa@4BF7@         (3)

, dE dx =1 n e n d MathType@MTEF@5@5@+= feaagKart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaqcfa4aaSaaaO qaaKqzGeGaamizaiaadweaaOqaaKqzGeGaamizaiaadIhaaaGaeyyp a0JaaGymaiabgkHiTiaad6gajuaGdaWgaaWcbaqcLbmacaWGLbaale qaaKqzGeGaeyOeI0IaamOBaKqbaoaaBaaaleaajugWaiaadsgaaSqa baaaaa@4728@        (4)

. F d = aE b+ | v i | 3 , v i =μE MathType@MTEF@5@5@+= feaagKart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbiqaaWUfjugibi aadAeajuaGdaWgaaWcbaqcLbmacaWGKbaaleqaaKqzGeGaeyypa0tc fa4aaSaaaOqaaKqzGeGaamyyaiaadweaaOqaaKqzGeGaamOyaiabgU caRKqbaoaaemaakeaajugibiaadAhajuaGdaWgaaWcbaqcLbmacaWG PbaaleqaaaGccaGLhWUaayjcSdqcfa4aaWbaaSqabeaajugWaiaaio daaaaaaKqzGeGaaiilaiaaysW7caaMe8UaaGjbVlaadAhajuaGdaWg aaWcbaqcLbmacaWGPbaaleqaaKqzGeGaeyypa0JaeqiVd0Maamyraa aa@5ABB@       (5)

Here concentrations of dust and electrons components are nd, ne; velocities of dust and ions components are vd, vi; electric field currency is E, ion-drag force is Fd, diffusion coefficient is D0. In the system (1)-(5): (1) is the dust momentum and (2) is the dust continuity equations, (3) is the balance equation of electrons neglecting the electron inertia, the Poisson law which completes the nonlinear system of equations, and the expressions for ion–drag force presented in (4, 5) constitute the governing equations. Also, one can consider equations (1) and (2) as the hydrodynamic part of the model9‒12 and the equations (3)-(5) are the electrostatic part of it.

Methods

The hydrodynamic part of the model can be expressed in the divergent form

u t + F x =f, MathType@MTEF@5@5@+= feaagKart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaqcfa4aaSaaaO qaaKqzGeGaeqOaIylcbeGaa8xDaaGcbaqcLbsacqaHciITcaWG0baa aiabgUcaRKqbaoaalaaakeaajugibiabekGi2kaa=zeaaOqaaKqzGe GaeqOaIyRaamiEaaaacqGH9aqpcaWFMbGaa8hlaiaa=bcacaWFGaaa aa@47A1@      (6)

where

u=( n d v d ),F=( n d v d 0.5 v d 2 + τ d ln n d ),f=( D 0 2 n d x 2 F d E α 0 v d ). MathType@MTEF@5@5@+= feaagKart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaacbeqcLbsaca WF1bGaeyypa0tcfa4aaeWaaOqaaKqzGeqbaeqabiqaaaGcbaqcLbsa caWGUbqcfa4aaSbaaSqaaKqzadGaamizaaWcbeaaaOqaaKqzGeGaam ODaKqbaoaaBaaaleaajugWaiaadsgaaSqabaaaaaGccaGLOaGaayzk aaqcLbsacaGGSaGaa8Nraiabg2da9Kqbaoaabmaakeaajugibuaabe qaceaaaOqaaKqzGeGaamOBaKqbaoaaBaaaleaajugWaiaadsgaaSqa baqcLbsacaWG2bqcfa4aaSbaaSqaaKqzadGaamizaaWcbeaaaOqaaK qzGeGaaGimaiaac6cacaaI1aGaamODaKqbaoaaDaaaleaajugWaiaa dsgaaSqaaKqzadGaaGOmaaaajugibiabgUcaRiabes8a0LqbaoaaBa aaleaajugWaiaadsgaaSqabaqcLbsaciGGSbGaaiOBaiaad6gajuaG daWgaaWcbaqcLbmacaWGKbaaleqaaaaaaOGaayjkaiaawMcaaKqzGe Gaaiilaiaa=zgacqGH9aqpjuaGdaqadaGcbaqcLbsafaqabeGabaaa keaajugibiaadseajuaGdaWgaaWcbaqcLbmacaaIWaaaleqaaKqbao aalaaakeaajugibiabgkGi2MqbaoaaCaaaleqabaqcLbmacaaIYaaa aKqzGeGaamOBaKqbaoaaBaaaleaajugWaiaadsgaaSqabaaakeaaju gibiabgkGi2kaadIhajuaGdaahaaWcbeqaaKqzadGaaGOmaaaaaaaa keaajugibiaadAeajuaGdaWgaaWcbaqcLbmacaWGKbaaleqaaKqzGe GaeyOeI0IaamyraiabgkHiTiabeg7aHLqbaoaaBaaaleaajugWaiaa icdaaSqabaqcLbsacaWG2bqcfa4aaSbaaSqaaKqzadGaamizaaWcbe aaaaaakiaawIcacaGLPaaajugibiaac6caaaa@924E@

Earlier the centered scheme was applied to the hydrodynamic part of the model as well as the Lax’s scheme with re-calculation.10 The eq. (6) was approximated with the second order using central scheme and the method of Runge-Kutta of the fourth order was used to calculate (3), (4).10 Also, in the numerical simulations the next restrictions were imposed: if nd>1 then nd was applied by 1 and vd was applied by vd0. Here we apply the MUSCL scheme to (6). The algorithm is free of any restrictions on nd and vd. A predictor-corrector procedure is used for obtaining the second approximation order in space and in time. To obtain monotonic shape of the numerical solution a MINMOD limiter based on the values nd is utilized. Parameters of the simulations are collected in Table 1.

Parameter

Value

D0

0

τi

0.125

τd

0.001

a

7.5

b

1.6

α0

2

µ

1.5

ne0

0.999

E0

10-6

Table 1 Parameters of the simulations

Results

The evolution of void generation in time in the initially unmoving flow (vd0=0) is presented in Figure 1 and Figure 2. The dynamics of dusty particles density nd is shown in Figures 1A-1D and the dynamics of dusty particles velocity vd is shown in Figures 2A-2D. Here two-dimensional plots for ndvd obtained by the rotation technique are presented. The mechanism of generation of voids is based on the superposition of the electrical field and the ion attraction force action. Void develops in time from the uniformly distributed density and velocity values with constant parameters. The initial circular structure is shown in Figure 1A, the void becomes saturated at t=300 and the contraction process occurs up to t=1000.

Figure 1 Evolution of the density of dust particles nd.

Figure 2 Evolution of the velocity of dust particles vd.

Conclusion

Generation of a pattern with empty region (void) has been modelled numerically in complex plasma. The modeling is based on the Avinash, Bhattacharjee and Hu model of a void formation. The model has been reduced to the divergent form and the MUSCL scheme of the second approximation order has been used for the hydrodynamic part of the model. Dynamics of the void parameters such as density and velocity of dust particles has been obtained. It has been shown that after the initial stage of the circular void structure formation and before the steady state establishing the intermediate stage occurs of a void subsequent expansion and partial contraction to the center.

Acknowledgements

None.

Conflict of interest

The author declares that there is no conflict of interest.

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