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Dive into the research topics where G. S. Lakhina is active.

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Featured researches published by G. S. Lakhina.


Advances in Space Research | 2001

Broadband electrostatic noise due to nonlinear electron-acoustic waves

S.V. Singh; R. V. Reddy; G. S. Lakhina

Abstract Nonlinear propagation of electron-acoustic waves is examined in an unmagnetized, four-component plasma consisting of hot Maxwellian electrons, fluid cold and beam electrons and ions. Solitary structures which are a possible final stage of the electron-acoustic wave growth are obtained. The soliton amplitude and width are numerically obtained. The results are compared with the spiky structures of the broadband electrostatic noise observed in the auroral region of the Earths magnetosphere. The model predicts parallel electric fields ∼ (10–400) mV/m with typical half widths of the structures ∼ a few Debye lengths.


Planetary and Space Science | 1997

INFLUENCE OF DUST MASS DISTRIBUTIONS ON GENERALIZED JEANS-BUNEMAN INSTABILITIES IN DUSTY PLASMAS

Peter Meuris; Frank Verheest; G. S. Lakhina

Abstract The linear dispersion law is given for a generalized Jeans-Buneman instability in the presence of a dust mass distribution. It is shown that this instability is easier to evoke when a reasonable power law mass distribution for the dust grains is assumed than for the mono-sized dust case. For Boltzmann distributed ions and electrons the dust-acoustic mode and the unstable Jeans mode are modified due to the self-gravitation and mass distribution. The frequency of the dust-acoustic mode is increased. For long wavelengths, a new stable mode occurs, due only to the dust mass distribution. The growth rate of the Jeans instability is increased, and the mode is extended beyond the usual wavelength domain. For high values of k a new instability arises, which is called the dust distribution instability.


Journal of Plasma Physics | 2004

Gas-dynamic description of electrostatic solitons

Frank Verheest; Tom Cattaert; G. S. Lakhina; S. V. Singh

The nonlinear propagation of electrostatic solitary structures in unmagnetized multispecies plasmas is studied in the wave frame, where they are stationary. via the recently developed MeKenzie approach as an alternative to the more usual Saagdeev pseudo-potential method. This way of looking at the problem brings out the gas-dynamic aspects, which then allow a straightforward characterization of the solitary wave possibilities in terms of the species own sonic points and of the global charge neutral points. A qualitative discussion of ion-. dust- and electron-acoustic solitary waves is given in terms of these concepts and the results are contrasted with those obtained by other methods. Ion-acoustic solitons can be shown to always be compressive. without invoking simplifying assumptions such as cold ions or Boltzmann electrons. Beam-plasmas can also be studied, as in the electron-acoustic solitary wave model for the spiky structures of the broadband electrostatic noise observed in the auroral regions of the Earths magnetosphere. Such solitons always show a potential dip.


Astrophysics and Space Science | 1997

Alfvenic solitons in ultrarelativistic electron-positron plasmas

G. S. Lakhina; Frank Verheest

In electron-positron plasmas some of the plasma modes are decoupled due to the equal charge-to-mass ratio of both species. We derive the dispersion law for a low-frequency, generalized X-mode, which exists at all angles of propagation with respect to the static magnetic field. Its nonlinear evolution is governed by a Korteweg-de Vries equation, valid at all angles of propagation except strictly parallel propagation, for which a different approach leads to a vector form of the modified Korteweg-de Vries equation. The nonlinearity is strongest at perpendicular propagation. Ultrarelativistic effects are discussed.


Physica Scripta | 2011

Electron acoustic solitary waves with kappa-distributed electrons

S Devanandhan; S. V. Singh; G. S. Lakhina

Electron acoustic solitary waves are studied in a three-component, unmagnetized plasma composed of hot electrons, fluid cold electrons and ions having finite temperatures. Hot electrons are assumed to have kappa distribution. The Sagdeev pseudo-potential technique is used to study the arbitrary amplitude electron-acoustic solitary waves. It is found that inclusion of cold electron temperature shrinks the existence regime of the solitons, and soliton electric field amplitude decreases with an increase in cold electron temperature. A decrease in spectral index, κ, i.e. an increase in the superthermal component of hot electrons, leads to a decrease in soliton electric field amplitude as well as the soliton velocity range. The soliton solutions do not exist beyond Tc/Th>0.13 for κ=3.0 and Mach number M=0.9 for the dayside auroral region parameters.


Physics of Plasmas | 2014

Ion acoustic solitons/double layers in two-ion plasma revisited

G. S. Lakhina; S. V. Singh; Amar Kakad

Ion acoustic solitons and double layers are studied in a collisionless plasma consisting of cold heavier ion species, a warm lighter ion species, and hot electrons having Boltzmann distributions by Sagdeev pseudo-potential technique. In contrast to the previous results, no double layers and super-solitons are found when both the heavy and lighter ion species are treated as cold. Only the positive potential solitons are found in this case. When the thermal effects of the lighter ion species are included, in addition to the usual ion-acoustic solitons occurring at M > 1 (where the Mach number, M, is defined as the ratio of the speed of the solitary wave and the ion-acoustic speed considering temperature of hot electrons and mass of the heavier ion species), slow ion-acoustic solitons/double layers are found to occur at low Mach number (M < 1). The slow ion-acoustic mode is actually a new ion-ion hybrid acoustic mode which disappears when the normalized number density of lighter ion species tends to 1 (i.e.,...


Planetary and Space Science | 1992

Ion-acoustic double layers and solitons in multispecies auroral beam-plasmas

R. V. Reddy; G. S. Lakhina; Frank Verheest

Abstract A general analysis for small amplitude ion-acoustic double layers and solitons is developed, taking into account any number of ion beams and their charges, together with cold and hot electrons. For auroral plasma parameters, the analysis predicts the excitation of fast and slow hydrogen (as well as oxygen) beam-acoustic modes, which can be either rarefactive double layers or rarefactive or compressive solitons. Variations in the temperature and beam speed of the hydrogen (oxygen) beam can lead to the conversion of modes from originally rarefactive double layers to rarefactive solitons and finally to compressive solitons. Fast and slow hydrogen beam-acoustic modes are the first to be excited. The excitation of fast and slow oxygen modes is usually possible for larger values of beam speeds or beam temperatures. The typical width and speed of the nonlinear modes are in good agreement with the observations of double layers and solitons by the S 3-3 and Viking satellites.


Journal of Plasma Physics | 2005

Arbitrary amplitude dust-acoustic double layers in a non-thermal plasma

S. K. Maharaj; S. R. Pillay; R. Bharuthram; R. V. Reddy; S. V. Singh; G. S. Lakhina

The existence of large-amplitude dust-acoustic double layers is investigated in an unmagnetized dusty plasma comprising a negatively charged warm dust fluid, non-thermal ions and Boltzmann electrons. It is found that the non-thermal plasma supports the existence of rarefactive double layers only. The dependence of the double-layer amplitude and Mach number on various parameters such as the non-thermal parameter, dust temperature and electron concentration is numerically examined.


Physics of Plasmas | 2014

Ion acoustic solitons and supersolitons in a magnetized plasma with nonthermal hot electrons and Boltzmann cool electrons

O. R. Rufai; R. Bharuthram; S. V. Singh; G. S. Lakhina

Arbitrary amplitude, ion acoustic solitons, and supersolitons are studied in a magnetized plasma with two distinct groups of electrons at different temperatures. The plasma consists of a cold ion fluid, cool Boltzmann electrons, and nonthermal energetic hot electrons. Using the Sagdeev pseudo-potential technique, the effect of nonthermal hot electrons on soliton structures with other plasma parameters is studied. Our numerical computation shows that negative potential ion-acoustic solitons and double layers can exist both in the subsonic and supersonic Mach number regimes, unlike the case of an unmagnetized plasma where they can only exist in the supersonic Mach number regime. For the first time, it is reported here that in addition to solitions and double layers, the ion-acoustic supersoliton solutions are also obtained for certain range of parameters in a magnetized three-component plasma model. The results show good agreement with Viking satellite observations of the solitary structures with density de...


Physics of Plasmas | 2013

Effect of ion temperature on ion-acoustic solitary waves in a magnetized plasma in presence of superthermal electrons

S. V. Singh; S. Devanandhan; G. S. Lakhina; R. Bharuthram

Obliquely propagating ion-acoustic soliatry waves are examined in a magnetized plasma composed of kappa distributed electrons and fluid ions with finite temperature. The Sagdeev potential approach is used to study the properties of finite amplitude solitary waves. Using a quasi-neutrality condition, it is possible to reduce the set of equations to a single equation (energy integral equation), which describes the evolution of ion-acoustic solitary waves in magnetized plasmas. The temperature of warm ions affects the speed, amplitude, width, and pulse duration of solitons. Both the critical and the upper Mach numbers are increased by an increase in the ion temperature. The ion-acoustic soliton amplitude increases with the increase in superthermality of electrons. For auroral plasma parameters, the model predicts the soliton speed, amplitude, width, and pulse duration, respectively, to be in the range of (28.7–31.8) km/s, (0.18–20.1) mV/m; (590–167) m, and (20.5–5.25) ms, which are in good agreement with Vik...

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R. Bharuthram

University of the Witwatersrand

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S. V. Singh

University of KwaZulu-Natal

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Frank Verheest

University of KwaZulu-Natal

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Bruce T. Tsurutani

California Institute of Technology

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R. V. Reddy

University of St Andrews

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R. V. Reddy

University of St Andrews

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S. Moolla

University of KwaZulu-Natal

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S. R. Pillay

University of KwaZulu-Natal

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