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相关论文: Multi-fluid Approach to High-frequency Waves in Pl…

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Ideal MHD provides an accurate description of low-frequency Alfv\'en waves in fully ionized plasmas. However, higher frequency waves in many plasmas of the solar atmosphere cannot be correctly described by ideal MHD and a more accurate…

太阳与恒星天体物理 · 物理学 2016-12-07 David Martínez-Gómez , Roberto Soler , Jaume Terradas

Alfv\'en waves are a particular class of magnetohydrodynamic waves relevant in many astrophysical and laboratory plasmas. In partially ionized plasmas the dynamics of Alfv\'en waves is affected by the interaction between ionized and neutral…

太阳与恒星天体物理 · 物理学 2015-06-15 R. Soler , M. Carbonell , J. L. Ballester , J. Terradas

The multi-fluid modelling of high-frequency waves in partially ionized plasmas has shown that the behavior of magnetohydrodynamics waves in the linear regime is heavily influenced by the collisional interaction between the different species…

太阳与恒星天体物理 · 物理学 2018-04-04 David Martínez-Gómez , Roberto Soler , Jaume Terradas

Compressible disturbances propagate in a plasma in the form of magnetoacoustic waves driven by both gas pressure and magnetic forces. In partially ionized plasmas the dynamics of ionized and neutral species are coupled due to ion-neutral…

太阳与恒星天体物理 · 物理学 2015-06-17 Roberto Soler , Marc Carbonell , Jose Luis Ballester

Chromospheric and prominence plasmas contain neutral atoms, which may change the plasma dynamics through collision with ions. Most of the atoms are neutral hydrogen, but a significant amount of neutral helium may also be present in the…

太阳与恒星天体物理 · 物理学 2015-05-30 T. V. Zaqarashvili , M. L. Khodachenko , H. O. Rucker

Magneto-acoustic waves in partially ionized plasmas are damped due to elastic collisions between charged and neutral particles. Here, we use a linearized two-fluid model to describe the influence of this collisional interaction on the…

等离子体物理 · 物理学 2025-10-17 David Martínez-Gómez

We derive the dynamics of magnetohydrodynamic waves in two-fluid partially ionized plasmas and to compare the results with those obtained under single-fluid description. Two-fluid magnetohydrodynamic equations are used, where ion-electron…

太阳与恒星天体物理 · 物理学 2015-05-27 T. V. Zaqarashvili , M. K. Khodachenko , H. O. Rucker

A ray-theoretic phase space description of linear waves in a two-fluid (charges and neutrals) magnetized plasma is used to calculate analytic decay rates and mode transmission and conversion coefficients between fast and slow waves in two…

太阳与恒星天体物理 · 物理学 2023-04-12 Paul S Cally , M. M. Gomez-Miguez

Our study investigates the properties of Alfv\'en waves in partially ionised solar plasmas in the presence of steady, field-aligned, flows of charged and neutral particles. Our work aims to understand how such flows modify wave propagation…

太阳与恒星天体物理 · 物理学 2025-11-17 Nada F. Alshehri , Istvan Ballai , Viktor Fedun , Gary Verth

A nonlinear time dependent fluid simulation model is developed that describes the evolution of magnetohydrodynamic waves in the presence of collisional and charge exchange interactions of a partially ionized plasma. The partially ionized…

空间物理 · 物理学 2015-05-19 Dastgeer Shaikh , G. P. Zank

The large abundance of electrically neutral particles has a remarkable impact on the dynamics of many astrophysical plasmas. Here, we use a two-fluid model that includes charge-neutral elastic collisions and Hall's current to study the…

太阳与恒星天体物理 · 物理学 2025-02-20 David Martínez-Gómez

Observations show that waves are ubiquitous in the solar atmosphere and may play an important role for plasma heating. The study of waves in the solar corona is usually based on linear ideal magnetohydrodynamics (MHD) for a fully ionized…

太阳与恒星天体物理 · 物理学 2015-06-12 R. Soler , A. J. Diaz , J. L. Ballester , M. Goossens

The cut-off of the Alfven wave, caused by plasma collisions with neutrals in multi-component partially ionized plasmas, is discussed. Full multi-component theory is used, and similarities and differences regarding the classic…

等离子体物理 · 物理学 2015-06-18 J. Vranjes , M. Kono

This Chapter outlines the basic properties of waves in solar partially ionized plasmas. It provides a summary of the main sets of equations, from the single-fluid formalism, to the multi-fluid one, giving examples for purely hydrogen, and…

太阳与恒星天体物理 · 物理学 2024-09-19 Elena Khomenko , David Martínez-Gómez

A simple collisional three-component plasma model consisting of electrons, ions, and neutrals with arbitrary collision frequencies and dynamic time scales is considered. It is shown that the usual MHD-approach dealing with magnetic field…

太阳与恒星天体物理 · 物理学 2014-02-20 Anatoly K. Nekrasov

Ion-neutral collisions may lead to the damping of Alfven waves in chromospheric and prominence plasmas. Neutral helium atoms enhance the damping in certain temperature interval, where the ratio of neutral helium and neutral hydrogen atoms…

太阳与恒星天体物理 · 物理学 2015-06-12 T. V. Zaqarashvili , M. L. Khodachenko , R. Soler

We develop a two dimensional, self-consistent, compressible fluid model to study evolution of Alfvenic modes in partially ionized astrophysical and space plasmas. The partially ionized plasma consists mainly of electrons, ions and…

空间物理 · 物理学 2015-05-14 Dastgeer Shaikh

An experimental study of Ion Acoustic (IA) wave propagation is performed to investigate the effect of neutral density for argon plasma in an unmagnetized linear plasma device. The neutral density is varied by changing the neutral pressure,…

The effects of friction on the ion acoustic (IA) wave in fully and partially ionized plasmas are studied. In a quasi-neutral electron-ion plasma the friction between the two species cancels out exactly and the wave propagates without any…

等离子体物理 · 物理学 2015-05-18 J. Vranjes , S. Poedts

Here we study the nature and characteristics of waves propagating in partially ionised plasmas in the weakly ionised limit, typical for the lower part of the solar atmosphere. The framework in which the properties of waves are discussed…

太阳与恒星天体物理 · 物理学 2022-03-02 A. Alharbi , I. Ballai , V. Fedun , G. Verth
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