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Solar Physics | 1991

Discrete Alfvén waves in solar loop prominences

Carlos A. de Azevedo; Altair Souza de Assis; H. Shigueoka; Paulo Hiroshi Sakanaka

It is shown that a discrete Alfvén wave can explain the natural oscillations of solar loop prominences by considering the existence of a current flow. Discrete Alfvén waves are a new class of Alfvén waves which is described by the inclusion of the finite ion cyclotron frequency (ω/ωcl≠0) and/or the equilibrium plasma current. In this paper we consider only the effect of the current since in solar prominences (ω/ωcl≈0). We have modeled the solar prominences as a cylindrical plasma, surrounded by vacuum (corona), with L ≫ a where L and a are the plasma column, length, and radius, respectively. We have calculated the spectrum of the discrete Alfvén waves as function of the magnitude and shape of the plasma current.


Physics of fluids. B, Plasma physics | 1989

Magnetosonic and kinetic Alfvén current drive analysis

K. H. Tsui; Altair Souza de Assis

Quasilinear equations are used together with the energy conservation equation to assess the merits of magnetosonic and kinetic Alfven current drive. It is found that the Alfven mode has a higher gain in terms of efficiency and current than the magnetosonic mode.


Archive | 1991

Coronal Loop Heating by the Fast Surface Wave

Altair Souza de Assis; K. H. Tsui

Although coronal plasmas are considered to be collisional, it is well known that particle collisions do not provide effective energy dissipation. It is shown that the wave-particle resonant interactions can dissipate energy fast enough to sustain the coronal temperature.


Space Science Reviews | 2003

Wave-Particle-Electric Field Synergetic Auroral Electron Acceleration

Altair Souza de Assis

We discuss afresh the problem of the auroral electron acceleration based on the controversy reports of Bryant, D. A. et al.: 1992, Phys. Rev. Lett. 68, 37, and Borovsky, J.: 1992, Phys. Rev. Lett. 69, 1054, related to which mechanism is more tenable to accelerate auroral electrons: dc electric field generated somehow in aurora or wave-particle interaction due to auroral wave turbulence? Here, we show that both mechanisms are important, and what is most likely to happen in aurora is that the turbulence and the dc electric field structure will assist each other so as to synergetically accelerate those electrons.


Geophysical Research Letters | 1983

A theory of long period magnetic pulsations, 3. Local field line oscillations

Akira Hasegawa; K. H. Tsui; Altair Souza de Assis


Brazilian Journal of Physics | 1993

Electron temperature effect on plasma potential for different resonant volumes in LISA machine

Altair Souza de Assis; H.R.T Silva; Cândido da Cunha Rapozo; A Serbeto


Revista EIA/ English version | 2017

Undesired Splash Over on Equipments Using Inductive Sensors for Monitoring Automotive Vehicles’ Controlled Speed

Silvio Monteiro; Maurício Réche; Altair Souza de Assis


Journal of Electromagnetic Analysis and Applications | 2015

Convective Schrödinger Equation: Insights on the Potential Energy's Role to Wave Particle Decay

Altair Souza de Assis; Héctor Torres-Silva; Göran Marklund


Journal of Atmospheric and Solar-Terrestrial Physics | 2005

Auroral electron acceleration induced by Cherenkov damped waves

Altair Souza de Assis


Archive | 2000

Inverted - V Events and LWD Spectral Gap Problem Revised

Altair Souza de Assis; Manfred P. Leubner; Paulo Hiroshi Sakanaka

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Carlos A. de Azevedo

Rio de Janeiro State University

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A. G. Elfimov

University of São Paulo

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C. A. de Azevedo

Rio de Janeiro State University

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H. Shigueoka

Federal Fluminense University

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K. H. Tsui

Federal Fluminense University

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V. S. Tsypin

Rio de Janeiro State University

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Abraham C.-L. Chian

National Institute for Space Research

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Padma Kant Shukla

University of KwaZulu-Natal

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Lennart Stenflo

Chinese Academy of Sciences

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