activity
20052022
most citedMultifluid modeling of magnetosonic wave propagation in the solar chromosphere -- effects of impact ionization and radiative recombination

53 citations · 88 across the 10 of their papers we have counts for

collaborators

10 papers

physics.plasm-ph2022★ 29 cited

Generalized Fluid Models of the Braginskii Type

P. Hunana, T. Passot, E. Khomenko +7

Several generalizations of the well-known fluid model of Braginskii (Rev. of Plasma Phys., 1965) are considered. We use the Landau collisional operator and the moment method of Gra…

astro-ph.SR2016★ 53 cited

Multifluid modeling of magnetosonic wave propagation in the solar chromosphere -- effects of impact ionization and radiative recombination

Yana G. Maneva, Alejandro A. Laguna, Andrea Lani +1

In order to study chromospheric magnetosonic wave propagation including, for the first time, the effects of ion-neutral interactions in the partially ionized solar chromosphere, we…

physics.plasm-ph2015

Dissipation of parallel and oblique Alfvén-cyclotron waves: implications for minor ion heating in the solar wind

Y. G. Maneva, Adolfo F. Viñas, Pablo S. Moya +2

We perform 2.5D hybrid simulations with massless fluid electrons and kinetic particle-in-cell ions to study the temporal evolution of ion temperatures, temperature anisotropies and…

physics.plasm-ph2011

Nonlinear Terms of MHD Equations for Homogeneous Magnetized Shear Flow

Z. D. Dimitrov, Y. G. Maneva, T. S. Hristov +1

We have derived the full set of MHD equations for incompressible shear flow of a magnetized fluid and considered their solution in the wave-vector space. The linearized equations g…

astro-ph.GA2009★ 1 cited

Amplification of Slow Magnetosonic Waves by Shear Flow: Heating and Friction Mechanisms of Accretion Disks

T. M. Mishonov, Z. D. Dimitrov, Y. G. Maneva +1

Propagation of three dimensional magnetosonic waves is considered for a homogeneous shear flow of an incompressible fluid. The analytical solutions for all magnetohydrodynamic vari…

astro-ph2007★ 1 cited

Theory of heating of hot magnetized plasma by Alfven waves. Application for solar corona

T. M. Mishonov, M. V. Stoev, Y. G. Maneva

The heating of magnetized plasma by propagation of Alfven waves is calculated as a function of the magnetic field spectral density. The results can be applied to evaluate the heati…