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Magnetic fields in protoplanetary discs: from MHD simulations to ALMA observations
(Oxford University Press, 2017-01)
Magnetic fields significantly influence the evolution of protoplanetary discs and the formation of planets, following the predictions of numerous magnetohydrodynamic (MHD) simulations. However, these predictions are yet ...
Study of fractal features of magnetized plasma through an MHD shell model
(American Institute of Physics, 2017)
A magnetohydrodynamic (MHD) shell model is used to describe the dissipative events which take place in magnetized plasmas. A scatter plot box-counting fractal dimension D is calculated for the time series of the magnetic ...
Study of the fractality of magnetized plasma using an MHD shell model driven by solar wind data
(American Institute of Physics Inc., 2018)
An MHD shell model is used to describe the dissipative events that take place in magnetized plasmas. We analyze the activity of the time series of the magnetic energy dissipation rate obtained in the MHD shell model, which ...
Simulation of multiple plasma eddies in 2DSimulación de torbellinos múltiples de plasma en 2D
(Universidad de Costa Rica, Centro de Investigación en Matemática Pura y Aplicada (CIMPA), 2020)
MAGNETOHYDRODYNAMIC SIMULATIONS OF RECONNECTION AND PARTICLE ACCELERATION: THREE-DIMENSIONAL EFFECTS
(IOP PUBLISHING LTD, 2011)
Magnetic fields can change their topology through a process known as magnetic reconnection. This process in not only important for understanding the origin and evolution of the large-scale magnetic field, but is seen as a ...
Energy transfer in Hall-MHD turbulence: Cascades, backscatter, and dynamo action
(Cambridge University Press, 2007-12)
Scale interactions in Hall magnetohydrodynamics (MHDs) are studied using both the mean field theory derivation of transport coefficients, and direct numerical simulations in three space dimensions. In the magnetically ...