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Sergio Servidio

Researcher at University of Calabria

Publications -  188
Citations -  6503

Sergio Servidio is an academic researcher from University of Calabria. The author has contributed to research in topics: Turbulence & Solar wind. The author has an hindex of 43, co-authored 170 publications receiving 5664 citations. Previous affiliations of Sergio Servidio include Swedish Institute of Space Physics & University of Delaware.

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Magnetic reconnection in two-dimensional magnetohydrodynamic turbulence.

TL;DR: Systematic analysis of numerical simulations of two-dimensional magnetohydrodynamic turbulence reveals the presence of a large number of X-type neutral points where magnetic reconnection occurs, and examines the statistical properties of this ensemble of reconnection events that are spontaneously generated by turbulence.
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Statistical Analysis of Discontinuities in Solar Wind ACE Data and Comparison with Intermittent MHD Turbulence

TL;DR: In this article, a comparison between Advanced Composition Explorer (ACE) solar wind data and simulations of magnetohydrodynamic (MHD) turbulence shows a good agreement in the waiting-time analysis of magnetic field increments.
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Evidence for Inhomogeneous Heating in the Solar Wind

TL;DR: In this article, the authors used magnetohydrodynamic (MHD) simulations to probe the nature of turbulence heating and found that significant inhomogeneous heating occurs in the solar wind, connected with current sheets that are dynamically generated by MHD turbulence.
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Local kinetic effects in two-dimensional plasma turbulence.

TL;DR: Using direct numerical simulations of a hybrid Vlasov-Maxwell model, kinetic processes are investigated in a two-dimensional turbulent plasma, opening a new path on the study of kinetic processes such as heating, particle acceleration, and temperature anisotropy, commonly observed in astrophysical and laboratory plasmas.
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Intermittent MHD structures and classical discontinuities

TL;DR: In this article, the authors examined statistics of rapid spatial variations of the magnetic field in simulations of magnetohydrodynamic (MHD) turbulence, by analyzing intermittency properties, and by using classical methods for identifying discontinuities.