Vortex Motions in the Solar Atmosphere: Definitions, Theory, Observations, and Modelling. [PDF]
Space Sci Rev, 2023 Tziotziou K +14 more
europepmc +1 more source
, 2019 | openaire: EC/H2020/665667/EU//EPFL FellowsEclipsing time variations have been observed for a wide range of binary systems, including post-common-envelope binaries. A frequently proposed explanation, apart from the possibility of having a third body, is
Völschow, Marcel +17 more
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Magneto-hydrodynamical nonlinear simulations of magnetically confined plasmas using smooth particle hydrodynamics (SPH) [PDF]
, 2019 The successful application of techniques inspired in Smoothed Particle Hydrodynamics (SPH) to magnetohydrodynamical (MHD) nonlinear simulations of magnetically confined plasmas requires the previous solution to a number of challenging issues that are ...
Reynolds Barredo, José Miguel +14 more
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Techno-Economic Evaluation of a Micro-Hydropower Plant for Rural Electrification in South Africa
, 2011 Published ArticleThis study investigated the techno-economic viability of micro-hydropower generation in the electrification of a rural area in KwaZulu-Natal, South Africa. The proposed scheme is composed of a squirrel cage induction machine running as a
Munda, J. L. +3 more
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Simulations of Gamma-Ray Emission from Magnetized Microquasar Jets
, 2018 In this work, we simulate $\gamma$-rays created in the hadronic jets of the compact object in binary stellar systems known as microquasars. We utilize as the main computational tool the 3D relativistic magnetohydrodynamical code PLUTO combined with in ...
Kosmas, Odysseas +3 more
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On the theory of ambipolar diffusion, with applications to astrophysical jets [PDF]
, 2018 1 online resource (x, 67 p.) : illustrations (chiefly colour)Includes abstract and appendices.Includes bibliographical references (p. 65-67).Numerically simulated magnetohydrodynamical jets are not at all morphologically similar to most of those which ...
Power, Michael Thomas
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Fluctuation Dynamos in Supersonic Turbulence at Pm ≳ 1
The Astrophysical JournalFluctuation dynamos provide a robust mechanism for amplifying weak seed magnetic fields in turbulent astrophysical plasmas. However, their behaviour in the highly compressible regimes characteristic of the interstellar medium remains incompletely ...
Ameya Uday Nagdeo +2 more
doaj +1 more source
On the effect of oscillatory phenomena on Stokes inversion results. [PDF]
Philos Trans A Math Phys Eng Sci, 2021 Keys PH, Steiner O, Vigeesh G.
europepmc +1 more source
Magnetic Rayleigh–Taylor Interchange Shapes Chiral Barbs in Solar Prominences
The Astrophysical Journal LettersSolar prominences are cool, dense condensations suspended in the million-degree corona by stressed magnetic fields. Because these fields store free magnetic energy before space-weather-relevant eruptions, prominence morphology provides a visible probe of
Hongyang Luo, Yuhong Fan
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Constrained Simulations of the Magnetic Field in the Local Supercluster and the Propagation of UHECR
, 2003 Magnetic fields (MF) in the Local Supercluster (LSC) of galaxies may have profound consequences for the propagation of Ultra High Energy Cosmic Rays (UHECR). Faraday rotations measurements provide some informations about MF in compact clusters.
Springel, V +3 more
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