Three dimensional simulations of Hall magnetohydrodynamics [PDF]
Proceedings of the International Astronomical Union, 2010 AbstractTurbulent flows take place in a large variety of astrophysical objects, and often times are the source of dynamo generated magnetic fields. Much of the progress in our understanding of dynamo mechanisms, has been made within the theoretical framework of magnetohydrodynamics (MHD).
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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
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Vortex Motions in the Solar Atmosphere: Definitions, Theory, Observations, and Modelling. [PDF]
Space Sci Rev, 2023 Tziotziou K +14 more
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Global Magnetohydrodynamical Simulations of Accretion Tori
The Astrophysical Journal, 2000 Global time-dependent simulations provide a means to investigate time-dependent dynamic evolution in accretion disks. This paper seeks to extend previous local simulations by beginning a systematic effort to develop fully global three-dimensional simulations.
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Learning effective physical laws for generating cosmological hydrodynamics with Lagrangian deep learning. [PDF]
Proc Natl Acad Sci U S A, 2021 Dai B, Seljak U.
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The Life and Times of Star-forming Cores: An Analysis of Dense Gas in the STARFORGE Simulations
The Astrophysical JournalDense gas in molecular clouds is an important signature of ongoing and future star formation. We identify and track dense cores in the starforge simulations, following the core evolution from birth through dispersal by stellar feedback for typical Milky ...
Stella S. R. Offner +2 more
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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.
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The Interaction of a Supernova Remnant with Background Interstellar Turbulence
The Astrophysical Journal Supplement SeriesSupernova explosions are among the most energetic events in the Universe. After the explosion, the material ejected by the supernova expands throughout the interstellar medium (ISM), forming what is called a supernova remnant (SNR). The shocks associated
Giuseppe Prete +4 more
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Cosmic-Ray Acceleration of Galactic Outflows in Multiphase Gas
The Astrophysical JournalWe investigate the dynamical interaction between cosmic rays (CRs) and the multiphase interstellar medium (ISM) using numerical magnetohydrodynamic (MHD) simulations with a two-moment CR solver and TIGRESS simulations of star-forming galactic disks.
Lucia Armillotta +3 more
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Multimessenger Binary Mergers Containing Neutron Stars: Gravitational Waves, Jets, and <i>γ</i>-Ray Bursts. [PDF]
Front Astron Space Sci, 2021 Ruiz M, Shapiro SL, Tsokaros A.
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