Search results for "Alfvén wave"

showing 2 items of 2 documents

Magnetic shuffling of coronal downdrafts

2017

Channelled fragmented downflows are ubiquitous in magnetized atmospheres, and have been recently addressed from an observation after a solar eruption. We study the possible back-effect of the magnetic field on the propagation of confined flows. We compare two 3D MHD simulations of dense supersonic plasma blobs downfalling along a coronal magnetic flux tube. In one, the blobs move strictly along the field lines; in the other, the initial velocity of the blobs is not perfectly aligned to the magnetic field and the field is weaker. The aligned blobs remain compact while flowing along the tube, with the generated shocks. The misaligned blobs are disrupted and merged by the chaotic shuffling of …

010504 meteorology & atmospheric sciencesField lineAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysicsSun:corona01 natural sciencesAlfvén waveSettore FIS/05 - Astronomia E AstrofisicaPhysics::Plasma Physics0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)0105 earth and related environmental sciencesPhysicsSolar flareAstronomy and AstrophysicsSun:activityPlasmaMagnetic fluxAccretion (astrophysics)Magnetic fieldAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary SciencePhysics::Space PhysicsMagnetohydrodynamicsmagnetohydrodynamics
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Chromospheric evaporation and phase mixing of Alfvén waves in coronal loops

2020

Phase mixing of Alfv\'en waves has been studied extensively as a possible coronal heating mechanism but without the full thermodynamic consequences considered self-consistently. It has been argued that in some cases, the thermodynamic feedback of the heating could substantially affect the transverse density gradient and even inhibit the phase mixing process. In this paper, we use MHD simulations with the appropriate thermodynamical terms included to quantify the evaporation following heating by phase mixing of Alfv\'en waves in a coronal loop and the effect of this evaporation on the transverse density profile. The numerical simulations were performed using the Lare2D code. We set up a 2D l…

Sun: generalatmosphere [Sun]Magnetohydrodynamics (MHD)corona [Sun]010504 meteorology & atmospheric sciencesDensity gradientThermodynamic equilibriumT-NDASEvaporationAstrophysics01 natural sciencesAlfvén wave0103 physical sciencesgeneral [Sun]QB AstronomyAstrophysics::Solar and Stellar AstrophysicsSun: oscillations010303 astronomy & astrophysicsQCQB0105 earth and related environmental sciencesPhysicsSun: coronaoscillations [Sun]Astronomy and AstrophysicsMechanicsCoronal loopDissipationTransverse planeQC PhysicsAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary SciencePhysics::Space PhysicsWavesMagnetohydrodynamicsBDCSun: atmosphere
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