We describe the presence of wave front dislocations in magnetohydrodynamic waves in stratified stellar atmospheres. Scalar dislocations such as edges and...
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PublicaciónDislocations in Magnetohydrodynamic Waves in a Stellar Atmosphere
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PublicaciónDiversity of dwarf galaxy IR-submm emission patterns: CLUES from hydrodynamical simulations
Context. The spectral energy distributions (SEDs) of low-mass low-metallicity (dwarf) galaxies are a challenging piece of the puzzle of galaxy formation in the...
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PublicaciónDynamics of an enhanced network region observed in Hα
This investigation is based on Hα observations of high spatial resolution. They stem from an enhanced network region near disk centre of the sun and consist of...
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PublicaciónEvaluating the Reliability of a Simple Method to Map the Magnetic Field Azimuth in the Solar Chromosphere
The Zeeman effect is of limited utility for probing the magnetism of the quiet solar chromosphere. The Hanle effect in some spectral lines is sensitive to such...
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PublicaciónEvidence of the multi-thermal nature of spicular downflows. Impact on solar atmospheric heating
Context. Spectroscopic observations of the emission lines formed in the solar transition region commonly show persistent downflows on the order of 10−15 km s −1...
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PublicaciónFast horizontal flows in a quiet sun MHD simulation and their spectroscopic signatures
Numerical simulations of solar surface convection have predicted the existence of supersonic horizontal flows in the photospheric granulation. Recently, the...
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PublicaciónFIRTEZ-dz. A forward and inverse solver of the polarized radiative transfer equation under Zeeman regime in geometrical scale
We present a numerical code that solves the forward and inverse problem of the polarized radiative transfer equation in geometrical scale under the Zeeman...
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PublicaciónFOREVER22: galaxy formation in protocluster regions
We present results from a new cosmological hydrodynamics simulation campaign of protocluster (PC) regions, FOREVER22: FORmation and EVolution of galaxies in...
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PublicaciónFormation and morphology of anomalous solar circular polarization
Context. The morphology of spectral line polarization is the most valuable observable to investigate the magnetic and dynamic solar atmosphere. However, in...