J
Javier Trujillo Bueno
Researcher at Spanish National Research Council
Publications - 83
Citations - 2147
Javier Trujillo Bueno is an academic researcher from Spanish National Research Council. The author has contributed to research in topics: Polarization (waves) & Scattering. The author has an hindex of 26, co-authored 83 publications receiving 1983 citations. Previous affiliations of Javier Trujillo Bueno include University of La Laguna.
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Spectropolarimetric Investigation of the Propagation of Magnetoacoustic Waves and Shock Formation in Sunspot Atmospheres
TL;DR: In this paper, the authors derived the Stokes inversion of temporal series of spectropolarimetric observations and derived the time delay between the photospheric and chromospheric signals, which happens to have a strong dependence on frequency.
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The Iron Line Formation Problem in Three-dimensional Hydrodynamic Models of Solar-like Photospheres
TL;DR: In this paper, a detailed theoretical investigation of the iron line formation NLTE problem in a three-dimensional model of the solar photosphere, which was obtained from a very recent radiation hydrodynamics simulation of solar surface convection, was presented.
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Iterative Methods for the Non-LTE Transfer of Polarized Radiation: Resonance Line Polarization in One-dimensional Atmospheres
TL;DR: In this article, the authors generalize the operator splitting methods that were originally developed for solving unpolarized transfer problems to non-LTE polarization transfer problems and show that these methods lead to the self-consistent solution independently of the chosen initialization.
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PORTA: A three-dimensional multilevel radiative transfer code for modeling the intensity and polarization of spectral lines with massively parallel computers
TL;DR: In this paper, the authors present PORTA, an efficient multilevel radiative transfer code for the simulation of the spectral line polarization caused by scattering processes and the Hanle and Zeeman effects in 3D models of stellar atmospheres.
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The magnetic field configuration of a solar prominence inferred from spectropolarimetric observations in the He I 10830 A triplet
TL;DR: In this article, the magnetic field vector configuration along a quiescent solar prominence was determined by interpreting spectropolarimetric measurements in the He I 1083.0 nm triplet obtained with the Tenerife Infrared Polarimeter installed at the German Vacuum Tower Telescope of the Observatorio del Teide.