Observations of the relation between continuum intensity and magnetic field strength in sunspots have been made for nearly five decades. This work presents full...
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PublicaciónThe Temperature - Magnetic Field Relation in Observed and Simulated Sunspots
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PublicaciónThe Thermal and Magnetic Structure of Umbral Dots from the Inversion of High-Resolution Full Stokes Observations
This paper presents the analysis of high-resolution Stokes observations of eight different umbral dots in a sunspot. The spectra were recorded with the La Palma...
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PublicaciónThe Three-dimensional Interaction between Emerging Magnetic Flux and a Large-Scale Coronal Field: Reconnection, Current Sheets, and Jets
Using MHD numerical experiments in three dimensions, we study the emergence of a bipolar magnetic region from the solar interior into a model corona containing...
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PublicaciónThe Three-dimensional Structure of a Sunspot Magnetic Field
We report on observations of the three-dimensional structure of a sunspot magnetic field from the photosphere to the chromosphere, obtained with the new visible...
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PublicaciónThe usefulness of analytic response functions
Aims:We introduce analytical response functions and their main properties as an important diagnostic tool that help understand Stokes profile formation physics...
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PublicaciónThe Zeeman Effect in the G Band
We investigate the possibility of measuring magnetic field strength in G-band bright points through the analysis of Zeeman polarization in molecular CH lines...
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PublicaciónThe Zigzag Path of Buoyant Magnetic Tubes and the Generation of Vorticity along Their Periphery
We study the generation of vorticity in the magnetic boundary layer of buoyant magnetic tubes and its consequences for the trajectory of magnetic structures...
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PublicaciónTHEMIS observations of the Hanle effect in C_2 lines.
Analysis of the Hanle effect in solar molecular lines allows us to obtain empirical information on unresolved, tangled magnetic fields at subresolution scales...
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PublicaciónTHEMIS: the 2006-2012 perspective. and beyond
Imaging of the solar surface from ground based telescopes has achieved to be diffraction limited almost ten years ago, while diffraction-limited...