We present a large-scale combination of near-infrared (near-IR) interstellar polarization data from background starlight with polarized emission data at...
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PublicaciónComparing Submillimeter Polarized Emission with Near-infrared Polarization of Background Stars for the Vela C Molecular Cloud
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PublicaciónComparison of Magnetic Field Structures on Different Scales in and around the Filamentary Dark Cloud GF 9
New visible polarization data combined with existing IR and FIR polarization data are used to study how the magnetic field threading the filamentary molecular...
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PublicaciónComparison of Prestellar Core Elongations and Large-scale Molecular Cloud Structures in the Lupus I Region
Turbulence and magnetic fields are expected to be important for regulating molecular cloud formation and evolution. However, their effects on sub-parsec to 100...
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PublicaciónComparison of the thin flux tube approximation with 3D MHD simulations
Context: The structure and dynamics of small vertical photospheric magnetic flux concentrations has been often treated in the framework of an approximation...
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PublicaciónCompressive sensing for spectroscopy and polarimetry
We demonstrate, through numerical simulations with real data, the feasibility of using compressive sensing techniques for the acquisition of spectro...
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PublicaciónConcerning the Existence of a ``Turbulent'' Magnetic Field in the Quiet Sun
We report on the a5F-y5Fo multiplet of Ti I and its interest for the study of ``turbulent'' magnetic fields in the quiet solar photosphere. In particular, we...
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PublicaciónConstraining the magnetic vector in the quiet solar photosphere and the impact of instrumental degradation
Context. With the advent of next generation high resolution telescopes, our understanding of how the magnetic field is organized in the internetwork (IN)...
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PublicaciónConstraining the regular Galactic magnetic field with the 5-year WMAP polarization measurements at 22 GHz
Context. The knowledge of the regular (large scale) component of the Galactic magnetic field gives important information about the structure and dynamics of the...
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PublicaciónConstruction of coronal hole and active region magnetohydrostatic solutions in two dimensions: Force and energy balance
Coronal holes and active regions are typical magnetic structures found in the solar atmosphere. We propose several magnetohydrostatic equilibrium solutions that...