Context. Inversion techniques applied to the radiative transfer equation for polarized light are capable of inferring the physical parameters in the solar...
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PublicationCombining magneto-hydrostatic constraints with Stokes profiles inversions. II. Application to Hinode/SP observations
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PublicationCombining magnetohydrostatic constraints with Stokes profiles inversions. I. Role of boundary conditions
Context. Inversion codes for the polarized radiative transfer equation, when applied to spectropolarimetric observations (i.e., Stokes vector) in spectral lines...
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PublicationComparing Submillimeter Polarized Emission with Near-infrared Polarization of Background Stars for the Vela C Molecular Cloud
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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PublicationComparison 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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PublicationComparison 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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PublicationComparison 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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PublicationCompressive 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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PublicationConcerning 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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PublicationConstraining 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)...