Synthetic observations produced from radiative magnetohydrodynamic simulations have predicted that higher polarization fractions in the quiet solar photosphere...
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PublicaciónExploring Magnetic Loops and Serpentine Fields in the Quiet Sun with the GRIS-IFU
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PublicaciónHinode Observations of Horizontal Quiet Sun Magnetic Flux and the ``Hidden Turbulent Magnetic Flux''
We present observations of magnetic fields of the very quiet Sun near disk center using the Spectro-Polarimeter of the Solar Optical Telescope aboard the Hinode...
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PublicaciónInfluence of unresolved optically-thin irregularities on quiet Sun magnetic field determinations.
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PublicaciónLong Characteristics versus Short Characteristics in 3D Radiative Transfer Simulations of Polarized Radiation
We compare maps of scattering polarization signals obtained from three-dimensional (3D) radiation transfer calculations in a magnetoconvection model of the...
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PublicaciónSolar-cycle and Latitude Variations in the Internetwork Magnetism
The importance of the quiet-Sun magnetism is that it is always there to a greater or lesser extent, being a constant provider of energy, independently of the...
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PublicaciónThe Impact of Limited Time Resolution on the Forward-scattering Polarization in the Solar Sr I 4607 Å Line
Theoretical investigations predicted that high spatiotemporal resolution observations in the Sr I 4607 Å line must show a conspicuous scattering polarization...
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PublicaciónThe Impact of Limited Time Resolution on the Forward-scattering Polarization in the Solar Sr I 4607 Å Line
Theoretical investigations predicted that high spatiotemporal resolution observations in the Sr I 4607 Å line must show a conspicuous scattering polarization...
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PublicaciónThe Magnetic Sensitivity of the (250-278 nm) Fe II Polarization Spectrum
This paper presents a theoretical investigation of the polarization and magnetic sensitivity of the near-ultraviolet (near-UV) solar spectral lines of Fe II...
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PublicaciónThe Sun at high resolution: first results from the Sunrise mission
The Sunrise balloon-borne solar observatory consists of a 1m aperture Gregory telescope, a UV filter imager, an imaging vector polarimeter, an image...