Search Results - "Díaz Baso, C. J."
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ACTIVE REGION FILAMENTS MIGHT HARBOR WEAK MAGNETIC FIELDS
Published in The Astrophysical journal (01-05-2016)“…ABSTRACT Recent spectropolarimetric observations of active region filaments have revealed polarization profiles with signatures typical of the strong field…”
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Radiative losses in the chromosphere during a C-class flare
Published 25-08-2022“…A&A 665, A50 (2022) Solar flares release an enormous amount of energy into the corona. A substantial fraction of this energy is transported to the lower…”
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3
Center-to-limb variation of spectral lines and continua observed with SST/CRISP and SST/CHROMIS
Published 19-03-2023“…A&A 671, A130 (2023) Observations of center-to-limb variations (CLV) of spectral lines and continua provide a good test for the accuracy of models of solar and…”
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Spatio-temporal analysis of chromospheric heating in a plage region
Published 30-03-2022“…A&A 664, A8 (2022) Our knowledge of the heating mechanisms that are at work in the chromosphere of plage regions remains highly unconstrained from…”
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An observationally-constrained model of strong magnetic reconnection in the solar chromosphere. Atmospheric stratification and estimates of heating rates
Published 09-02-2021“…A&A 647, A188 (2021) The evolution of the photospheric magnetic field plays a key role in the energy transport into the chromosphere and the corona. In active…”
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6
Bayesian Stokes inversion with Normalizing flows
Published 19-12-2021“…A&A 659, A165 (2022) Stokes inversion techniques are very powerful methods for obtaining information on the thermodynamic and magnetic properties of solar and…”
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Solar image denoising with convolutional neural networks
Published 07-08-2019“…A&A 629, A99 (2019) The topology and dynamics of the solar chromosphere are greatly affected by the presence of magnetic fields. The magnetic field can be…”
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Inference of the chromospheric magnetic field configuration of solar plage using the Ca II 8542 {\AA} line
Published 16-10-2020“…A&A 644, A43 (2020) It has so far proven impossible to reproduce all aspects of the solar plage chromosphere in quasi-realistic numerical models. The magnetic…”
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Active region chromospheric magnetic fields
Published 07-09-2021“…A&A 662, A88 (2022) Context. A proper estimate of the chromospheric magnetic fields is believed to improve modelling of both active region and coronal mass…”
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Spectropolarimetric analysis of an active region filament. II. Evidence of the limitations of a single component model
Published 24-04-2019“…A&A 625, A129 (2019) Our aim is to demonstrate the limitations of using a single component model to study the magnetic field of an active region filament. For…”
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Spectropolarimetric analysis of an active region filament. I. Magnetic and dynamical properties from single component inversions
Published 21-04-2019“…A&A 625, A128 (2019) The determination of the magnetic filed vector in solar filaments is possible by interpreting the Hanle and Zeeman effects in suitable…”
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Three-dimensional magnetic field structure of a flux emerging region in the solar atmosphere
Published 29-10-2019“…A&A 632, A112 (2019) We analyze high-resolution spectropolarimetric observations of a flux emerging region (FER) in order to understand its magnetic and…”
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13
Active region filaments might harbor weak magnetic fields
Published 17-03-2016“…Recent spectropolarimetric observations of active region filaments have revealed polarization profiles with signatures typical of the strong field Zeeman…”
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14
Spectral resolution effects on the information content in solar spectra
Published 20-09-2024“…When interpreting spectropolarimetric observations of the solar atmosphere, wavelength variations of the emergent intensity and polarization translate into…”
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15
Properties of sunspot light bridges on a geometric height scale
Published 14-08-2024“…Investigating light bridges (LBs) helps us comprehend key aspects of sunspots. However, few studies have analyzed the properties of LBs in terms of the…”
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Enhancing SDO/HMI images using deep learning
Published 30-01-2018“…A&A 614, A5 (2018) The Helioseismic and Magnetic Imager (HMI) provides continuum images and magnetograms with a cadence better than one per minute. It has been…”
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Designing wavelength sampling for Fabry-P\'erot observations. Information-based spectral sampling
Published 24-03-2023“…A&A 673, A35 (2023) Fabry-P\'erot interferometers (FPIs) have become very popular in solar observations because they offer a balance between cadence, spatial…”
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Non-LTE inversions of a confined X2.2 flare: I. Vector magnetic field in the photosphere and chromosphere
Published 03-09-2020“…A&A 645, A1 (2021) Obtaining the magnetic field vector accurately in the solar atmosphere is essential for studying changes in field topology during flares and…”
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Exploring spectropolarimetric inversions using neural fields. Solar chromospheric magnetic field under the weak-field approximation
Published 08-09-2024“…Full-Stokes polarimetric datasets, originating from slit-spectrograph or narrow-band filtergrams, are routinely acquired nowadays. The data rate is increasing…”
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Diagnostic potential of the Ca II 8542A line for solar filaments
Published 18-02-2019“…A&A 623, A178 (2019) In this study we explore the diagnostic potential of the chromospheric Ca II line at 8542A for studying the magnetic and dynamic…”
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