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Exploring spectropolarimetric inversions using neural fields. Solar chromospheric magnetic field under the weak-field approximation
C. J. Díaz Baso, A. Asensio Ramos, J. de la Cruz Rodríguez +2
Full-Stokes polarimetric datasets, originating from slit-spectrograph or narrow-band filtergrams, are routinely acquired nowadays. The data rate is increasing with the advent of bi…
Stratification of physical parameters in a C-class solar flare using multi-line observations
Rahul Yadav, C. J. D. Baso, J. de la Cruz Rodr'iguez +2
We present high-resolution and multi-line observations of a C2-class solar flare, occurred in NOAA AR 12740 on May 6, 2019. The rise, peak and decay phases of the flare were record…
Non-LTE inversions of a confined X2.2 flare: I. Vector magnetic field in the photosphere and chromosphere
G. J. M. Vissers, S. Danilovic, J. de la Cruz Rodriguez +7
Obtaining the magnetic field vector accurately in the solar atmosphere is essential for studying changes in field topology during flares and to reliably model space weather. We tac…
Inference of the chromospheric magnetic field configuration of solar plage using the Ca II 8542 Å line
A. G. M. Pietrow, D. Kiselman, J. de la Cruz Rodríguez +3
It has so far proven impossible to reproduce all aspects of the solar plage chromosphere in quasi-realistic numerical models. The magnetic field configuration in the lower atmosphe…
Three-dimensional magnetic field structure of a flux emerging region in the solar atmosphere
Rahul Yadav, J. de la Cruz Rodríguez, C. J. Díaz Baso +4
We analyze high-resolution spectropolarimetric observations of a flux emerging region (FER) in order to understand its magnetic and kinematic structure. Our spectropolarimetric obs…