Bibcode
                                    
                            Alsina Ballester, Ernest; Belluzzi, Luca; Trujillo Bueno, Javier
    Bibliographical reference
                                    Physical Review Letters
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                        8
            
                        2021
            
  Journal
                                    
                            Citations
                                    16
                            Refereed citations
                                    16
                            Description
                                    Twenty-five years ago, enigmatic linear polarization signals were discovered in the core of the sodium D1 line. The only explanation that could be found implied that the solar chromosphere is practically unmagnetized, in contradiction with other evidences. This opened a paradox that has challenged physicists for many years. Here we present its solution, demonstrating that these polarization signals can be properly explained in the presence of magnetic fields in the gauss range. This result opens a novel diagnostic window for exploring the elusive magnetism of the solar chromosphere.
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Magnetism, Polarization and Radiative Transfer in Astrophysics
            
    Magnetic fields pervade all astrophysical plasmas and govern most of the variability in the Universe at intermediate time scales. They are present in stars across the whole Hertzsprung-Russell diagram, in galaxies, and even perhaps in the intergalactic medium. Polarized light provides the most reliable source of information at our disposal for the
            
            Ernest
            
                        Alsina Ballester
            
  