The three-dimensional Magnetic Structure of solar Filaments and Prominenses - MaSFiPro -327419

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Asensio Ramos
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173.370,60 €
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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

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Pino Alemán