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

In force date
Call year
2014
Investigator
Andrés
Asensio Ramos
Financial institution
Financing program
Financing subprogram
Amount granted to the IAC Consortium
173.370,60 €
Related projects
Project Image
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

Tanausú del
Pino Alemán