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Magnetic connectivity through the Solar Partially Ionized Atmosphere (SPIA)

Date du début: 1 janv. 2012, Date de fin: 31 déc. 2016,

"The broad scientific objective of the SPIA proposal is to understand the magnetism of the Sun and stars and to establish connections between the magnetic activity in sub-surface layers and its manifestation in the outer atmosphere. The complex interactions in magnetized stellar plasmas are best studied via numerical simulations, a new powerful method of research that appeared in astrophysics with ...
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