CORDIS Project
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MAGHEAT investigates how energy is transported and released in the solar chromosphere. By analyzing observational data and developing new simulation methods, the project aims to identify the mechanisms responsible for heating in solar active regions.
The mechanisms that heat the solar chromosphere and corona, and that drive the solar dynamo, arguably remain some of the foremost questions in solar and stellar physics.
Here, we focus on the question of how energy is transported and released in the solar chromosphere.
During the past 20 years, numerical simulations of the chromosphere have been used, with increasing degree of sophistication, to validate various proposed heating mechanisms.
These studies have gradually come to recognise that the…
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