CORDIS Project
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This project aims to solve the coronal heating problem in solar physics by using advanced observational techniques. It will utilize the Atacama Large Millimeter/submillimeter Array to study energy transport and dissipation in the Sun's atmosphere, focusing on the chromosphere.
How are the outer layers of the Sun heated to temperatures in excess of a million kelvin? A large number of heating mechanisms have been proposed to explain this so-called coronal heating problem, one of the fundamental questions in contemporary solar physics.
It is clear that the required energy is transported from the solar interior through the chromosphere into the outer layers but it remains open by which physical mechanisms and how the provided energy is eventually dissipated.
The key to s…
UNIVERSITETET I OSLO
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