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What is Coronal Heating: Ion Cyclotron Resonance about?

This paper investigates the Coronal Heating Problem, focusing on Ion Cyclotron Resonance (ICR) as a key mechanism for the high temperatures observed in the solar corona. It discusses the role of plasma physics, wave phenomena, and turbulence in heating the corona, while also highlighting recent empirical data from the Parker Solar Probe that supports the ICR theory. The document concludes that a comprehensive understanding of coronal heating likely requires a combination of multiple heating mechanisms.

Author

Daphne Blumin

Language

EN