Magnetism and the Invisible Man: The mysteries of coronal cavities
Sarah Gibson

TL;DR
This paper explores the magnetic structures of coronal cavities in the solar corona, using multi-wavelength observations and new magnetic field measurements to understand their role in solar eruptions and space weather.
Contribution
It introduces novel multi-wavelength observational techniques and presents unprecedented coronal magnetic field measurements to elucidate the magnetic nature of coronal cavities.
Findings
Coronal cavities contain twisted magnetic fields.
Observations suggest cavities are precursors to CMEs.
Magnetic measurements support the link between cavities and eruptions.
Abstract
Magnetism defines the complex and dynamic solar corona. Twists and tangles in coronal magnetic fields build up energy and ultimately erupt, hurling plasma into interplanetary space. These coronal mass ejections (CMEs) are transient riders on the ever-outflowing solar wind, which itself possesses a three-dimensional morphology shaped by the global coronal magnetic field. Coronal magnetism is thus at the heart of any understanding of the origins of space weather at the Earth. However, we have historically been limited by the difficulty of directly measuring the magnetic fields of the corona, and have turned to observations of coronal plasma to trace out magnetic structure. This approach is complicated by the fact that plasma temperatures and densities vary among coronal magnetic structures, so that looking at any one wavelength of light only shows part of the picture. In fact, in some…
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