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Solar Coronal Magnetic Fields: Quantitative Measurements at Radio Wavelengths

Published onMay 31, 2019
Solar Coronal Magnetic Fields: Quantitative Measurements at Radio Wavelengths
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Abstract

Quantitative measurements of coronal and chromospheric magnetic field is currently in its infancy. We describe a foundation of such observations, which is a key input for MHD numerical models of the solar atmosphere and eruptive processes, and a key link between lower layers of the solar atmosphere and the heliosphere.

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