The sun seen with the atacama large mm and sub-mm array (ALMA) - first results
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Observations of the solar magnetic field are largely confined to the radiation emitted from the photosphere, the thin layer of the solar atmosphere which we cal
This volume provides an overview of our current understanding of the physics related to: coronal structures and coronal heating; large-scale coronal shock waves
The bulk of the contributions address optical, radio, extreme ultraviolet, and soft X-ray observations, their implications for theory, and their contribution to