Abstract
The coronal portion of the solar atmosphere consists of a wide variety of structures which exhibit a similarly wide variety of dynamical processes and kinds of activity. The launch of the SMM presented an opportunity to study the low and intermediate corona from space with multiple instruments for protracted periods of time. This opportunity had been lacking for years, and it was enthusiastically awaited by those interested in coronal studies. The research performed during the SMM Workshop and reported here shows how successfully the SMM and collaborative observations have been used to advance our knowledge of the corona and how these observations have stimulated our theoretical understanding of why the corona is the way we observe it to be.
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Hildner, E. et al. (1989). Coronal Mass Ejections and Coronal Structures. In: Kundu, M.R., Woodgate, B., Schmahl, E.J. (eds) Energetic Phenomena on the Sun. Astrophysics and Space Science Library, vol 153. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-2331-7_6
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