Abstract
The research into the physics of the solar corona by using the solar-A satellite is reviewed. Discussions are given on coronal heating mechanisms, the physics of coronal loops, coronal holes, coronal mass ejections, and the observational approach to these topics to be taken by the Solar-A satellite.
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© 1991 Springer-Verlag
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Sakurai, T. (1991). Magnetic structures in the corona. In: Uchida, Y., Canfield, R.C., Watanabe, T., Hiei, E. (eds) Flare Physics in Solar Activity Maximum 22. Lecture Notes in Physics, vol 387. Springer, Berlin, Heidelberg. https://doi.org/10.1007/BFb0032646
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DOI: https://doi.org/10.1007/BFb0032646
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