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2.2.1 How do CMEs contribute to the global evolution of magnetic flux in the heliosphere?
27 May, 2015 • Yannis Zouganelis
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1.2.1.6 Resolve the geometry of fine elemental loop strands
27 May, 2015 • Yannis Zouganelis
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1.2.1.7 Detect and characterise waves in closed and open structures
27 May, 2015 • Yannis Zouganelis
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1.2.1.5 Determine whether coronal heating is spatially localized or uniform, and time steady or transient or impulsive for a wide range of magnetic loops with different spatial scales.
27 May, 2015 • Yannis Zouganelis
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1.2.1.3 Contribution of flare-like events on all scales
27 May, 2015 • Yannis Zouganelis