NASA NTRS · 19980029717
Magnetic Helicity and the Solar Dynamo
Abstract
The objective of this investigation is to open a new window into the solar dynamo, convection, and magnetic reconnection through measurement of the helicity density of magnetic fields in the photosphere and tracing of large-scale patterns of magnetic helicity in the corona.
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Canfield, Richard C.. 1997-10-13. Magnetic Helicity and the Solar Dynamo. https://ntrs.nasa.gov/citations/19980029717
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