3D Magnetic Reconnection at a Coronal Null Point
presentationposted on 18.04.2018 by Shane Maloney, Adian O'Flannagain, Peter Gallagher, Philippa Browning, Jose Refojo
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An overview of a series of obversion combining, GOES and RHESSI X-rays, Nancay RadioHeliograph imaging and spectra, and SDO AIA EUV images and HMI magnetograms. These observations are interpreted as magnetic reconnection and 3D coronal null point and compared to numerical simulations and show good agreement.