Identifying Potential Markers of the Sun’s Giant Convective Scale

Kavli Affiliate: Philip H. Scherrer | Summary:Line-of-sight magnetograms from the Helioseismic and Magnetic Imager (HMI) of the Solar Dynamics Observatory (SDO) are analyzed using a diagnostic known as the "Magnetic Range of Influence," or MRoI. The MRoI is a measure of the length over which a photospheric magnetogram is balanced and so its application gives […]


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