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On Magnetic Activity Band Overlap, Interaction, and the Formation of Complex Solar Active Regions
Scott W. McIntosh, Robert J. Leamon
Recent work has revealed an phenomenological picture of the how the 11-year sunspot cycle of Sun arises. The production and destruction of sunspots is a consequence of the la…
Deciphering Solar Magnetic Activity I: On The Relationship Between The Sunspot Cycle And The Evolution Of Small Magnetic Features
Scott W. McIntosh, Xin Wang, Robert J. Leamon +6
Sunspots are a canonical marker of the Sun's internal magnetic field which flips polarity every ~22-years. The principal variation of sunspots, an ~11-year variation in number, mod…
Identifying Potential Markers of the Sun's Giant Convective Scale
Scott W. McIntosh, Xin Wang, Robert J. Leamon +1
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 I…