108 citations · 185 across the 14 of their papers we have counts for
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Sun-like stars produce superflares roughly once per century
Valeriy Vasilyev, Timo Reinhold, Alexander I. Shapiro +7
Stellar superflares are energetic outbursts of electromagnetic radiation, similar to solar flares but releasing more energy, up to erg on main sequence stars. It is unkno…
Combined Surface Flux Transport and Helioseismic Far-side Active Region Model (FARM)
Dan Yang, Stephan G. Heinemann, Robert H. Cameron +1
Maps of the magnetic field at the Sun's surface are commonly used as boundary conditions in space-weather modeling. However, continuous observations are only available from the Sun…
The rush to the poles and the role of magnetic buoyancy in the solar dynamo
Simon Cloutier, Robert H. Cameron, Laurent Gizon
The butterfly diagram of the solar cycle exhibits a poleward migration of the diffuse magnetic field resulting from the decay of trailing sunspots. It is one component of what is s…
Solar Inertial Modes
Laurent Gizon, Yuto Bekki, Aaron C. Birch +5
The Sun's global inertial modes are very sensitive to the solar differential rotation and to properties of the deep solar convection zone which are currently poorly constrained. Th…
A flux-independent increase in outflows prior to the emergence of active regions on the Sun
Hannah Schunker, William Roland-Batty, Aaron C. Birch +3
Emerging active regions are associated with convective flows on the spatial scale and lifetimes of supergranules. To understand how these flows are involved in the formation of act…
The mean solar butterfly diagram and poloidal field generation rate at the surface of the Sun
Simon Cloutier, Robert H. Cameron, Laurent Gizon
The difference between individual solar cycles in the magnetic butterfly diagram can mostly be ascribed to the stochasticity of the emergence process. We aim to obtain the expectat…
The Sun's differential rotation is controlled by high-latitude baroclinically unstable inertial modes
Yuto Bekki, Robert H. Cameron, Laurent Gizon
Rapidly rotating fluids have a rotation profile which depends only on the distance from the rotation axis, in accordance with the Taylor-Proudman theorem. Although the Sun was expe…