170 citations · 1.3k across the 27 of their papers we have counts for
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3D Numerical Simulations of f-Mode Propagation Through Magnetic Flux Tubes
K. Daiffallah, T. Abdelatif, A. Bendib +2
Three-dimensional numerical simulations have been used to study the scattering of a surface-gravity wave packet by vertical magnetic flux tubes, with radii from 200 km to 3 Mm, emb…
Changes of the solar meridional velocity profile during cycle 23 explained by flows towards the activity belts
R. H. Cameron, M. Schüssler
The solar meridional flow is an important ingredient in Babcock-Leighton type models of the solar dynamo. Global variations of this flow have been suggested to explain the variatio…
Mesogranular structure in a hydrodynamical simulation
Ł. Matloch, R. Cameron, S. Shelyag +2
We analyse mesogranular flow patterns in a three-dimensional hydrodynamical simulation of solar surface convection in order to determine its characteristics. We calculate divergenc…
Expansion of magnetic flux concentrations: a comparison of Hinode SOT d ata and models
A. Pietarila, R. Cameron, S. K. Solanki
Context: The expansion of network magnetic fields with height is a fundamental property of flux tube models. A rapid expansion is required to form a magnetic canopy. Aims: We chara…