Bekki, Y.; Cameron, R. H.; Gizon, L.: The Sun's differential rotation is controlled by high-latitude baroclinically unstable inertial modes. Science Advances 10, p. eadk5643 (2024)
Bhatia, T. S.; Cameron, R.; Peter, H.; Solanki, S.: Small-scale dynamo in cool stars. III. Changes in the photospheres of F3V to M0V stars. Astronomy and Astrophysics 681, p. A32 (2024)
Breu, C. A.; Peter, H.; Solanki, S. K.; Cameron, R.; De Moortel, I.: Non-thermal broadening of coronal lines in a 3D MHD loop model. Monthly Notices of the Royal Astronomical Society (2024)
Finley, A. J.; Brun, A. S.; Strugarek, A.; Cameron, R.: How well does surface magnetism represent deep Sun-like star dynamo action? Astronomy and Astrophysics 684, p. A92 (2024)
Bekki, Y.; Cameron, R. H.: Three-dimensional non-kinematic simulation of the post-emergence evolution of bipolar magnetic regions and the Babcock-Leighton dynamo of the Sun. Astronomy and Astrophysics 670, p. A101 (2023)
Weisshaar, E.; Cameron, R. H.; Schüssler, M.: No evidence for synchronization of the solar cycle by a "clock". Astronomy and Astrophysics 671, p. A87 (2023)
Baumgartner, C.; Birch, A. C.; Schunker, H.; Cameron, R. H.; Gizon, L.: Impact of spatially correlated fluctuations in sunspots on metrics related to magnetic twist. Astronomy and Astrophysics 664, p. A183 (2022)
Bekki, Y.; Cameron, R. H.; Gizon, L.: Theory of solar oscillations in the inertial frequency range: Amplitudes of equatorial modes from a nonlinear rotating convection simulation. Astronomy and Astrophysics 666, p. A135 (2022)
Bekki, Y.; Cameron, R. H.; Gizon, L.: Theory of solar oscillations in the inertial frequency range: Linear modes of the convection zone. Astronomy and Astrophysics 662, p. A16 (2022)
Bhatia, T. S.; Cameron, R. H.; Solanki, S. K.; Peter, H.; Przybylski, D.; Witzke, V.; Shapiro, A.: Small-scale dynamo in cool stars. I. Changes in stratification and near-surface convection for main-sequence spectral types. Astronomy and Astrophysics 663, p. A166 (2022)
Biswas, A.; Karak, B. B.; Cameron, R.: Toroidal Flux Loss due to Flux Emergence Explains why Solar Cycles Rise Differently but Decay in a Similar Way. Physical Review Letters 129, p. 241102 (2022)
Gottschling, N.; Schunker, H.; Birch, A.; Cameron, R. H.; Gizon, L.: Testing solar surface flux transport models in the first days after active region emergence. Astronomy and Astrophysics 660, A6 (2022)
Gottschling, N.; Schunker, H.; Birch, A. C.; Cameron, R.; Gizon, L.: Testing solar surface flux transport models in the first days after active region emergence. Astronomy and Astrophysics 660, p. A6 (2022)
Application deadline 1 October 2024. PhD projects in planetary science, solar and stellar physics, solar magnetism, heliophysics, helioseismology, asteroseismology, ...
In analyzing solar observations from the 19th century, scientists are turning to amateur researchers for help. The project will allow to better understand the history of our star.
Astronomical teamwork: By combining data from Solar Orbiter and SDO, a group of researchers has unambiguously determined the magnetic field at the solar surface.
Application deadline 1 October 2023. PhD projects in planetary science, solar and stellar physics, solar magnetism, heliophysics, helioseismology, asteroseismology, ...
Philipp Löschl has co-authored an excellent publication on Solar Orbiter data which has been awarded best Solar Physics paper of 2022 (Gherardo Valori et al. 2022)