Bhatia, T. S.; Panja, M.; Cameron, R. H.; Solanki, S. K.: 3D radiative MHD simulations of starspots: II. Large-scale structure. Astronomy and Astrophysics 693, p. A264 (2025)
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)
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)
Breu, C.; 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 530, pp. 2361 - 2377 (2024)
Cloutier, S.; Cameron, R. H.; Gizon, L.: The mean solar butterfly diagram and poloidal field generation rate at the surface of the Sun. Astronomy and Astrophysics 691, p. A9 (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)
First Light! The spectro-polarimeter of the world's largest solar telescope in Hawaii looks at the Sun for the first time. The instrument was developed in Germany.
Analyzing the high spatial resolution solar Ca II H and K emission data obtained by the SUNRISE mission and building a model of other stars more active than the Sun
Dr. Theodosios Chatzistergos receives award by the European Space Weather and Space Climate Association for his research findings on the historical activity of the Sun.
The Zdenĕk Švetska Senior Prize of the Solar Physics Division of the European Physical Society (EPS) recognizes Solanki’s pioneering contributions to solar research.