Publikationen von Robert H. Cameron

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, S. 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, S. 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, S. 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, S. A32 (2024)

Bhatia, T. S.; Cameron, R. H.; Peter, H.; Solanki, S. K.: Small-scale dynamo in cool stars. III. Changes in the photospheres of F3V to M0V stars. Astronomy and Astrophysics 681, S. 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, S. 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, S. 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, S. A92 (2024)

Finley, A.; Brun, A.; Strugarek, A.; Cameron, R.: How well does surface magnetism represent deep Sun-like star dynamo action? ASTRONOMY & ASTROPHYSICS (2024)

Hofer, B.; Krivova, N. A.; Cameron, R.; Solanki, S. K.; Jiang, J.: The influence of small bipolar magnetic regions on basic solar quantities. Astronomy and Astrophysics 683, S. A48 (2024)

Hofer, B.; Krivova, N. A.; Cameron, R.; Solanki, S. K.; Jiang, J.: The influence of small bipolar magnetic regions on basic solar quantities. Astronomy and Astrophysics 683, S. A48 (2024)

Isik, E.; Solanki, S. K.; Cameron, R. H.; Shapiro, A. I.: Low-latitude Magnetic Flux Emergence on Rapidly Rotating Solar-type Stars. The Astrophysical Journal 976, S. 215 (2024)

Kostogryz, N. M.; Shapiro, A. I.; Witzke, V.; Cameron, R. H.; Gizon, L.; Krivova, N. A.; Ludwig, H.-G.; Maxted, P. F. L.; Seager, S.; Solanki, S. K. et al.; Valenti, J.: Magnetic origin of the discrepancy between stellar limb-darkening models and observations. Nature Astronomy (2024)

Kostogryz, N. M.; Shapiro, A. I.; Witzke, V.; Cameron, R. H.; Gizon, L.; Krivova, N. A.; Ludwig, H.-G.; Maxted, P. F. L.; Seager, S.; Solanki, S. K. et al.; Valenti, J.: Magnetic origin of the discrepancy between stellar limb-darkening models and observations. Nature Astronomy 8, S. 929 - 937 (2024)

Ondratschek, P. A.; Przybylski, D.; Smitha, H. N.; Cameron, R.; Solanki, S. K.; Leenaarts, J.: Mg II h&k spectra of an enhanced network region simulated with the MURaM-ChE code: Results using 1.5D synthesis. Astronomy and Astrophysics 692, S. A6 (2024)

Witzke, V.; Shapiro, A. I.; Kostogryz, N. M.; Mauviard, L.; Bhatia, T. S.; Cameron, R.; Gizon, L.; Przybylski, D.; Solanki, S. K.; Unruh, Y. C. et al.; Yue, L.: Testing MURaM and MPS-ATLAS against the quiet solar spectrum. Astronomy and Astrophysics 681, S. A81 (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, S. A101 (2023)

Breu, C.; Peter, H.; Cameron, R.; Solanki, S. K.: Swirls in the solar corona. Astronomy and Astrophysics 675, S. A94 (2023)

Breu, C.; Peter, H.; Cameron, R. H.; Solanki, S. K.; Przybylski, D.; Rempel, M.; Chitta, P.: A solar coronal loop in a box: Energy generation and heating (Corrigendum). Astronomy and Astrophysics 669 (2023)