Daiffallah, K.; Abdelatif, T.; Bendib, A.; Cameron, R.; Gizon, L.: 3D Numerical Simulations of f-Mode Propagation Through Magnetic Flux Tubes. Solar Physics 268, pp. 309 - 320 (2011)
Innes, D. E.; Cameron, R. H.; Solanki, S. K.: EUV Jets, Type III Radio Bursts and Sunspot Waves Investigated Using SDO/AIA Observations. Astronomy and Astrophysics 531, L13 (2011)
Jiang, J.; Cameron, R. H.; Schmitt, D.; Schüssler, M.: The solar magnetic field since 1700 I. Characteristics of sunspot group emergence and reconstruction of the butterfly diagram. Astronomy and Astrophysics 528, A82 (2011)
Jiang, J.; Cameron, R. H.; Schmitt, D.; Schüssler, M.: The solar magnetic field since 1700 II. Physical reconstruction of total, polar and open flux. Astronomy and Astrophysics 528, A83 (2011)
Röhrbein, D.; Cameron, R.; Schüssler, M.: Is there a non-monotonic relation between photospheric brightness and magnetic field strength? Astronomy and Astrophysics 532, A140 (2011)
Schunker, H.; Cameron, R. H.; Gizon, L.; Moradi, H.: Constructing and Characterising Solar Structure Models for Computational Helioseismology. Solar Physics 271 (1-2), pp. 1 - 26 (2011)
Cameron, R. H.; Jiang, J.; Schmitt, D.; Schüssler, M.: Surface flux transport modeling for solar cycles 15-21: effects of cycle-dependent tilt angles of sunspot groups. Astrophysical Journal 719, pp. 264 - 270 (2010)
Cameron, R. H.; Schüssler, M.: Changes of the solar meridional velocity profile during cycle 23 explained by flows towards the activity belts. Astrophysical Journal 720, pp. 1030 - 1032 (2010)
Gizon, L.; Schunker, H.; Baldner, C. S.; Basu, S.; Birch, A. C.; Bogart, R. S.; Braun, D. C.; Cameron, R.; Duvall Jr., T. L.; Hanasoge, S. M.et al.; Jackiewicz, J.; Roth, M.; Stahn, T.; Thompson, M. J.; Zharkov, S.: Erratum to: Helioseismology of Sunspots: A Case Study of NOAA Region 9787. Space Science Reviews 156, pp. 257 - 258 (2010)
Jiang, J.; Işık, E.; Cameron, R. H.; Schmitt, D.; Schüssler, M.: The effect of activity-related meridional flow modulation on the strength of the solar polar magnetic field. Astrophysical Journal 717, pp. 597 - 602 (2010)
Moradi, H.; Baldner, C.; Birch, A. C.; Braun, D. C.; Cameron, R. H.; Duvall Jr., T. L.; Gizon, L.; Haber, D.; Hanasoge, S. M.; Hindman, B. W.et al.; Jackiewicz, J.; Khomenko, E.; Komm, R.; Rajaguru, P.; Rempel, M.; Roth, M.; Schlichenmaier, R.; Schunker, H.; Spruit, H. C.; Strassmeier, K. G.; Thompson, M. J.; Zharkov, S.: Modeling the subsurface structure of sunspots. Solar Physics 267, pp. 1 - 62 (2010)
Pietarila, A.; Cameron, R.; Solanki, S. K.: Expansion of Magnetic Flux Concentrations: A Comparison of Hinode SOT Data md Models. Astronomy and Astrophysics 518, A50 (2010)
Schrinner, M.; Schmitt, D.; Cameron, R.; Hoyng, P.: Saturation and time dependence of geodynamo models. Geophysical Journal International 182, pp. 675 - 681 (2010)
Birch, A. C.; Braun, D. C.; Hanasoge, S.; Cameron, R.: Surface-focused seismic holography of sunspots: II. Expectations from numerical simulations using sound-speed perturbations. Solar Physics 254, pp. 17 - 27 (2009)
First Light for Sunrise III: the first tests with real sunlight were successful. The balloon-borne solar observatory should be ready for launch at the end of May.
First icy cold, then midnight sun: at the Arctic Circle, the team will prepare the next flight of the balloon-borne solar observatory - and hopes for solar fireworks.
Astronomical teamwork: By combining data from Solar Orbiter and SDO, a group of researchers has unambiguously determined the magnetic field at the solar surface.
The magnetic field in the solar atmosphere exceeds the geomagnetic field strength by four orders of magnitude. It greatly influences the processes of energy transport within the solar atmosphere, and dominates the morphology of the solar chromosphere and corona. Kinetic energy from convective motions in the Sun can be efficiently stored in magnetic fields and subsequently released - to heat the solar corona to several million degrees or to blast off coronal mass ejections.