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)
The Planetary Plasma Environments group (PPE) has a strong heritage in the exploration of planetary magnetospheres and space plasma interactions throughout the solar system. It has contributed instruments to several past missions that flew-by or orbited Jupiter (Galileo, Cassini, Ulysses). The PPE participates in the JUICE mission by contributing hardware and scientific expertise to the Particle Environment Package (PEP).
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.
Images from ESA’s Solar Orbiter offer the best look yet at a source region of the solar wind - and challenge our view of the continuous particle stream from the Sun.