Cameron, R.; Gizon, L.; Daiffallah, K.: SLiM: a code for the simulation of wave propagation through an inhomogeneous, magnetised solar atmosphere. Astron. Nachrichten 328, pp. 313 - 318 (2007)
Cameron, R.; Schüssler, M.; Vögler, A.: The Sun - a ball of electrically well-conducting gas. inSIDE - Innovatives Supercomputing 2 (1), pp. 4 - 5 (2004)
Kigure, H.; Uchida, Y.; Nakamura, M.; Hirose, S.; Cameron, R.: Distribution of Faraday rotation measure in jets from active galactic nuclei. I. Predictions from our sweeping magnetic twist model. Astrophysical Journal 600 (1), pp. 88 - 95 (2004)
Kigure, H.; Uchida, Y.; Nakamura, M.; Hirose, S.; Cameron, R.: Distribution of Faraday rotation measure in jets from Active Galactic Nuclei. II. Prediction from our sweeping magnetic twist model for the wiggled parts of active galactic nucleus jets and tails. Astrophysical Journal 608, pp. 119 - 135 (2004)
Cameron, R.; Vögler, A.; Schüssler, M.: Simulation of solar magneto-convection. In: High Performance Computing in Science and Engineering: Transactions of the Second Joint HLRB and KONWIHR Result and Reviewing Workshop, pp. 431 - 442 (Eds. Wagner, S.; Hanke, W.; Bode, A.; Durst, F.). Springer, Berlin (2004)
Asvestari, E.; Usoskin, I. G.; Cameron, R. H.; Krivova, N. A.: Semi-empirical Long-term Reconstruction of the Heliospheric Parameters: Validation by Cosmogenic Radionuclide Records. Publications of the astronomical society of the pacific 504, pp. 269 - 272 (2016)
Schunker, H.; Cameron, R.; Gizon, L.: Convectively stabilised background solar models for local helioseismology. In: Proceedings of the HELAS Workshop NA3-4, ``The Acoustic Solar Cycle'', University of Birmingham, 6-8 January 2009 (Eds. Elsworth, Y. P.; Thompson, M. J.). The University of Sheffield (2010)
Pietarila, A.; Cameron, R.; Solanki, S. K.: Expansion of Magnetic Flux Concentrations with Height: A Comparison of Hinode SOT Data and MHD Simulations. In: The Second Hinode Science Meeting: Beyond Discovery - Torward Understanding, 91 (Eds. Lites, B.; Cheung, M.; Magara, T.; Mariska, J.; Reeves, K.). (2009)
Gizon, L.; Cameron, R.; Jackiewicz, J.; Roth, M.; Schunker, H.; Stahn, T.: Helioseismology at MPS. In: Modern Solar Facilities - Advanced Solar Science, pp. 89 - 102 (Eds. Kneer, F.; Puschmann, K. G.; Wittmann, A. D.). Universitätsverlag Göttingen, Göttingen, Germany (2007)
Cameron, R.; Gizon, L.: Three-dimensional numerical simulation of wave propagation through a model sunspot. In: Proceedings of SOHO 18 / GONG 2006 / HELAS I - Beyond the spherical Sun, 7-11 August 2006, Sheffield, UK (Ed. Fletcher, K.). ESA Publ. Div., Noordwijk, The Netherlands (2006)
Cameron, R.; Vögler, A.; Schüssler, M.; Zakharov, V.: Simulations of solar pores. In: Proceedings of the 11th European Solar Physics Meeting - The Dynamic Sun: Challenges for Theory and Observations, 11-16 September 2005 (Eds. Danesy, D.; Poedts, S.; De Groof, A.; Andries, J.). ESA Publ. Div., Noordwijk (2005)
Cameron, R.; Vögler, A.; Shelyag, S.; Schüssler, M.: The Decay of a Simulated Pore. In: The Solar-B Mission and the Forefront of Solar Physics, pp. 57 - 62 (Eds. Sakurai, T.; Sekii, T.). (2004)
How does our star heat its outer atmosphere, the solar corona, to unimaginable temperatures of up to 10 million degrees Celsius? With unprecedented observational data from ESA's Solar Orbiter spacecraft and powerful computer simulations, ERC starting grant awardee Pradeep Chitta intends to bring new momentum to the search for the coronal heating mechanism.
The research group “Solar Lower Atmosphere and Magnetism” (SLAM) studies the conditions and dynamic processes in the atmospheric layer between the solar surface (photosphere) and the overlying chromosphere, an approximately 2000 km thick gas layer.
The main research fields of the department "Sun and Heliosphere" are covered by the research groups "Solar and Stellar Coronae", "Solar Lower Atmosphere and Magnetism", "Solar and Stellar Magnetohydrodynamics" and "Solar Variability and Climate".