Hanasoge, S. M.; Komatitsch, D.; Gizon, L.: An absorbing boundary formulation for the stratified, linearized, ideal MHD equations based on an unsplit, convolutional perfectly matched layer. Astronomy and Astrophysics 522, A87 (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)
Hanasoge, S. M.; Cally, P. S.: Multiple scattering of waves by a pair of gravitationally stratified flux tubes. Astrophysical Journal 697, pp. 651 - 659 (2009)
Hanasoge, S. M.; Cally, P. S.: Multiple Scattering of Waves by a Pair of Gravitationally Stratified Flux Tubes. The Astrophysical Journal 697, 651 (2009)
Birch, A.; Gizon, L.; Hanasoge, S.; Langfellner, J.: Ist die Konvektion im Sonneninneren langsamer als gedacht? In: Jahrbuch 2013, n/a. Max-Planck-Gesellschaft, München (2013)
Moradi, H.; Hanasoge, S. M.: Deep-focus diagnostics of sunspot structure. In: Magnetic Coupling between the Interior and Atmosphere of the Sun, pp. 378 - 385 (Eds. Hasan, S. S.; Rutten, R. J.). (2010)
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".