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)
The dwarf planet is a bizarre, cryovolcanic world. However, the organic deposits discovered on its surface so far are unlikely to originate from its interior.
The Uranian magnetic field is more expansive than previously thought, according to newly analyzed data from Voyager 2, making it easier to search for moons with oceans.