Duvall Jr., T. L.; Hanasoge, S. M.; Chakraborty, S.: Additional Evidence Supporting a Model of Shallow, High-Speed Supergranulation. Solar Physics 289 (9), pp. 3421 - 3433 (2014)
Hanasoge, S. M.: Measurements and kernels for source-structure inversions in noise tomography. Geophysical Journal International 196 (2), pp. 971 - 985 (2014)
Hanasoge, S. M.; Sreenivasan, K. R.: The Quest to Understand Supergranulation and Large-Scale Convection in the Sun. Solar Physics 289 (9), pp. 3403 - 3419 (2014)
Dombroski, D. E.; Birch, A. C.; Braun, D. C.; Hanasoge, S. M.: Testing Helioseismic-Holography Inversions for Supergranular Flows Using Synthetic Data. Solar Physics 282 (2), pp. 361 - 378 (2013)
Duvall Jr., T. L.; Hanasoge, S. M.: Subsurface supergranular vertical flows as measured using large distance separations in time-distance helioseismology. Solar Physics 287 (1-2), pp. 71 - 83 (2013)
Hanasoge, S. M.; Branicki, M.: Interpreting cross-correlations of one-bit filtered seismic noise. Geophysical Journal International 195, pp. 1811 - 1830 (2013)
Jackiewicz, J.; Birch, A. C.; Gizon, L.; Hanasoge, S. M.; Hohage, T.; Ruffio, J.-B.; Švanda, M.: Multichannel Three-Dimensional SOLA Inversion for Local Helioseismology. Solar Physics 276 (1-2), pp. 19 - 33 (2012)
Luo, Y.; Hanasoge, S.; Tromp, J.; Pretorius, F.: Detectable seismic consequences of the interaction of a primordial black hole with Earth. Astrophysical Journal 751, 16 (2012)
Švanda, M.; Gizon, L.; Hanasoge, S. M.; Ustyugov, S. D.: Validated helioseismic inversions for 3D vector flows. Astronomy and Astrophysics 530, A148 (2011)
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)
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".