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)
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.: Helioseismology of sunspots: a case study of NOAA region 9787. Space Science Reviews 144, pp. 249 - 273 (2009)
Gizon, L.; Schunker, H.; Baldner, C. S.; Basu, S.; Birch, A. C.; Bogart, R. S.; Braun, D. C.; Cameron, R. H.; Jr., T. L. D.; Hanasoge, S. M.et al.; Jackiewicz, J.; Roth, M.; Stahn, T.; Thompson, M. J.; Zharkov, S.: Helioseismology of Sunspots: A Case Study of NOAA Region 9787. Space Science Reviews 144 (1-4), pp. 249 - 273 (2009)
Jackiewicz, J.; Gizon, L.; Birch, A. C.: High-resolution mapping of flows in the solar interior: Fully consistent OLA inversion of helioseismic travel times. Solar Physics 251, pp. 381 - 415 (2008)
Gaudio, S.; Jackiewicz, J.; Bedell, K.: Many body exchange effects close to the s-wave Feshbach resonance in two-component Fermi systems: Is a triplet superfluid possible? Phil. Mag. Lett. 87, pp. 713 - 721 (2007)
Jackiewicz, J.; Gizon, L.; Birch, A. C.; Duvall Jr., T. L.: Time-distance helioseismology: Sensitivity of f-mode travel times to flows. Astrophysical Journal 671, pp. 1051 - 1064 (2007)
Jackiewicz, J.; Gizon, L.; Birch, A. C.; Thompson, M. J.: A procedure for the inversion of f-mode travel times for solar flows. Astron. Nachrichten 328, pp. 234 - 239 (2007)
Jackiewicz, J.; Gizon, L.; Birch, A. C.: Sensitivity of solar f-mode travel times to internal flows. In: Proceedings of SOHO 17 - 10 Years of SOHO and Beyond, 7-12 May 2006, Giardini Naxos, Sicily, Italy (Ed. Lacoste, H.). ESA Publ. Div., Noordwijk (2006)
Jackiewicz, J.; Gizon, L.; Birch, A. C.: F-mode sensitivity kernels for flows. 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)
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".
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.