Martinez Gonzalez, M. J.; Bellot Rubio, L. R.; Solanki, S. K.; Martinez Pillet, V.; Del Toro Iniesta, J. C.; Barthol, P.; Schmidt, W.: Resolving the Internal Magnetic Structure of the Solar Network. Astrophysical Journal 758 (2), L40 (2012)
Martínez González, M. J.; Asensio Ramos, A.; Manso Sainz, R.; Khomenko, E.; Martínez Pillet, V.; Solanki, S. K.; López Ariste, A.; Schmidt, W.; Barthol, P.; Gandorfer, A.: Unnoticed Magnetic Field Oscillations in the Very Quiet Sun Revealed by Sunrise/IMaX. Astrophysical Journal 730, L37 (2011)
Perez-Grande, I.; Sanz-Andres, A.; Bezdenejnykh, N.; Farrahi, A.; Barthol, P.; Meller, R.: Thermal control of SUNRISE, a balloon-borne solar telescope. J. Aerosp. Eng 225 (G9), pp. 1037 - 1049 (2011)
Yelles Chaouche, L.; Moreno-Insertis, F.; Martínez Pillet, V.; Wiegelmann, T.; Bonet, J. A.; Knölker, M.; Bellot Rubio, L. R.; del Toro Iniesta, J. C.; Barthol, P.; Gandorfer, A.et al.; Schmidt, W.; Solanki, S. K.: Mesogranulation and the Solar Surface Magnetic Field Distribution. Astrophysical Journal 727, L30 (2011)
Bell, A.; Barthol, P.; Berkefeld, T.; Feger, B.; Gandorfer, A. M.; Heidecke, F.; Knoelker, M.; Pillet, V. M.; Schmidt, W.; Sigwarth, M.et al.; Solanki, S. K.; Soltau, D.; Title, A. M.: Flight control software for the wave-front sensor of SUNRISE 1m balloon telescope. Proceedings of the SPIE 7740, 774003 (2010)
Bello Gonzalez, N.; Franz, M.; Martinez Pillet, V.; Bonet, J. A.; Solanki, S. K.; del Toro Iniesta, J. C.; Schmidt, W.; Gandorfer, A.; Domingo, V.; Barthol, P.et al.; Berkefeld, T.; Knoelker, M.: Detection of Large Acoustic Energy Flux in the Solar Atmosphere. Astrophysical Journal 723 (2), pp. L134 - L138 (2010)
Borrero, J. M.; Martinez-Pillet, V.; Schlichenmaier, R.; Solanki, S. K.; Bonet, J. A.; del Toro Iniesta, J. C.; Schmidt, W.; Barthol, P.; Gandorfer, A.; Domingo, V.et al.; Knoelker, M.: Supersonic Magnetic Upflows in Granular Cells Observed with SUNRISE/IMaX. Astrophysical Journal 723 (2), pp. L144 - L148 (2010)
Danilovic, S.; Beeck, B.; Pietarila, A.; Schüssler, M.; Solanki, S. K.; Martinez Pillet, V.; Bonet, J. A.; del Toro Iniesta, J. C.; Domingo, V.; Barthol, P.et al.; Berkefeld, T.; Gandorfer, A.; Knölker, M.; Schmidt, W.; Title, A. M.: Transverse Component of the Magnetic Field in the Solar Photosphere Observed by SUNRISE. Astrophysical Journal 723 (2), pp. L149 - L153 (2010)
Riethmüller, T. L.; Solanki, S. K.; Pillet, V. M.; Hirzberger, J.; Feller, A.; Bonet, J. A.; Bello González, N.; Franz, M.; Schüssler, M.; Barthol, P.et al.; Berkefeld, T.; del Toro Iniesta, J. C.; Domingo, V.; Gandorfer, A.; Knölker, M.; Schmidt, W.: Bright points in the quiet Sun as observed in the visible and near-UV by the balloon-borne observatory Sunrise. Astrophysical Journal 723, L169 (2010)
Roth, M.; Franz, M.; Bello González, N.; Martinez Pillet, V.; Bonet, J. A.; Gandorfer, A.; Barthol, P.; Solanki, S. K.; Berkefeld, T.; Schmidt, W.et al.; del Toro Iniesta, J. C.; Domingo, V.; Knölker, M.: Surface Waves in Solar Granulation Observed with SUNRISE. Astrophysical Journal 723 (2), pp. L175 - L179 (2010)
Analyzing the high spatial resolution solar Ca II H and K emission data obtained by the SUNRISE mission and building a model of other stars more active than the Sun
The magnetic field in the solar atmosphere exceeds the geomagnetic field strength by four orders of magnitude. It greatly influences the processes of energy transport within the solar atmosphere, and dominates the morphology of the solar chromosphere and corona. Kinetic energy from convective motions in the Sun can be efficiently stored in magnetic fields and subsequently released - to heat the solar corona to several million degrees or to blast off coronal mass ejections.
For PhD students whose project is already funded and who are applying for admission to the IMPRS, or for applicants who want to bring their own funding and their own project idea to the IMPRS.
The Solar Lower Atmosphere and Magnetism (SLAM) group covers many exciting subjects in solar physics, focussing on the development and testing of highly novel solar instrumentation, reduction and analysis of highest quality solar observations, or improving and developing advanced techniques for the analysis of solar observations.