Young, P. R.; Tian, H.; Peter, H.; Rutten, R. J.; Nelson, C. J.; Huang, Z.; Schmieder, B.; Vissers, G. J. M.; Toriumi, S.; van der Voort, L. H. M. R.et al.; Madjarska, M. S.; Danilovic, S.; Berlicki, A.; Chitta, L. P.; Cheung, M. C. M.; Madsen, C.; Reardon, K. P.; Katsukawa, Y.; Heinzel, P.: Solar Ultraviolet Bursts. Space Science Reviews 214, 120 (2018)
Fu, H.; Madjarska, M. S.; Xia, L.; Li, B.; Huang, Z.; Wangguan, Z.: Charge States and FIP Bias of the Solar Wind from Coronal Holes, Active Regions, and Quiet Sun. Astronomical Journal 836, 169 (2017)
Galsgaard, K.; Madjarska, M. S.; Moreno-Insertis, F.; Huang, Z.; Wiegelmann, T.: Magnetic topological analysis of coronal bright points. Astronomy and Astrophysics 606, A46 (2017)
Huang, Z.; Madjarska, M. S.; Scullion, E. M.; Xia, L.-D.; Doyle, J. G.; Ray, T.: Explosive events in active region observed by IRIS and SST/CRISP. Monthly Notices of the Royal Astronomical Society 464 (2), pp. 1753 - 1761 (2017)
Xie, H.; Madjarska, M. S.; Li, B.; Huang, Z.; Xia, L.; Wiegelmann, T.; Fu, H.; Mou, C.: The Plasma Parameters and Geometry of Cool and Warm Active Region Loops. Astrophysical Journal 842, 38 (2017)
Madjarska, M. S.; Wiegelmann, T.: Coronal hole boundary evolution at small scales. I. EIT 195 Å and TRACE 171 Å view. Astronomy and Astrophysics 503, pp. 991 - 997 (2009)
Innes, D. E.; Attie, R.; Hara, H.; Madjarska, M. S.: EIS/ Hinode Observations of Doppler Flow Seen through the 40-Arcsec Wide-Slit. Solar Physics 252, pp. 283 - 292 (2008)
Madjarska, M. S.; Doyle, J. G.: Small-scale flows in SUMER and TRACE high-cadence co-observations. Astronomy and Astrophysics 482, pp. 273 - 278 (2008)
Pérez-Suárez, D.; Maclean, R. C.; Doyle, J. G.; Madjarska, M. S.: The structure and dynamics of a bright point as seen with Hinode, SoHO and TRACE. Astronomy and Astrophysics 492, pp. 575 - 583 (2008)
Santos, J.; Büchner, J.; Madjarska, M. S.; Alves, M.: On the relation between DC current locations and an EUV bright point: A case study. ASTRONOMY & ASTROPHYSICS (1), pp. 345 - 352 (2008)
Subramanian, S.; Madjarska, M. S.; Maclean, R. C.; Doyle, J. G.; Bewsher, D.: Magnetic topology of blinkers. Astronomy and Astrophysics 488, pp. 323 - 329 (2008)
Doyle, J. G.; Giannikakis, J.; Xia, L. D.; Madjarska, M. S.: Line broadening of EUV lines across the solar limb: A spicule contribution? Astronomy and Astrophysics 431, pp. L17 - L20 (2005)
García-Alvarez, D.; Johns-Krull, C. M.; Doyle, J. G.; Ugarte-Urra, I.; Madjarska, M. S.; Butler, C. J.: Optical and EUV observations of solar flare kernels. Astronomy and Astrophysics 444, pp. 593 - 603 (2005)
Ugarte-Urra, I.; Doyle, J. G.; Walsh, R. W.; Madjarska, M. S.: Electron density along a coronal loop observed with CDS/SOHO. Astronomy and Astrophysics 439, pp. 351 - 359 (2005)
Teriaca, L.; Banerjee, D.; Falchi, A.; Doyle, J. G.; Madjarska, M. S.: Transition region small-scale dynamics as seen by SUMER on SOHO. Astronomy and Astrophysics 427, pp. 1065 - 1074 (2004)
Koumtzis, A.; Wiegelmann, T.; Madjarska, M. S.: Computing the global coronal magnetic field during activity maximum and minimum with a newly developed nonlinear force-free Yin-Yang code. In: EGU General Assembly Conference Abstracts, pp. EGU - 17168. EGU General Assembly Conference Abstracts, Vienna, Austria, 2023. (2023)
Madjarska, M. S.; Wiegelmann, T.: Evolution of coronal hole boundaries seen in EIT 195 Å and TRACE 171 Å images. In: Modern Solar Facilities - Advanced Solar Science, pp. 249 - 252 (Eds. Kneer, F.; Puschmann, K. G.; Wittmann, A. D.). Universitätverlag Göttingen (2007)
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
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 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.
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.