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)
First Light for Sunrise III: the first tests with real sunlight were successful. The balloon-borne solar observatory should be ready for launch at the end of May.
First icy cold, then midnight sun: at the Arctic Circle, the team will prepare the next flight of the balloon-borne solar observatory - and hopes for solar fireworks.
Astronomical teamwork: By combining data from Solar Orbiter and SDO, a group of researchers has unambiguously determined the magnetic field at the solar surface.
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.