Asvestari, E.; Temmer, M.; Caplan, R. M.; Linker, J. A.; Heinemann, S. G.; Pinto, R. F.; Henney, C. J.; Arge, C. N.; Owens, M. J.; Madjarska, M. S.et al.; Pomoell, J.; Hofmeister, S. J.; Scolini, C.; Samara, E.: Coronal Models and Detection of the Open Magnetic Field. The Astrophysical Journal 971, p. 45 (2024)
Chae, J.; van Noort, M.; Madjarska, M. S.; Lee, K.; Kang, J.; Cho, K.: Large-amplitude transverse MHD waves prevailing in the Hα chromosphere of a solar quiet region revealed by MiHI integrated field spectral observations. Astronomy and Astrophysics 687, p. A249 (2024)
Cho, K.-S.; Kumar, P.; Cho, I.-H.; Madjarska, M. S.; Nakariakov, V. M.; Lim, E.-K.; Cao, W.; Yurchyshyn, V.; Yang, X.; Park, S.-H.: High-resolution Observations of Plume Footpoints in a Solar Coronal Hole. The Astrophysical Journal 953, p. 69 (2023)
Hou, Z.; Tian, H.; Su, W.; Madjarska, M. S.; Chen, H.; Zheng, R.; Bai, X.; Deng, Y.: A Type II Radio Burst Driven by a Blowout Jet on the Sun. The Astrophysical Journal 953, p. 171 (2023)
Madjarska, M. S.; Galsgaard, K.; Wiegelmann, T.: Photospheric magnetic flux and coronal emission properties of small-scale bright and faint loops in the quiet Sun. Astronomy and Astrophysics 678, p. A32 (2023)
Nóbrega-Siverio, D.; Moreno-Insertis, F.; Galsgaard, K.; Krikova, K.; Rouppe van der Voort, L.; Joshi, R.; Madjarska, M. S.: Deciphering Solar Coronal Heating: Energizing Small-scale Loops through Surface Convection. The Astrophysical Journal 958, p. L38 (2023)
Yang, H.; Cho, K.; Bong, S.-C.; Choi, S.; Madjarska, M. S.; Kim, Y.-H.; Reginald, N.; Newmark, J.: Feasibility Study of Measuring Degree of Linear Polarization of the Solar F-Corona Using Filter Observations on the COronal Diagnostic EXperiment. Solar Physics 298, p. 57 (2023)
Madjarska, M. S.; Mackay, D. H.; Galsgaard, K.; Wiegelmann, T.; Xie, H.: Eruptions from coronal bright points: A spectroscopic view by IRIS of a mini-filament eruption, QSL reconnection, and reconnection-driven outflows. Astronomy and Astrophysics 660, p. A45 (2022)
Cho, K.; Chae, J.; Madjarska, M. S.: Investigation of the subsurface structure of a sunspot based on the spatial distribution of oscillation centers inferred from umbral flashes. Astronomy and Astrophysics 656, A86 (2021)
Cho, K.-S.; Cho, I.-H.; Madjarska, M. S.; Nakariakov, V. M.; Yang, H.; Choi, S.; Lim, E.-K.; Lee, K.-S.; Seough, J.-J.; Lee, J.et al.; Kim, Y.-H.: On the Nature of Propagating Intensity Disturbances in Polar Plumes during the 2017 Total Solar Eclipse. The Astrophysical Journal 909 (2), 202 (2021)
Lim, E.-K.; Yang, H.; Yurchyshyn, V.; Chae, J.; Song, D.; Madjarska, M. S.: Detection of Opposite Magnetic Polarity in a Light Bridge: Its Emergence and Cancellation in Association with LB Fan-shaped Jets. The Astrophysical Journal 904 (2), 84 (2020)
Galsgaard, K.; Madjarska, M. S.; Mackay, D. H.; Mou, C.: Eruptions from quiet Sun coronal bright points. II. Non-potential modelling. Astronomy and Astrophysics 623, A78 (2019)
Fu, H.; Madjarska, M. S.; Li, B.; Xia, L.; Huang, Z.: Helium abundance and speed difference between helium ions and protons in the solar wind from coronal holes, active regions, and quiet Sun. Monthly Notices of the Royal Astronomical Society 478 (2), pp. 1884 - 1892 (2018)
Mou, C.; Madjarska, M. S.; Galgaard, K.; Xia, L.: Eruptions from quiet Sun coronal bright points. I. Observations. Astronomy and Astrophysics 619, A55 (2018)
Subramanian, S.; Kashyap, V. L.; Tripathi, D.; Madjarska, M. S.; Doyle, J. G.: Energetics of Hi-C EUV brightenings. Astronomy and Astrophysics 615, A47 (2018)
First Light! The spectro-polarimeter of the world's largest solar telescope in Hawaii looks at the Sun for the first time. The instrument was developed in Germany.
Dr. Theodosios Chatzistergos receives award by the European Space Weather and Space Climate Association for his research findings on the historical activity of the Sun.
The Zdenĕk Švetska Senior Prize of the Solar Physics Division of the European Physical Society (EPS) recognizes Solanki’s pioneering contributions to solar research.
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.
Application deadline 1 October 2024. PhD projects in planetary science, solar and stellar physics, solar magnetism, heliophysics, helioseismology, asteroseismology, ...