Baker, D.; van Driel-Gesztelyi, L.; James, A. W.; Démoulin, P.; To, A. S. H.; Murabito, M.; Long, D. M.; Brooks, D. H.; McKevitt, J.; Laming, J. M.et al.; Green, L. M.; Yardley, S. L.; Valori, G.; Mihailescu, T.; Matthews, S. A.; Kuniyoshi, H.: Searching for Evidence of Subchromospheric Magnetic Reconnection on the Sun. The Astrophysical Journal 970, p. 39 (2024)
Jafarzadeh, S.; Schiavo, L. A. C. A.; Fedun, V.; Solanki, S. K.; Stangalini, M.; Calchetti, D.; Verth, G.; Jess, D. B.; Grant, S. D. T.; Ballai, I.et al.; Gafeira, R.; Keys, P. H.; Fleck, B.; Morton, R. J.; Browning, P. K.; Silva, S. S. A.; Appourchaux, T.; Gandorfer, A.; Gizon, L.; Hirzberger, J.; Kahil, F.; Orozco Suárez, D.; Schou, J.; Strecker, H.; del Toro Iniesta, J. C.; Valori, G.; Volkmer, R.; Woch, J.: Sausage, kink, and fluting magnetohydrodynamic wave modes identified in solar magnetic pores by Solar Orbiter/PHI. Astronomy and Astrophysics 688, p. A2 (2024)
Liu, Y.; Komm, R.; Brummell, N.; Hoeksema, J.; Manek, B.; Valori, G.: The Relationship between Kinetic and Magnetic Helicity in Solar Active Regions. ASTROPHYSICAL JOURNAL (1) (2024)
Petrova, E.; Van Doorsselaere, T.; Berghmans, D.; Parenti, S.; Valori, G.; Plowman, J.: Observations of fan-spine topology by Solar Orbiter/EUI: Rotational motions and indications of Alfvén waves. Astronomy and Astrophysics 687, p. A13 (2024)
Baker, D.; Démoulin, P.; Yardley, S. L.; Mihailescu, T.; van Driel-Gesztelyi, L.; D'Amicis, R.; Long, D. M.; To, A. S. H.; Owen, C. J.; Horbury, T. S.et al.; Brooks, D. H.; Perrone, D.; French, R. J.; James, A. W.; Janvier, M.; Matthews, S.; Stangalini, M.; Valori, G.; Smith, P.; Aznar Cuadrado, R.; Peter, H.; Schühle, U.; Harra, L.; Barczynski, K.; Berghmans, D.; Zhukov, A. N.; Rodriguez, L.; Verbeeck, C.: Observational Evidence of S-web Source of the Slow Solar Wind. The Astrophysical Journal 950, p. 65 (2023)
Liu, Y.; Welsch, B. T.; Valori, G.; Georgoulis, M. K.; Guo, Y.; Pariat, E.; Park, S.-H.; Thalmann, J. K.: Changes of Magnetic Energy and Helicity in Solar Active Regions from Major Flares. The Astrophysical Journal 942, p. 27 (2023)
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.