Parenti, S.; Chifu, I.; Del Zanna, G.; Edmondson, J.; Giunta, A.; Hansteen, V.H.; Higginson, A.; Laming, J.M.; Lepri, S.T.; Lynch, B.J.et al.; Rivera, Y.J.; von Steiger, R.; Wiegelmann, T.; Wimmer-Schweingruber, R.F.; Zambrana Prado, N.; Pelouze, G.: Linking the Sun to the Heliosphere Using Composition Data and Modelling: A Test Case with a Coronal Jet. Space Science Reviews 217 (8), 78 (2021)
Mierla, M.; Seaton, D. B.; Berghmans, D.; Chifu, I.; De Groof, A.; Inhester, B.; Rodriguez, L.; Stenborg, G.; Zhukov, A. N.: Study of a Prominence Eruption using PROBA2/SWAP and STEREO/EUVI Data. Solar Physics 286, pp. 241 - 253 (2013)
Chifu, I.; Inhester, B.; Mierla, M.; Chifu, V.; Wiegelmann, T.: First 4D Reconstruction of an Eruptive Prominence Using Three Simultaneous View Directions. Solar Physics 281, pp. 121 - 135 (2012)
Mierla, M.; Chifu, I.; Inhester, B.; Rodriguez, L.; Zhukov, A.: Low polarised emission from the core of coronal mass ejections. Astronomy and Astrophysics 530, L1 (2011)
Wiegelmann, T.; Chifu, I.; Inhester, B.: Global coronal magnetic field modelling for Solar Orbiter. SPICE Operations Consortium Meeting , Göttingen, Germany (2019)
Wiegelmann, T.; Neukirch, T.; Nickeler, D. H.; Chifu, I.; Inhester, B.: Global coronal magnetic field modelling: new models. ISSI-meeting on „Linking the Sun to the heliosphere using composition data and modelling", Berne, Switzerland (2019)
Wiegelmann, T.; Chifu, I.; Inhester, B.: Global magnetic field modelling for the Solar Orbiter mission. 6th Metis Workshop with Focus on Operations, Göttingen, Germany (2018)
Wiegelmann, T.; Chifu, I.; Inhester, B.: Global magnetic field modelling for the Solar Orbiter mission. Mini-Workshop on Solar Magnetic Field at the Purple Mountain Observatory, Nanjing, Nanjing, China (2018)
Chifu, I.; Wiegelmann, T.; Inhester, B.: Nonlinear force-free coronal magnetic stereoscopy. SOLARNET IV, The Physics of the Sun from the Interior to the Outer Atmosphere, Lanzarote, Spain (2017)
Chifu, I.; Wiegelmann, T.; Inhester, B.: Coronal magnetic field modeling using stereoscopic constraints. 15th European Solar Physics Meeting, Budapest, Hungary (2017)
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.
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".