Zong, Q.-G.; Wilken, B.; Daglis, I. A.; Livi, S.; Woch, J.; Reeves, G.; Doke, T.; Iyemori, T.; Mukai, T.; Yamamoto, T.et al.; Kokubun, S.; Pu, Z.-Y.; Ullaland, S.: GEOTAIL observation of energetic ion species and magnetic field in plasmoid-like structures in the course of a substorm. In: Proc. 3rd Int. Conf. on Substorms (ICS-3), Versailles, France 1996, pp. 619 - 624. ESA Publ. Div., Noordwijk (1996)
Woch, J.; Lundin, R.; Potemra, T. A.; Shapshak, M.: The projection of the magnetospheric boundary layers to mid-altitudes. In: Physical Signatures of Magnetospheric Boundary Layer Processes, pp. 83 - 97 (Eds. Holtet, J. A.; Egeland, A.). Kluwer Acad. Publ., Dordrecht (1994)
Shapshak, M.; Marklund, G.; Blomberg, L.; Woch, J.; Elphinstone, R.; Zanetti, L.: High-altitude electric field observations: Modelling the ionospheric response. Physics of Space Plasmas, p. 609 (1993)
Lundin, R.; Sandahl, I.; Woch, J.; Yamauchi, M.; Elphinstone, R.; Murphree, J. S.: Boundary layer driven magnetospheric substorms. In: Proceedings of the International Conference on Substorms. (1992)
Mishin, V. M.; Woch, J.; Eliasson, L.; Saifudinova, T. I.; Bazarzhapov, A. D.; Shirapov, D. S.; Lunyushkin, S. B.: Substorm scenario with two active phases: a study of the CDAW-9C events. In: Proceedings of the International Conference on Substorms. (1992)
Sandahl, I.; Barabash, S.; Dubinin, E. B.; Koskinen, H.; Liede, I.; Lundin, R.; Pellinen, R.; Pissarenko, N. F.; Pulkkinen, T.; Rautio, B.et al.; Woch, J.; Zakharov, A. V.: PROMICS-3, A hot plasma experient in the Interball project. In: Proceedings of the International Conference on Substorms. (1992)
Lundin, R.; Woch, J.; Yamauchi, M.: The present understanding of the cusp. In: Proceedings of the CLUSTER Workshop, Svalbard, Norway, 16-19 September 1991. ESA Publ. Div., Noordwijk (1991)
Wedeken, U.; Maul, A.; Woch, J.; Hillebrand, O.; Voelker, H.: Magnetic pulsations recorded in northern Scandinavia during the IMS: a study of Pc 4-5 events. In: Proceedings of the Achievements of the International Magnetospheric Studies (IMS). (1984)
Albert, K.; Hizberger, J.; Woch, J.; Michalik, H.: On-board calibration of the PHI instrument on-board the Solar Orbiter: Autonomous flat fielding of the HRT. Ground and space-based instruments for future research in Solar Terrestrial physics, L'Aquila, Italy (2016)
Dubinin, E.; Fraenz, M.; Zhang, T.-L.; Woch, J.; Wei, Y.: Ionospheric magnetic fields and currents at Venus and Mars. European Geosciences Union General Assembly 2014, Vienna, Austria (2014)
Dubinin, E.; Fraenz, M.; Zhang, T.-L.; Woch, J.; Wei, Y.: Ionospheric magnetic fields at Venus and Mars and their effect on plasma flow in the near planet wakes. EPSC, Estoril, Portugal (2014)
Dubinin, E.; Fraenz, M.; Zhang, T.-L.; Woch, J.; Wei, Y.; Barabash, S.: Asymmetrical response of the ionospheric magnetization and the plasma sheet formation on the IMF orientation. 6th Alfven Conference: Plasma Interactions with Solar System Objects anticipating Rosetta, MAVEN and Mars Orbiter Mission, London, UK (2014)
Albert, K.; Hirzberger, J.; Busse, D.; Rodrguez, J. B.; Castellanos Durán, J. S.; Carrascosa, J. P. C.; Fiethe, B.; Gandorfer, A. M.; Guan, Y.; Kolleck, M.et al.; Lange, T.; Michalik, H.; Solanki, S. K.; Iniesta, J. C. d. T.; Woch, J.: Performance analysis of the SO/PHI software framework for on-board data reduction. 28th annual international Astronomical Data Analysis Software & Systems (ADASS) conference, College Park, Maryland, USA (2019)
Woch, J.: Langperiodische Änderungen des Magnetfeldes und der Teilchenverteilung in der Magnetosphäre und ihr Zusammenhang mit Plasmainstabilitäten. Dissertation, Georg-August-Universität Göttingen (1987)
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".