Jockers, K.; Rosenbush, V. K.; Bonev, T.; Credner, T.: Images of polarization and colour in the inner coma of comet Hale-Bopp. Earth, Moon and Planets 78, pp. 373 - 379 (1997)
Geyer, E. H.; Jockers, K.; Kiselev, N. N.; Chernova, G. P.: A novel quadruple beam imaging polarimeter and its application to Comet Tanaka-Machholz 1992 X. Astrophysics and Space Science 239, pp. 259 - 274 (1996)
Golev, V.; Yankulova, I.; Bonev, T.; Jockers, K.: New narrow-band imaging of the extended emission-line region in the Seyfert galaxy NGC 3516. Mon. Not. Roy. Astron. Soc. 273, pp. 129 - 138 (1995)
Schleicher, H.; Balthasar, H.; Knölker, M.; Schmidt, W.; Jockers, K.: The impact of fragment ``L'' of comet SL-9 on Jupiter. Earth, Moon and Planets 66, pp. 13 - 17 (1994)
Rauer, H.; Bonev, T.; Jockers, K.; Thomas, N.: Low-resolution spectra of the Io plasma torus 2 days after the Ulysses encounter. Planetary and Space Science 41, pp. 1021 - 1028 (1993)
Rosenbauer, H.; Shutte, N.; Apathy, I.; Verigin, M.; Witte, M.; Galeev, A.; Gringauz, K.; Grünwaldt, H.; Jockers, K.; Kiraly, P.et al.; Kotova, G.; Livi, S.; Marsch, E.; Remizov, A.; Richter, A.; Riedler, W.; Szego, K.; Hemmerich, P.; Schwenn, R.; Schwingenschuh, K.; Steller, M.: First meansurements of ions of Martian origin and observation of a plasma layer in the magnetosphere of Mars: the TAUS experiment on the spacecraft PHOBOS 2. Sov. Astron. Letter 16, pp. 156 - 160 (1990)
Rosenbauer, H.; Shutte, N.; Apathy, I.; Verigin, M.; Witte, M.; Galeev, A.; Gringauz, K.; Grünwaldt, H.; Jockers, K.; Kiraly, P.et al.; Kotova, G.; Livi, S.; Marsch, E.; Remizov, A.; Richter, A.; Riedler, W.; Szego, K.; Hemmerich, P.; Schwenn, R.; Schwingenschuh, K.; Steller, M.: Evidence of a plasmasheet in the Martian magnetotail based on the TAUS experiment data from the `Phobos-2' spacecraft. Pis'ma v Astronomicheskie Zhurnal 16, pp. 368 - 377 (1990)
Jockers, K.: Near-infrared observations of the encounter of Comet Shoemaker-Levy 9 with Jupiter with the ESO-German 2.2 m telescope on La Silla, Chile. In: IAU Highlights of Astronomy, pp. 630 - 632 (Ed. Appenzeller, I.). Kluwer Acad. Publ., Dordrecht (1995)
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".