Marsch, E.; Mühlhäuser, K.-H.; Rosenbauer, H.; Schwenn, R.: On the Equation of State of Solar Wind Ions Derived From Helios Measurements. Journal Geophysical Research 88, pp. 2982 - 2992 (1983)
Pizzo, V.; Schwenn, R.; Marsch, E.; Rosenbauer, H.; Mühlhäuser, K.-H.; Neubauer, F. M.: Determination of the solar wind angular momentum flux from the Helios data - an observational test of the Weber and Davis theory. Astrophysical Journal 271, pp. 335 - 354 (1983)
Burlaga, L. F.; Klein, L.; Sheeley, N. R.; Michels, D. J.; Howard, R. A.; Koomen, M. J.; Schwenn, R.; Rosenbauer, H.: A magnetic cloud and a coronal mass ejection. Geophysical Research Letters 9, pp. 1317 - 1320 (1982)
Marsch, E.; Mühlhäuser, K.-H.; Rosenbauer, H.; Schwenn, R.; Neubauer, F. M.: Solar wind helium ions: Observations of the Helios solar probes between 0.3 and 1 AU. Journal Geophysical Research 87, pp. 35 - 51 (1982)
Marsch, E.; Mühlhäuser, K.-H.; Rosenbauer, H.; Schwenn, R.; Denskat, K. U.: Pronounced proton core temperature anisotropy, ion differential speed, and simultaneous Alfvén wave activity in slow solar wind at 0.3 AU. Journal Geophysical Research 86, pp. 9199 - 9203 (1981)
Burlaga, L.; Lepping, R.; Weber, R.; Armstrong, T.; Goodrich, C.; Sullivan, J.; Gurnett, D.; Kellogg, P.; Keppler, E.; Mariani, F.et al.; Neubauer, F. M.; Rosenbauer, H.; Schwenn, R.: Interplanetary particles and fields, November 22 to December 6, 1977: Helios, Voyager, and IMP observations between 0.6 and 1.6 AU. Journal Geophysical Research 85, pp. 2227 - 2242 (1980)
Schwenn, R.; Rosenbauer, H.; Mühlhäuser, K.-H.: Singly-ionized helium in the driver gas of an interplanetary shock wave. Geophysical Research Letters 7, pp. 201 - 204 (1980)
Gurnett, D. A.; Marsch, E.; Pilipp, W.; Schwenn, R.; Rosenbauer, H.: Ion-Acoustic Waves and Related Plasma Observations in the Solar Wind. Journal Geophysical Research 84, pp. 2029 - 2038 (1979)
Burlaga, L. F.; Ness, N. F.; Mariani, F.; Bavassano, B.; Villante, U.; Rosenbauer, H.; Schwenn, R.; Harvey, J.: Magnetic fields and flows between 1 and 0.3 AU during the primary mission of Helios-1. Journal Geophysical Research 83, pp. 5167 - 5174 (1978)
Cuperman, S.; Levush, B.; Dryer, M.; Rosenbauer, H.; Schwenn, R.: On the radial expansion of the solar wind plasma between 0.3 and 1.0 astronomical units. Astrophysical Journal 226, pp. 1120 - 1128 (1978)
Schwenn, R.; Montgomery, M. D.; Rosenbauer, H.; Mühlhäuser, K.-H.; Bame, S. J.; Feldman, W. C.; Hansen, R. T.: Direct observation of the latitudinal extent of a high-speed stream in the solar wind. Journal Geophysical Research 83, pp. 1011 - 1017 (1978)
Rosenbauer, H.; Schwenn, R.; Marsch, E.; Meyer, B.; Miggenrieder, H.; Montgomery, M.; Mühlhäuser, K.-H.; Pilipp, W.; Voges, W.; Zink, S. K.: A Survey on Initial Results of the Helios Plasma Experiment. J. Geophys. 42, pp. 561 - 580 (1977)
Hilchenbach, M.; Chares, B.; Rosenbauer, H.: First contact with a comet surface: Rosetta lander simulations. In: The new Rosetta targets: Oberservations, simulations and instrument performances, pp. 289 - 296 (Eds. Colangeli, L.; Epifani, E.; Palumbo, P.). Kluwer Academic Publishers, Dordrecht Boston London (2004)
Witte, M.; Rosenbauer, H.; Banaszkiewicz, M.; Fahr, H.: The ULYSSES Neutral Gas experiment: Determination of the velocity and temperature of the interstellar neutral helium. In: International Heliospheric Study, (Newsletter 8), p. 36 (1994)
Kikuchi, H.; Gurnett, D. A.; Anderson, R. R.; Keppler, E.; Richter, A. K.; Schwenn, R.; Marsch, E.; Pilipp, W. G.; Richter, K.; Rosenbauer, H.: Type II interplanetary radio bursts and electron plasma oscillations associated with interplanetary shocks, superthermal electrons, and low/medium energy protons. In: Proceedings of the Second International Workshop on the Relation Between Laboratory and Space Plasmas, Tokyo, Japan, November 25-26, 1986, pp. 415 - 421 (Ed. Kikuchi, H.). Springer-Verlag, Berlin (1988)
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".