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)
First Light! The spectro-polarimeter of the world's largest solar telescope in Hawaii looks at the Sun for the first time. The instrument was developed in Germany.
Dr. Theodosios Chatzistergos receives award by the European Space Weather and Space Climate Association for his research findings on the historical activity of the Sun.
The Zdenĕk Švetska Senior Prize of the Solar Physics Division of the European Physical Society (EPS) recognizes Solanki’s pioneering contributions to solar research.
The magnetic field in the solar atmosphere exceeds the geomagnetic field strength by four orders of magnitude. It greatly influences the processes of energy transport within the solar atmosphere, and dominates the morphology of the solar chromosphere and corona. Kinetic energy from convective motions in the Sun can be efficiently stored in magnetic fields and subsequently released - to heat the solar corona to several million degrees or to blast off coronal mass ejections.
Application deadline 1 October 2024. PhD projects in planetary science, solar and stellar physics, solar magnetism, heliophysics, helioseismology, asteroseismology, ...