Gloeckler, G.; Geiss, J.; Balsiger, H.; Bedini, P.; Cain, J. C.; Fisher, J.; Fisk, L. A.; Galvin, A. B.; Gliem, F.; Hamilton, D. C.et al.; Hollweg, J. V.; Ipavich, F. M.; Joos, R.; Livi, S.; Lundgren, R.; Mall, U.; McKenzie, J. F.; Ogilvie, K. W.; Ottens, F.; Rieck, W.; Tums, E. O.; von Steiger, R.; Weiss, W.; Wilken, B.: The solar wind ion composition spectrometer. Astronomy and Astrophysics, Suppl. Ser. 92, pp. 267 - 289 (1992)
Sauer, K.; Roatsch, T.; Motschman, U.; Schwingenshuh, K.; Lundin, R.; Rosenbauer, H.; Livi, S.: Observations of plasma boundaries and phenomena around Mars with Phobos 2. Journal Geophysical Research 97, pp. 6227 - 6233 (1992)
Schwingenshuh, K.; Riedler, W.; Zhang, T. L.; Lichtenegger, H.; Rosenbauer, H.; Livi, S.; Gevai, G.; Gringauz, K.; Verigin, M.; Yeroshenko, Y.et al.; Moehlmann, D.; Roatsch, T.; Lundin, R.; Russel, C. T.; Luhmann, J.: The Martian magnetic field environment: induced or dominated by an intrinsic magnetic field? Advances in Space Research 12 (9), pp. 213 - 219 (1992)
Kirsch, E.; Keppler, E.; Witte, M.; Rosenbauer, H.; Livi, S.; Schwingenschuh, K.; McKenna-Lawlor, S. M. P.; Afonin, V. V.; O'Sullivan, D.; Thompson, A.: Pick-up ions (Eo+ > 55 keV) measured near Mars by Phobos-2 in February/March 1989. Annales Geophysicae 9, pp. 761 - 767 (1991)
Kirsch, E.; Keppler, E.; Witte, M.; Rosenbauer, H.; Livi, S.; Schwingenshuh, K.; McKenna-Lawlor, S.; Afonin, V. V.; O'Sullivan, D.; Thompson, A.: Pickup ions ( E O+ > 55 keV) measured near Mars by Phobos-2 in February/March 1989. Annales Geophysicae 9, pp. 761 - 767 (1991)
Verigin, M. I.; Gringauz, K. I.; Kotova, G. A.; Shutte, N. M.; Rosenbauer, H.; Livi, S.; Richter, A. K.; Riedler, W.; Schwingenshuh, K.; Szego, K.: On the problem of the Martian atmosphere dissipation: PhOBOS 2 TAUS spectrometer results. Journal Geophysical Research 96, pp. 19315 - 19320 (1991)
Verigin, M. I.; Shutte, N. M.; Galeev, A. A.; Gringauz, K. I.; Kotova, G. A.; Remizov, A. P.; Rosenbauer, H.; Hemmerich, P.; Livi, S.; Richter, A. K.et al.; Apathy, I.; Szego, K.; Riedler, W.; Schwingenshuh, K.; Steller, M.; Yeroshenko, Y. G.: Ions of planetary origin in the Martian magnetosphere (Phobos 2/Taus experiment). Planetary and Space Science 39, pp. 131 - 137 (1991)
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)
Kohl, L. J.; Weiser, H.; Livi, S.: Spectroscopic measurements of solar wind parameters near the Sun, Solar System Plasma Physic. Geophysical Monograph 54, pp. 81 - 88 (1989)
Hernandez, R.; Livi, S.; Marsch, E.: On the He2+ to H+ temperature ratio in slow solar wind. Journal Geophysical Research 92 (A7), pp. 7723 - 7727 (1987)
Livi, S.; Marsch, E.: Generation of solar wind proton tails and double beams by Coulomb collisions. Journal Geophysical Research 92 (A7), pp. 7255 - 7261 (1987)
Marsch, E.; Livi, S.: Observational evidence for marginal stability of solar wind ion beams. Journal Geophysical Research 92 (A7), pp. 7263 - 7268 (1987)
Livi, S.; Marsch, E.: Comparison of the Bhatnagar-Gross-Krook approximation with the exact Coulomb collision operator. Physical Review A 34 (1), pp. 533 - 540 (1986)
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".