Verigin, M. I.; Kotova, G. A.; Remizov, A. P.; Shutte, N. M.; Schwingenschuh, K.; Riedler, W.; Zhang, T.-L.; Rosenbauer, H.; Szegö, K.; Tátrallyay, M.et al.; Styazhkin, V.: Studies of the Martian bow shock response to the variations of the magnetosphere dimensions according to TAUS and MAGMA measurements aboard the PHOBOS 2 orbiter. Advances in Space Research 20, pp. 155 - 158 (1997)
Verigin, M.; Kotova, G.; Shutte, N.; Remizov, A.; Szegö, K.; Tátrallyay, M.; Apáthy, I.; Rosenbauer, H.; Livi, S.; Richter, A. K.et al.; Schwingenschuh, K.; Zhang, T.-L.; Slavin, J.; Lemaire, J.: Quantitative model of the Martian magnetopause shape and its variation with the solar wind ram pressure based on Phobos 2 observations. Journal Geophysical Research 102, pp. 2147 - 2155 (1997)
Astudillo, H. F.; Livi, S.; Marsch, E.; Rosenbauer, H.: Evidence for nongyrotropic alpha particle and proton distribution functions: TAUS solar wind measurements. Journal Geophysical Research 101, pp. 24423 - 24432 (1996)
Banaszkiewicz, M.; Witte, M.; Rosenbauer, H.: Determination of interstellar helium parameters from the ULYSSES-NEUTRALGAS experiment: Method of data analysis. Astron. Astrophys. Suppl. Ser. 120, pp. 587 - 602 (1996)
Bavassano, B.; Bruno, R.; Rosenbauer, H.: MHD compressive turbulence in the solar wind and the nearly incompressible approach. Astrophysics and Space Science 243, pp. 159 - 162 (1996)
Bavassano, B.; Bruno, R.; Rosenbauer, H.: MHD compressive turbulence in the solar wind and the nearly incompressible approach. Astrophysics and Space Science 243, pp. 159 - 162 (1996)
Marsch, E.; Tu, C.-Y.; Rosenbauer, H.: Multifractal scaling of the kinetic energy flux in solar wind turbulence. Annales Geophysicae 14 (3), pp. 259 - 269 (1996)
Tu, C.-Y.; Marsch, E.; Rosenbauer, H.: An extended structure-function model and its application to the analysis of solar wind intermittency properties. Annales Geophysicae 14 (3), pp. 270 - 285 (1996)
Witte, M.; Banaszkiewicz, M.; Rosenbauer, H.: Recent results on the parameters of the interstellar helium from the ULYSSES/GAS experiment. Space Science Reviews 78, pp. 289 - 296 (1996)
Shelley, E. G.; Ghielmetti, A. G.; Balsiger, H.; Black, R. K.; Bowles, J. A.; Bowman, R. P.; Bratschi, O.; Burch, J. L.; Carlson, C. W.; Coker, A. J.et al.; Drake, J. F.; Fischer, J.; Geiss, J.; Johnstone, A.; Kloza, D. L.; Lennartsson, O. W.; Magoncelli, A. L.; Paschmann, G.; Peterson, W. K.; Rosenbauer, H.; Sanders, T. C.; Steinacher, M.; Walton, D. M.; Whalen, B. A.; Young, D. T.: The Toroidal Imaging Mass-Angle Spectrograph (TIMAS) for the POLAR Mission. Space Science Reviews 71, pp. 497 - 530 (1995)
Shutte, N.; Gringauz, K.; Király, P.; Kotova, G.; Nagy, A. F.; Rosenbauer, H.; Szegö, K.; Verigin, M.: Nightside electron flux measurements at Mars by the Phobos-2 HARP instrument. Geophysical Research Letters 22, pp. 863 - 866 (1995)
Zhang, T.-L.; Schwingenschuh, K.; Petrinec, S. M.; Russell, C. T.; Luhmann, J. G.; Rosenbauer, H.; Verigin, M. I.; Kotova, G.: Studies of the draping and flaring angles of the Mars and Earth magnetotails. Advances in Space Research 16, pp. (4)99 - (4)103 (1995)
Goldstein, R.; Altwegg, K.; Fuselier, S. A.; Goldstein, B. E.; Balsiger, H.; Jost, F.; Coates, A.; Neubauer, F. M.; Rosenbauer, H.: Giotto ion mass spectrometer measurements at comet P/Grigg-Skjellerup. Journal Geophysical Research 99, pp. 19255 - 19265 (1994)
Rosenbauer, H.; Verigin, M. I.; Kotova, G. A.; Livi, S.; Remizov, A. P.; Riedler, W.; Schwingenschuh, K.; Shutte, N. M.; Slavin, J. A.; Szegö, K.et al.; Tátrallyay, M.; Zhang, T.-L.: The relationship between the magnetic field in the Martian magnetotail and upstream solar wind parameters. Journal Geophysical Research 99, pp. 17199 - 17204 (1994)
Zhang, T.-L.; Schwingenschuh, K.; Russell, C. T.; Luhmann, J. G.; Rosenbauer, H.; Verigin, M. I.; Kotova, G.: The flaring of the Martian magnetotail observed by the Phobos 2 spacecraft. Geophysical Research Letters 21, pp. 1121 - 1124 (1994)
Altwegg, K.; Balsiger, H.; Geiss, J.; Goldstein, R.; Ip, W.-H.; Meier, A.; Neugebauer, M.; Rosenbauer, H.; Shelley, E.: The ion population between 1300 km and 230 000 km in the coma of comet P/Halley. Astronomy and Astrophysics 279, pp. 260 - 266 (1993)
Kirsch, E.; McKenna-Lawler, S. M. P.; Afonin, V. V.; Keppler, E.; Livi, S.; Rosenbauer, H.; Witte, M.; Schwingenshuh, K.; Tompson, A.; O'Sullivan, D.: Signature of the Martian moon Phobos in the fluxes of energetic particles as measured by experiment SLED onboard Phobos 2. Space Science Reviews 4 (6), pp. 435 - 440 (1993)
Kirsch, E.; McKennal-Lawlor, S. M. P.; Afonin, V. V.; Keppler, E.; Livi, S.; Rosenbauer, H.; Witte, M.; Schwingenschuh, K.; Thompson, A.; O'Sullivan, D.: Signatures of the Martian moon Phobos in the fluxes of energetic particles as measured by experiment SLED onboard Phobos 2. Planetary and Space Science 41 (6), pp. 435 - 440 (1993)
Verigin, M. I.; Gringauz, K. I.; Kotova, G. A.; Remizov, A. P.; Shutte, N. M.; Rosenbauer, H.; Livi, S.; Richter, A. K.; Riedler, W.; Schwingenshuh, K.et al.; Szego, K.; Apathy, I.; Tatrallyay, M.: The dependence of the Martian magnetopause and bow shock on the solar wind ram pressure according to PHOBOS 2/TAUS spectrometer measurements. Journal Geophysical Research 98 (A2), pp. 1303 - 1309 (1993)
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".
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.