Tu, C.-Y.; Marsch, E.: Comment on ``Evolution of energy-containing turbulent eddies in the solar wind'' by W. H. Matthaeus, S. Oughton, Pontius, Jr., D. H. and Y. Zhou. Journal Geophysical Research 100, pp. 12323 - 12328 (1995)
Wilhelm, K.; Curdt, W.; Marsch, E.; Schühle, U.; Lemaire, P.; Gabriel, A.; Vial, J.-C.; Grewing, M.; Huber, M. C. E.; Jordan, S. D.et al.; Poland, A. I.; Thomas, R. J.; Kühne, M.; Timothy, J. G.; Hassler, D. M.; Siegmund, O. H. W.: SUMER-Solar ultraviolet measurements of emitted radiation. Solar Physics 162, pp. 189 - 231 (1995)
LaBelle, J.; Treumann, R. A.; Marsch, E.: Elsässer variable analysis of fluctuations in the ion foreshock and undisturbed solar wind. Journal Geophysical Research 99 (A1), pp. 65 - 71 (1994)
Marsch, E.; Liu, S.: Structure functions and intermittency of velocity fluctuations in the inner solar wind. Annales Geophysicae 11, pp. 227 - 238 (1993)
Marsch, E.; Tu, C.-Y.: Modelling results on spatial transport and spectral transfer of solar wind Alfvénic turbulence. Journal Geophysical Research 98, pp. 21045 - 21059 (1993)
Marsch, E.; Tu, C.-Y.: Correlations between the fluctuations of pressure, density, temperature and magnetic field in the solar wind. Annales Geophysicae 11, pp. 659 - 677 (1993)
McKenzie, J. F.; Marsch, E.; Baumgärtel, K.; Sauer, K.: Wave and stability properties of multi-ion plasmas with application to winds and flows. Annales Geophysicae 11, pp. 341 - 353 (1993)
Tu, C.-Y.; Marsch, E.: A model of solar wind fluctuations with two components: Alfvén waves and convective structures. Journal Geophysical Research 98, pp. 1257 - 1276 (1993)
Grappin, R.; Mangeney, A.; Marsch, E.: On the origin of solar wind MHD turbulence: Helios data revisited. Journal Geophysical Research 95, pp. 8197 - 8209 (1990)
Marsch, E.; Tu, C.-Y.: Spectral and spatial evolution of compressible turbulence in the inner solar wind. Journal Geophysical Research 95, pp. 11945 - 11956 (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.: 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)
Thieme, K. M.; Marsch, E.; Schwenn, R.: Spatial structures in high-speed streams as signatures of fine structures in coronal holes. Annales Geophysicae 8 (11), pp. 713 - 724 (1990)
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".