Tu, C.-Y.; Marsch, E.: Evidence for a ``background'' spectrum of solar wind turbulence in the inner heliosphere. Journal Geophysical Research 95, pp. 4337 - 4341 (1990)
Tu, C.-Y.; Marsch, E.; Rosenbauer, H.: The dependence of MHD turbulence spectra on the inner solar wind stream structure near solar minimum. Geophysical Research Letters 17, pp. 283 - 286 (1990)
Marsch, E.; Pilipp, W. G.; Thieme, K. M.; Rosenbauer, H.: Cooling of solar wind electrons inside 0.3 AU. Journal Geophysical Research 94, pp. 6893 - 6898 (1989)
Marsch, E.; Tu, C.-Y.: Dynamics of correlation functions with Elsässer variables for inhomogeneous MHD turbulence. Journal of Plasma Physics 41, pp. 479 - 491 (1989)
Thieme, K. M.; Marsch, E.; Rosenbauer, H.: Estimates of alpha particle heating in the solar wind inside 0.3 AU. Journal Geophysical Research 94, pp. 2673 - 2676 (1989)
Thieme, K. M.; Schwenn, R.; Marsch, E.: Are structures in high-speed streams signatures of coronal fine structures? Advances in Space Research 9, pp. 127 - 130 (1989)
Tu, C.-Y.; Marsch, E.; Thieme, K. M.: Basic properties of solar wind MHD turbulence near 0.3 AU analysed by means of Elsässer variables. Journal Geophysical Research 94, pp. 11739 - 11759 (1989)
Richter, A. K.; Marsch, E.: Helios observational constraints on the development of interplanetary slow shocks. Annales Geophysicae 6, pp. 319 - 324 (1988)
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)
Marsch, E.; Richter, A. K.: On the equation of state and collision time for a multicomponent, anisotropic solar wind. Annales Geophysicae 5A, pp. 71 - 82 (1987)
Hernández, R.; Marsch, E.: Collisional transfer of energy and momentum between drifting tri-Maxwellians. Journal of Plasma Physics 35, pp. 473 - 482 (1986)
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)
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.