Marsch, E.; Pilipp, W. G.; Schwenn, R.; Mühlhäuser, K.-H.; Rosenbauer, H.: Some characteristics of proton velocity distributions in the solar wind as observed by the Helios solar probes. In: Solar Wind Four, Proceedings of the Conference held in Burghausen, August 28 - September 1, 1978, pp. 126 - 130 (Ed. Rosenbauer, H.). Max-Planck-Institut für Aeronomie, Katlenburg-Lindau (1981)
Pilipp, W. G.; Schwenn, R.; Marsch, E.; Mühlhäuser, K.-H.; Rosenbauer, H.: Electron characteristics in the solar wind as deduced from Helios observations. In: Solar Wind Four, Proceedings of the Conference held in Burghausen, August 28 - September 1, 1978, pp. 126 - 130 (Ed. Rosenbauer, H.). Max-Planck-Institut für Aeronomie, Katlenburg-Lindau (1981)
Rosenbauer, H.; Marsch, E.; Mühlhäuser, K.-H.; Pilipp, W.; Schwenn, R.: Helios: Indications of resonant wave-particle interaction in fast stream solar wind ion distributions. In: Solar Wind Four, Proceedings of the Conference held in Burghausen, August 28 - September 1, 1978, pp. 126 - 130 (Ed. Rosenbauer, H.). Max-Planck-Institut für Aeronomie, Katlenburg-Lindau (1981)
Schwenn, R.; Mühlhäuser, K.-H.; Marsch, E.; Rosenbauer, H.: Two state of the solar wind at the time of solar activity minimum, II. Radial gradients of plasma parameters in fast and slow streams. In: Solar Wind Four, Proceedings of the Conference held in Burghausen, August 28 - September 1, 1978, pp. 126 - 130 (Ed. Rosenbauer, H.). Max-Planck-Institut für Aeronomie, Katlenburg-Lindau (1981)
Wilhelm, K.; Marsch, E.; Dwivedi, B.; Feldman, U.: Observations of the Sun at vacuumu-ultravioletwavelengths form space. Part II: Results and interpretations. Max-Planck-Institut für Sonnensystemforschung, Katlenburg-Lindau, Germany (2007)
Thieme, K. M.; Marsch, E.; Schwenn, R.: Relationship between structures in the solar wind and their source regions in the corona. Max-Planck-Institut für Aeronomie, Katlenburg-Lindau (1987)
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".