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)
The Planetary Plasma Environments group (PPE) has a strong heritage in the exploration of planetary magnetospheres and space plasma interactions throughout the solar system. It has contributed instruments to several past missions that flew-by or orbited Jupiter (Galileo, Cassini, Ulysses). The PPE participates in the JUICE mission by contributing hardware and scientific expertise to the Particle Environment Package (PEP).
Application deadline 1 October 2024. PhD projects in planetary science, solar and stellar physics, solar magnetism, heliophysics, helioseismology, asteroseismology, ...
In analyzing solar observations from the 19th century, scientists are turning to amateur researchers for help. The project will allow to better understand the history of our star.
Astronomical teamwork: By combining data from Solar Orbiter and SDO, a group of researchers has unambiguously determined the magnetic field at the solar surface.