He, J.; Marsch, E.; Tu, C.; Tian, H.: Excitation of kink waves due to small-scale magnetic reconnection in the chromosphere? Astrophysical Journal 705, pp. L217 - L222 (2009)
Mecheri, R.; Marsch, E.: Erratum Drift instabilities in the solar corona within the multi-fluid description. Astronomy and Astrophysics 503, pp. 589 - 590 (2009)
Stverák, S.; Maksimovic, M.; Trávnicek, P. M.; Marsch, E.; Fazakerley, A. N.; Scime, E. E.: Radial evolution of nonthermal electron populations in the low-latitude solar wind: Helios, Cluster, and Ulysses Observations. Journal Geophysical Research 114, A05104 (2009)
Bourouaine, S.; Marsch, E.; Vocks, C.: On the efficiency of nonresonant ion heating by coronal Alfven waves. Astrophysical Journal 684, pp. L119 - L122 (2008)
Curdt, W.; Tian, H.; Dwivedi, B. N.; Marsch, E.: The redshifted network contrast of transition region emission. Astronomy and Astrophysics 491, pp. L13 - L16 (2008)
He, J.-S.; Tu, C.-Y.; Marsch, E.: Modeling of Solar Wind in the Coronal Funnel with Mass and Energy Supplied at 5 Mm. Solar Physics 250, pp. 147 - 158 (2008)
Marsch, E.; Tian, H.; Sun, J.; Curdt, W.; Wiegelmann, T.: Plasma flows guided by strong magnetic fields in the solar corona. Astrophysical Journal 685, pp. 1262 - 1269 (2008)
Mecheri, R.; Marsch, E.: Drift instabilities in the solar corona within the multi-fluid description. Astronomy and Astrophysics 481, pp. 853 - 860 (2008)
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, ...
First Light for Sunrise III: the first tests with real sunlight were successful. The balloon-borne solar observatory should be ready for launch at the end of May.
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.