Maneva, Y. G.; Araneda, J. A.; Marsch, E.: Regulation of Ion Drifts and Anisotropies by Parametrically Unstable Finite-Amplitude Alfven-Cyclotron Waves in the Fast Solar Wind. Astrophysical Journal 783 (2), 139 (2014)
Perrone, D.; Bourouaine, S.; Valentini, F.; Marsch, E.; Veltri, P.: Generation of temperature anisotropy for alpha particle velocity distributions in solar wind at 0.3 AU: Vlasov simulations and Helios observations. Journal Geophysical Research 119 (4), pp. 2400 - 2410 (2014)
Araneda, J. A.; Astudillo, H.; Marsch, E.: Intercations of Alfven-Cyclotron Waves with Ions in the Solar Wind. Space Science Reviews 172, pp. 361 - 372 (2012)
Bourouaine, S.; Alexandrova, O.; Marsch, E.; Maksimovic, M.: On spectral breaks in the power spectra of magnetic fluctuations in fast solar wind between 0.3 and 0.9 AU. Astrophysical Journal 749, pp. 102 - 109 (2012)
Gupta, G. R.; Teriaca, L.; Marsch, E.; Solanki, S. K.; Banerjee, D.: Spectroscopic observations of propagating disturbances in a polar coronal hole: evidence of slow magneto-acoustic waves. Astronomy and Astrophysics 546, A93 (2012)
He, J.; Tu, C.; Marsch, E.; Yao, S.: Do oblique Alfven/ion-cyclotron or fast-mode/whistler waves dominate the dissipation of solar wind turbulence near the proton inertial length? Astrophysical Journal 745, L8 (2012)
He, J.; Tu, C.; Marsch, E.; Yao, S.: Reproduction of the Observed Two-Component Magnetic Helicity in Solar Wind Turbulence by a Superposition of Parallel and Oblique Alfven Waves. Astrophysical Journal 749 (1), 86 (2012)
Bourouaine, S.; Marsch, E.; Neubauer, F. M.: Temperature anisotropy and differential streaming of solar wind ions. Correlations with transverse fluctuations. Astronomy and Astrophysics 536, A39 (2011)
Bourouaine, S.; Marsch, E.; Neubauer Fritz, M.: On the Relative Speed and Temperature Ratio of Solar Wind Alpha Particles and Protons: Collisions Versus Wave Effects. Astrophysical Journal 728, pp. L3 - L7 (2011)
de Lucas, A.; Schwenn, R.; dal Lago, A.; Marsch, E.; Clúa de Gonzalez, A. L.: Interplanetary shock wave extent in the inner heliosphere as observed by multiple spacecraft. Journal of Atmospheric and Solar-Terrestrial Physics 73, pp. 1281 - 1292 (2011)
He, J.; Marsch, E.; Tu, C.; Yao, S.; Tian, H.: Possible evidence of Alfven-cyclotron waves in the angle distribution of magnetic helicity of solar wind turbulence. Astrophysical Journal 731, 85 (2011)
He, J.-S.; Marsch, E.; Tu, C.-Y.; Zong, Q.-G.; Yao, S.; Tian, H.: Two-dimensional correlation functions for density and magnetic field fluctuations in magnetosheath turbulence measured by the Cluster spacecraft. Journal Geophysical Research 116, A06207 (2011)
Hellinger, P.; Matteini, L.; Štverák, Š.; Trávníček, P. M.; Marsch, E.: Heating and cooling of protons in the fast solar wind between 0.3 and 1 AU: Helios revisited. Journal Geophysical Research 116, A09105 (2011)
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, ...
Two scientific associations have awarded Prof. Dr. Thorsten Kleine the title "Geochemistry Fellow" for his contributions to the understanding of how the Solar System was formed.
Call for applications: PhD positions in planetary science, solar physics, stellar physics, with a starting date in September 2024, at the IMPRS in Göttingen.
Application deadline 1 October 2023. PhD projects in planetary science, solar and stellar physics, solar magnetism, heliophysics, helioseismology, asteroseismology, ...
The MPS instruments on board ESA’s JUICE spacecraft have successfully completed their commissioning in space - and delivered their first observational data.