Kallenbach, R.; Bamert, K.; Hilchenbach, M.: Isotopic Composition of the Solar Wind Inferred from In-Situ Spacecraft Measurements. Space Science Reviews 130, pp. 173 - 182 (2007)
Czechowski, A.; Hilchenbach, M.; Hsieh, K. C.; Kallenbach, R.; Kota, J.: Estimating the thickness of the heliosheath from CELIAS/HSTOF and Voyager 1 data. Astrophysical Journal 647, pp. L69 - L72 (2006)
Klecker, B.; Möbius, E.; Popecki, M. A.; Kistler, L. M.; Kucharek, H.; Hilchenbach, M.: Observation of energy-dependent ionic charge states in impulsive solar energetic particle events. Advances in Space Research 38, pp. 493 - 497 (2006)
Czechowski, A.; Hilchenbach, M.; Hsieh, K. C.: Heliospheric energetic neutral atoms as a means to determine the anomalous cosmic ray spectrum at the termination shock. Astronomy and Astrophysics 431, pp. 1061 - 1068 (2005)
Kallenbach, R.; Hilchenbach, M.; Chalov, S. V.; Le Roux, J. A.; Bamert, K.: On the injection problem at the solar wind termination shock. Astronomy and Astrophysics 439, pp. 1 - 22 (2005)
Wilhelm, K.; Schühle, U.; Curdt, W.; Hilchenbach, M.; Marsch, E.; Lemaire, P.; Bertaux, J.-L.; Jordan, S. D.; Feldman, U.: On the nature of the unidentified solar emission near 117 nm. Astronomy and Astrophysics 439, pp. 701 - 711 (2005)
Bamert, K.; Wimmer-Schweingruber, R.; Kallenbach, R.; Hilchenbach, M.; Klecker, B.: Suprathermal ions of solar and interstellar origin associated with the April 912, 2001, CMEs. Advances in Space Research 34, pp. 161 - 165 (2004)
Czechowski, A.; Hsieh, K.; Hilchenbach, M.; Kota, J.; Shaw, A.: Anomalous helium ions as the source of energetic helium atoms in the outer heliosphere. Advances in Space Research 34, pp. 104 - 108 (2004)
Hsieh, K. C.; Zurbuchen, T. H.; Orr, J.; Gloeckler, G.; Hilchenbach, M.: A collimator design for monitoring heliospheric energetic neutral atoms at 1 AU. Advances in Space Research 34, pp. 213 - 218 (2004)
Kallenbach, R.; Bamert, K.; Wimmer-Schweingruber, R.; Klecker, B.; Hilchenbach, M.: Probing diffusion parameters of suprathermal ions near heliospheric shocks. Advances in Space Research 34, pp. 157 - 160 (2004)
Kucharek, H.; Möbius, E.; Li, W.; Farrugia, C. J.; Popecki, M. A.; Galvin, A. B.; Klecker, B.; Hilchenbach, M.; Bochsler, P.: On the source and acceleration of energetic He+. Journal Geophysical Research 108 (A10), 8040 (2003)
Bamert, K.; Wimmer-Schweingruber, R. F.; Kallenbach, R.; Hilchenbach, M.; Klecker, B.; Bogdanov, A.; Wurz, P.: Origin of the May 1998 suprathermal particles: Solar and Heliospheric Observatory/Charge, Element, and Isotope Analysis System Suprathermal Time of Flight results. Journal Geophysical Research 107 (A7), 1130 (2002)
Bogdanov, A. T.; Klecker, B.; Möbius, E.; Hilchenbach, M.; Popecki, M. A.; Kistler, L. M.; Hovestadt, D.: Observations of heavy ion charge spectra in CME driven gradual solar energetic particle events. Advances in Space Research 30 (1), pp. 111 - 117 (2002)
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.