Štverák, Š.; Trávníček, P.; Maksimovic, M.; Marsch, E.; Fazakerley, A. N.; Scime, E. E.: Electron temperature anisotropy constraints in the solar wind. Journal Geophysical Research 113, A03103 (2008)
Tian, H.; Marsch, E.; Tu, C.-Y.; Xia, L.-D.; He, J.-S.: Sizes of transition-region structures in coronal holes and in the quiet Sun. Astronomy and Astrophysics 482, pp. 267 - 272 (2008)
Tu, C.-Y.; Schwenn, R.; Donovan, E.; Marsch, E.; Wang, J.-S.; Xia, L.-D.; Zhang, Y.-W.; the working team, K.: Space weather explorer - The KuaFu mission. Advances in Space Research 41, pp. 190 - 209 (2008)
Marsch, E.: The radial wavefunction of a relativistic binary of two fermions bound by the Coulomb force. Annalen der Physik 16 (7-8), pp. 553 - 562 (2007)
Matteini, L.; Landi, S.; Hellinger, P.; Pantellini, F.; Maksimovic, M.; Velli, M.; Goldstein, B. E.; Marsch, E.: Evolution of the solar wind proton temperature anisotropy from 0.3 to 2.5 AU. Geophysical Research Letters 34, L20105 (2007)
Tian, H.; Tu, C.-Y.; He, J.-S.; Marsch, E.: Emission heights of coronal bright points on Fe XII radiance map. Advances in Space Research 39, pp. 1853 - 1859 (2007)
Wilhelm, K.; Marsch, E.; Dwivedi, B. N.; Feldman, U.: Observations of the Sun at Vacuum-Ultraviolet Wavelengths from Space. Part II: Results and Interpretations. Space Science Reviews 133, pp. 103 - 179 (2007)
Zhou, G.-Q.; He, J.-S.; Tu, C.-Y.; Marsch, E.: Correlation Height of the Source Region of Si II Emission Lines in Coronal Hole Regions. Chinese Astronomy and Astrophysics 31, pp. 137 - 145 (2007)
Boswell, R. W.; Marsch, E.; Charles, C.: The current-free electric double layer in a coronal magnetic funnel. Astrophysical Journal 640, pp. L199 - L202 (2006)
Marsch, E.: Addendum and erratum, The relativistic energy spectrum of hydrogen [Ann.Phys.(Leipzig) 14, 324(2005)]. Annalen der Physik 15 (6), pp. 434 - 437 (2006)
Marsch, E.; Zhou, G.-Q.; He, J.-S.; Tu, C.-Y.: Magnetic structure of the solar transition region as observed in various ultraviolet lines emitted at different temperatures. Astronomy and Astrophysics 457, pp. 699 - 706 (2006)
The Uranian magnetic field is more expansive than previously thought, according to newly analyzed data from Voyager 2, making it easier to search for moons with oceans.
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).