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)
Curdt, W.; Tian, H.; Teriaca, L.; Schühle, U.; Lemaire, P.: The Ly-α profile and center-to-limb variation of the quiet Sun. Astronomy and Astrophysics 492, pp. L9 - L12 (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)
Teriaca, L.; Curdt, W.; Solanki, S. K.: SUMER observations of the inverse Evershed effect in the transition region above a sunspot. Astronomy and Astrophysics 491, pp. L5 - L8 (2008)
Wilhelm, K.; Curdt, W.; Dammasch, I. E.; Hassler, D. M.: Comment on ``Energy levels and spectral lines of NeVIII''. Eur. Phys. J. D 47 (3), p. 325 - 325 (2008)
Fontenla, J. M.; Curdt, W.; Avrett, E. H.; Harder, J.: Log-normal intensity distribution of the quiet-Sun FUV continuum observed by SUMER. Astronomy and Astrophysics 468, pp. 695 - 699 (2007)
Madjarska, M. S.; Doyle, J. G.; Innes, D. E.; Curdt, W.: Jets or High-Velocity Flows Revealed in High-Cadence Spectrometer and Imager Co-observations? Astrophysical Journal 670, pp. L57 - L60 (2007)
McIntosh, S. W.; Davey, A. R.; Hassler, D. M.; Armstrong, J. D.; Curdt, W.; Wilhelm, K.; Lin, G.: Observations supporting the role of magnetoconvection in energy supply to the quiescent solar atmosphere. Astrophysical Journal 654, pp. 650 - 664 (2007)
Emerich, C.; Lemaire, P.; Vial, J.-C.; Curdt, W.; Schühle, U.; Wilhelm, K.: A new relation between the central spectral solar H I Lyman α irradiance and the line irradiance measured by SUMER/SOHO during the cycle 23. Icarus 178, pp. 429 - 433 (2005)
Gömöry, P.; Rybak, J.; Kucera, A.; Curdt, W.; Wöhl, H.: Variability and dynamics of the outer atmospheric layers in the quiet solar network. Hvar Obs. Bull. 29, pp. 71 - 78 (2005)
Lemaire, P.; Emerich, C.; Vial, J.-C.; Curdt, W.; Schühle, U.; Wilhelm, K.: Variation of the full Sun hydrogen Lyman profiles through solar cycle 23. Advances in Space Research 35, pp. 384 - 387 (2005)
The dwarf planet is a bizarre, cryovolcanic world. However, the organic deposits discovered on its surface so far are unlikely to originate from its interior.
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).