Baumann, I.; Schmitt, D.; Schüssler, M.: A necessary extension of the flux transport model. Memorie della Societa Astronomica Italiana 76, pp. 933 - 936 (2005)
Usoskin, I. G.; Schüssler, M.; Solanki, S. K.; Mursula, K.: Solar activity, cosmic rays and Earth's temperature: A millenium-scale comparison. Journal Geophysical Research 110, p. A10102 (2005)
Vögler, A.; Shelyag, S.; Schüssler, M.; Cattaneo, F.; Emonet, T.; Linde, T.: Simulations of magneto-convection in the solar photosphere: Equations, methods and results of the MURaM code. Astronomy and Astrophysics 429, pp. 335 - 351 (2005)
Baumann, I.; Schmitt, D.; Schüssler, M.; Solanki, S. K.: Evolution of the large-scale magnetic field on the solar surface: a parameter study. Astronomy and Astrophysics 426, pp. 1075 - 1091 (2004)
Cameron, R.; Schüssler, M.; Vögler, A.: The Sun - a ball of electrically well-conducting gas. inSIDE - Innovatives Supercomputing 2 (1), pp. 4 - 5 (2004)
Kolesnikov, F.; Bünte, M.; Schmitt, D.; Schüssler, M.: Kelvin-Helmholtz and shear instability of a helical flow around a magnetic flux tube. Astronomy and Astrophysics 420 (2), pp. 737 - 749 (2004)
Preuss, O.; Schüssler, M.; Holzwarth, V.; Solanki, S. K.: Distribution of magnetically confined circumstellar matter in oblique rotators. Astronomy and Astrophysics 417, pp. 987 - 992 (2004)
Shelyag, S.; Schüssler, M.; Solanki, S. K.; Berdyugina, S.; Vögler, A.: G-band spectral synthesis and diagnostics of simulated solar magneto-convection. Astronomy and Astrophysics 427, pp. 335 - 343 (2004)
Solanki, S. K.; Usoskin, I. G.; Kromer, B.; Schüssler, M.; Beer, J.: Unusual activity of the Sun during recent decades compared to the previous 11,000 years. Nature 431 (7012), pp. 1084 - 1087 (2004)
Usoskin, I. G.; Mursula, K.; Solanki, S. K.; Schüssler, M.; Alanko, K.: Reconstruction of solar activity for the last millenium using 10Be data. Astronomy and Astrophysics 413, pp. 745 - 751 (2004)
Analyzing the high spatial resolution solar Ca II H and K emission data obtained by the SUNRISE mission and building a model of other stars more active than the Sun
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).
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.