Kramar, M.; Inhester, B.; Solanki, S. K.: Vector tomography for the coronal magnetic field. I. Longitudinal Zeeman effect measurements. Astronomy and Astrophysics 456, pp. 665 - 673 (2006)
Loukitcheva, M.; Solanki, S. K.; White, S.: The dynamics of the solar chromosphere: comparison of model predictions with millimeter-interferometer observations. Astronomy and Astrophysics 456, pp. 713 - 723 (2006)
Raouafi, N.-E.; Solanki, S. K.: Sensitivity of solar off-limb line profiles to electron density stratification and the velocity distribution anisotropy. Astronomy and Astrophysics 445, pp. 735 - 745 (2006)
Sasso, C.; Lagg, A.; Solanki, S. K.: Milne-Eddington inversions of the He I 10 830 Å{} Stokes profiles: influence of the Paschen-Back effect. Astronomy and Astrophysics 456, pp. 367 - 371 (2006)
Sasso, C.; Lagg, A.; Solanki, S. K.; Socas-Navarro, H.: Influence of the Paschen-Back effect on the results of polarimetric inversions of the He I 10830 Å triplet. Memorie della Societa Astronomica Italiana Supplement 9, p. 126 (2006)
Selwa, M.; Solanki, S. K.; Murawski, K.; Wang, T. J.; Shumlak, U.: Numerical simulations of impulsively generated vertical oscillations in a solar coronal arcade loop. Astronomy and Astrophysics 454, pp. 653 - 661 (2006)
Tripathi, D.; Solanki, S. K.; Schwenn, R.; Bothmer, V.; Mierla, M.; Stenborg, G.: Observation of a bright coronal downflow by SOHO/EIT. Astronomy and Astrophysics 449, pp. 369 - 378 (2006)
Usoskin, I. G.; Solanki, S. K.; Korte, M.: Solar activity reconstructed over the last 7000 years: The influence of geomagnetic field changes. Geophysical Research Letters 33, L08103 (2006)
Usoskin, I. G.; Solanki, S. K.; Kovaltsov, G. A.; Beer, J.; Kromer, B.: Solar proton events in cosmogenic isotope data. Geophysical Research Letters 33, L08107 (2006)
Usoskin, I. G.; Solanki, S. K.; Taricco, C.; Bhandari, N.; Kovaltsov, G. A.: Long-term solar activity reconstructions: direct test by cosmogenic 44Ti in meteorites. Astronomy and Astrophysics 457, pp. L25 - L28 (2006)
Wang, T. J.; Innes, D. E.; Solanki, S. K.: Fe XIX observations of active region brightenings in the corona. Astronomy and Astrophysics 455, pp. 1105 - 1113 (2006)
Wenzler, T.; Solanki, S. K.; Krivova, N. A.; Fröhlich, C.: Reconstruction of solar irradiance variations in cycles 21-23 based on surface magnetic fields. Astronomy and Astrophysics 460, pp. 583 - 595 (2006)
White, S. M.; Loukitcheva, M.; Solanki, S. K.: High-resolution millimeter-interferometer observations of the solar chromosphere. Astronomy and Astrophysics 456, pp. 697 - 711 (2006)
Balmaceda, L.; Solanki, S. K.; Krivova, N.: A cross-calibrated sunspot areas time series since 1874. Memorie della Societa Astronomica Italiana 76, pp. 929 - 932 (2005)
Baumann, I.; Solanki, S. K.: On the size distribution of sunspot groups in the Greenwich sunspot record 1874-1976. Astronomy and Astrophysics 443, pp. 1061 - 1066 (2005)
Berdyugina, S. V.; Braun, P. A.; Fluri, D. M.; Solanki, S. K.: The molecular Zeeman effect and diagnostics of solar and stellar magnetic fields. III. Theoretical spectral patterns in the Paschen-Back regime. Astronomy and Astrophysics 444, pp. 947 - 960 (2005)
Borrero, J. M.; Lagg, A.; Solanki, S. K.; Collados, M.: On the fine structure of the sunspot penumbrae. II} The nature of the {Evershed flow. Astronomy and Astrophysics 436, pp. 333 - 345 (2005)
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.