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)
Frutiger, C.; Solanki, S. K.; Mathys, G.: Fundamental parameters and granulation properties of Alpha Centauri A and B obtained from inversions of their spectra. Astronomy and Astrophysics 444 (2), pp. 549 - 559 (2005)
Khomenko, E. V.; Martinez Gonzalez, M. J.; Collados, M.; Vögler, A.; Solanki, S. K.; Ruiz Cobo, B.; Beck, C.: Magnetic flux in the internetwork quiet Sun. Astronomy and Astrophysics 436, pp. L27 - L30 (2005)
Khomenko, E. V.; Shelyag, S.; Solanki, S. K.; Vögler, A.: Stokes diagnostics of simulations of magnetoconvection of mixed-polarity quiet-Sun regions. Astronomy and Astrophysics 442, pp. 1059 - 1078 (2005)
Krivova, N. A.; Solanki, S. K.: Modelling of irradiance variations through atmosphere models. Memorie della Societa Astronomica Italiana 76, pp. 834 - 841 (2005)
Images from ESA’s Solar Orbiter offer the best look yet at a source region of the solar wind - and challenge our view of the continuous particle stream from the Sun.
Deciphering the magnetic origins of the Sun's hot corona: developing a framework for coronal heating by probing the elusive photosphere-corona connection
Using unique observational data and computer simulations, the MPS scientist is striving to understand the incredibly hot temperatures in the solar corona.
For the first time, images of the Sun have been taken from a distance of only 77 million kilometres enabling a completely new view of our star possible.
In his doctoral thesis, Sudip Mandal investigated how special pressure waves help maintain temperatures of several million degrees in the outermost solar atmosphere.