Preuss, O.; Solanki, S. K.; Haugan, M. P.; Jordan, S.: Gravity-induced birefringence within the framework of Poincaré gauge theory. Physical Review D 72, p. 042001 (2005)
Selwa, M.; Murawski, K.; Solanki, S. K.: Excitation and damping of slow magnetosonic standing waves in a solar coronal loop. Astronomy and Astrophysics 436, pp. 701 - 709 (2005)
Selwa, M.; Murawski, K.; Solanki, S. K.; Wang, T. J.; Tóth, G.: Numerical simulations of vertical oscillations of a solar coronal loop. Astronomy and Astrophysics 440, pp. 385 - 390 (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)
Wenzler, T.; Solanki, S. K.; Krivova, N. A.: Can surface magnetic fields reproduce solar irradiance variations in cycles 22 and 23? Astronomy and Astrophysics 432, pp. 1057 - 1061 (2005)
Zakharov, V.; Gandorfer, A.; Solanki, S. K.; Löfdahl, M.: A comparative study of the contrast of solar magnetic elements in CN and CH. Astronomy and Astrophysics 437, pp. L43 - L46 (2005)
Aznar Cuadrado, R.; Jordan, S.; Napiwotzki, R.; Schmid, H. M.; Solanki, S. K.; Mathys, G.: Discovery of kilogauss magnetic fields in three DA white dwarfs. Astronomy and Astrophysics 423, pp. 1081 - 1094 (2004)
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)
Borrero, J. M.; Solanki, S. K.; Bellot Rubio, L. R.; Lagg, A.; Mathew, S. K.: On the fine structure of sunspot penumbrae - I. A quantitative comparison of two semiempirical models with implications for the Evershed effect. Astronomy and Astrophysics 422, pp. 1093 - 1104 (2004)
Bruls, J. H. M. J.; Solanki, S. K.: Apparent solar radius variations - The influence of magnetic network and plage. Astronomy and Astrophysics 427 (2), pp. 735 - 743 (2004)
Krivov, A. V.; Krivova, N. A.; Solanki, S. K.; Titov, V. B.: Towards understanding the β Pictoris dust stream. Astronomy and Astrophysics 417, pp. 341 - 352 (2004)
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.