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)
Vögler, A.: On the effect of photospheric magnetic fields on solar surface brightness: Results of radiative MHD simulations. Memorie della Societa Astronomica Italiana 76, pp. 842 - 849 (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)
Cameron, R.; Schüssler, M.; Vögler, A.: The Sun - a ball of electrically well-conducting gas. inSIDE - Innovatives Supercomputing 2 (1), pp. 4 - 5 (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)
Vögler, A.; Bruls, J. H. M. J.; Schüssler, M.: Approximations for non-grey radiative transfer in numerical simulations of the solar photosphere. Astronomy and Astrophysics 421, pp. 741 - 754 (2004)
Janßen, K.; Vögler, A.; Kneer, F.: On the fractal dimension of small-scale magnetic structures in the Sun. Astronomy and Astrophysics 409, pp. 1127 - 1134 (2003)
Schüssler, M.; Shelyag, S.; Berdyugina, S.; Vögler, A.; Solanki, S. K.: Why solar magnetic flux concentrations are bright in molecular bands. Astrophysical Journal 597, pp. L173 - L176 (2003)
Vögler, A.; Schmitt, D.: Generation of bisymmetric magnetic fields in galaxies with tidal interaction. Astronomy and Astrophysics 374, pp. 36 - 41 (2001)
Schüssler, M.; Bruls, J. H. M. J.; Vögler, A.; Vollmöller, P.: Simulation of solar radiative magneto-convection. In: Analysis and Numerics for Conservation Laws, pp. 107 - 136 (Ed. Warnecke, G.). Springer Verlag, Berlin (2005)
Cameron, R.; Vögler, A.; Schüssler, M.: Simulation of solar magneto-convection. In: High Performance Computing in Science and Engineering: Transactions of the Second Joint HLRB and KONWIHR Result and Reviewing Workshop, pp. 431 - 442 (Eds. Wagner, S.; Hanke, W.; Bode, A.; Durst, F.). Springer, Berlin (2004)
Cameron, R.; Vögler, A.; Schüssler, M.; Zakharov, V.: Simulations of solar pores. In: Proceedings of the 11th European Solar Physics Meeting - The Dynamic Sun: Challenges for Theory and Observations, 11-16 September 2005 (Eds. Danesy, D.; Poedts, S.; De Groof, A.; Andries, J.). ESA Publ. Div., Noordwijk (2005)
First Light! The spectro-polarimeter of the world's largest solar telescope in Hawaii looks at the Sun for the first time. The instrument was developed in Germany.
Dr. Theodosios Chatzistergos receives award by the European Space Weather and Space Climate Association for his research findings on the historical activity of the Sun.
The Zdenĕk Švetska Senior Prize of the Solar Physics Division of the European Physical Society (EPS) recognizes Solanki’s pioneering contributions to solar research.
The magnetic field in the solar atmosphere exceeds the geomagnetic field strength by four orders of magnitude. It greatly influences the processes of energy transport within the solar atmosphere, and dominates the morphology of the solar chromosphere and corona. Kinetic energy from convective motions in the Sun can be efficiently stored in magnetic fields and subsequently released - to heat the solar corona to several million degrees or to blast off coronal mass ejections.
Application deadline 1 October 2024. PhD projects in planetary science, solar and stellar physics, solar magnetism, heliophysics, helioseismology, asteroseismology, ...