Cameron, R. H.; Jiang, J.; Schmitt, D.; Schüssler, M.: Surface flux transport modeling for solar cycles 15-21: effects of cycle-dependent tilt angles of sunspot groups. Astrophysical Journal 719, pp. 264 - 270 (2010)
Cameron, R. H.; Schüssler, M.: Changes of the solar meridional velocity profile during cycle 23 explained by flows towards the activity belts. Astrophysical Journal 720, pp. 1030 - 1032 (2010)
Cheung, M. C. M.; Rempel, M.; Title, A. M.; Schüssler, M.: Simulation of the formation of a solar active region. Astrophysical Journal 720, pp. 233 - 244, (2010)
Danilovic, S.; Beeck, B.; Pietarila, A.; Schüssler, M.; Solanki, S. K.; Martinez Pillet, V.; Bonet, J. A.; del Toro Iniesta, J. C.; Domingo, V.; Barthol, P.et al.; Berkefeld, T.; Gandorfer, A.; Knölker, M.; Schmidt, W.; Title, A. M.: Transverse Component of the Magnetic Field in the Solar Photosphere Observed by SUNRISE. Astrophysical Journal 723 (2), pp. L149 - L153 (2010)
Danilovic, S.; Schüssler, M.; Solanki, S. K.: Magnetic field intensification: comparison of 3D MHD simulations with Hinode/SP results. Astronomy and Astrophysics 509, A76 (2010)
Danilovic, S.; Schüssler, M.; Solanki, S. K.: Probing quiet Sun magnetism using MURaM simulations and Hinode/SP results: support for a local dynamo. Astronomy and Astrophysics 513, A1 (2010)
Jiang, J.; Işık, E.; Cameron, R. H.; Schmitt, D.; Schüssler, M.: The effect of activity-related meridional flow modulation on the strength of the solar polar magnetic field. Astrophysical Journal 717, pp. 597 - 602 (2010)
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Jiang, J.; Cameron, R.; Schmitt, D.; Schüssler, M.: Countercell Meridional Flow and Latitudinal Distribution of the Solar Polar Magnetic Field. Astrophysical Journal 693, pp. L96 - L99 (2009)
Pietarila Graham, J.; Danilovic, S.; Schüssler, M.: Turbulent magnetic fields in the quiet Sun: implications of Hinode observations and small-scale dynamo simulations. Astrophysical Journal 693, pp. 1728 - 1735 (2009)
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.