Zhang, J.; Solanki, S. K.; Woch, J.: Discovery of inward moving magnetic enhancements in sunspot penumbrae. Astronomy and Astrophysics 475 (2), pp. 695 - 700 (2007)
Zhang, J.; Solanki, S. K.; Woch, J.; Wang, J.: The velocity structure of moving magnetic feature pairs around sunspots: Support for the U-loop model. Astronomy and Astrophysics 471, pp. 1035 - 1041 (2007)
Zhang, J.; Dere, K. P.; Howard, R. A.; Bothmer, V.: Identification of solar sources of major geomagnetic storms between 1996 and 2000. Astrophysical Journal 582 (1), pp. 520 - 533 (2003)
Zhang, J.; Solanki, S. K.; Wang, J.: On the nature of moving magnetic feature pairs around sunspots. Astronomy and Astrophysics 399, pp. 755 - 761 (2003)
Zhang, J.; Woch, J.; Solanki, S. K.; von Steiger, R.; Forsyth, R.: Interplanetary and solar surface properties of coronal holes obseved during solar maximum. Journal Geophysical Research 108 (A4), 1144 (2003)
Zhang, J.; Wang, J.: Are homologous flare-coronal mass ejection events triggered by moving magnetic features? Astrophysical Journal 566, pp. L117 - L120 (2002)
Zhang, J.; Woch, J.; Solanki, S. K.; von Steiger, R.: The Sun at solar minimum: North-south asymmetry of the polar coronal holes. Geophysical Research Letters 29 (8), 1236 (2002)
Various application review phases in 2025. PhD projects in cosmochemistry, planetary science, solar and stellar physics, helioseismology, asteroseismology, ...
The dwarf planet is a bizarre, cryovolcanic world. However, the organic deposits discovered on its surface so far are unlikely to originate from its interior.
The Uranian magnetic field is more expansive than previously thought, according to newly analyzed data from Voyager 2, making it easier to search for moons with oceans.