He, J.; Marsch, E.; Tu, C.; Yao, S.; Tian, H.: Possible evidence of Alfven-cyclotron waves in the angle distribution of magnetic helicity of solar wind turbulence. Astrophysical Journal 731, 85 (2011)
He, J.-S.; Marsch, E.; Tu, C.-Y.; Zong, Q.-G.; Yao, S.; Tian, H.: Two-dimensional correlation functions for density and magnetic field fluctuations in magnetosheath turbulence measured by the Cluster spacecraft. Journal Geophysical Research 116, A06207 (2011)
Guo, L.-J.; Tian, H.; He, J.-S.: Quasi-periodic outflows observed by the X-Ray Telescope onboard Hinode in the boundary of an active region. Res. Astron. Astrophys. 10 (12), pp. 1307 - 1314 (2010)
He, J.-S.; Marsch, E.; Tu, C.-Y.; Guo, L.-J.; Tian, H.: Intermittent outflows at the edge of an active region - a possible source of the solar wind? Astronomy and Astrophysics 516, A14 (2010)
He, J.-S.; Tu, C.-Y.; Tian, H.; Marsch, E.: Solar wind origins in coronal holes and in the quiet Sun. Advances in Space Research 45, pp. 303 - 309 (2010)
Tian, H.; Marsch, E.; Tu, C.; Curdt, W.; He, J.: New views on the emission and structure of the solar transition region. New Astron. Rev. 54, pp. 13 - 30 (2010)
Tian, H.; Tu, C.; Marsch, E.; He, J.; Kamio, S.: The nascent fast solar wind observed by the EUV imaging spectrometer on board Hinode. Astrophysical Journal 709, pp. L88 - L93 (2010)
He, J.; Marsch, E.; Tu, C.; Tian, H.: Excitation of kink waves due to small-scale magnetic reconnection in the chromosphere? Astrophysical Journal 705, pp. L217 - L222 (2009)
He, J.-S.; Marsch, E.; Tu, C.-Y.; Tian, H.: Upward and downward propagation of transverse waves due to small-scale magnetic reconnection in the chromosphere. In: Twelfth International Solar Wind Conference, pp. 32 - 35 (Eds. Maksimovic, M.; Issautier, K.; Meyer-Vernet, N.; Moncuquet, M.; Pantellini, F.). American Institute of Physics (2010)
Tian, H.; Tu, C.-Y.; Marsch, E.; He, J.-S.; Zhou, C.; Zhao, L.: Upflows in the upper transition region of the quiet Sun. In: Twelfth International Solar Wind Conference, pp. 36 - 39 (Eds. Maksimovic, M.; Issautier, K.; Meyer-Vernet, N.; Moncuquet, M.; Pantellini, F.). American Institute of Physics (2010)
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, ...