Vasyliūnas, V. M.: Comparing Jupiter and Saturn: dimensionless input rates from plasma sources within the magnetosphere. Annales Geophysicae 26, pp. 1341 - 1343 (2008)
Vasyliūnas, V. M.: The mechanical advantage of the magnetosphere: solar-wind-related forces in the magnetosphere-ionosphere-Earth system. Annales Geophysicae 25, pp. 255 - 269 (2007)
Vasyliūnas, V. M.; Pontius Jr., D. H.: Rotationally driven interchange instability: Reply to André and Ferrière. Journal Geophysical Research 112, A10204 (2007)
Tsurutani, B. T.; Gonzalez, W. D.; Gonzalez, A. L. C.; Guarnieri, F. L.; Gopalswamy, N.; Grande, M.; Kamide, Y.; Kasahara, Y.; Lu, G.; Mann, I.et al.; McPherron, R.; Søraas, F.; Vasyliūnas, V. M.: Corotating solar wind streams and recurrent geomagnetic activity: A review. Journal Geophysical Research 111, A07S01 (2006)
Vasyliūnas, V. M.: Ionospheric and boundary contributions to the Dessler-Parker-Sckopke formula for Dst. Annales Geophysicae 24, pp. 1085 - 1097 (2006)
Luhmann, J. G.; Curtis, D. W.; Lin, R. P.; Larson, D.; Schroeder, P.; Cummings, A.; Mewaldt, R. A.; Stone, E. C.; Davis, A.; von Rosenvinge, T.et al.; Acuna, M. H.; Reames, D.; Ng, C.; Ogilvie, K.; Mueller-Mellin, R.; Kunow, H.; Mason, G. M.; Wiedenbeck, M.; Sauvaud, A.; Aoustin, C.; Louarn, P.; Dandouras, J.; Korth, A.; Bothmer, V.; Vasyliūnas, V.; Sanderson, T.; Marsden, R. G.; Russell, C. T.; Gosling, J. T.; Bougeret, J. L.; McComas, D. J.; Linker, J. A.; Riley, P.; Odstrcil, D.; Pizzo, V. J.; Gombosi, T.; DeZeeuw, D.; Kecskemety, K.: IMPACT: Science goals and firsts with STEREO. Advances in Space Research 36, pp. 1534 - 1543 (2005)
Song, P.; Vasyliūnas, V. M.; Ma, L.: Solar wind-magnetosphere-ionosphere coupling: Neutral atmosphere effects on signal propagation. Journal Geophysical Research 110, A09309 (2005)
Reinisch, B. W.; Huang, X.; Song, P.; Green, J. L.; Fung, S. F.; Vasyliūnas, V. M.; Gallagher, D. L.; Sandel, B. R.: Plasmaspheric mass loss and refilling as a result of a magnetic storm. Journal Geophysical Research 109 (A1), A01202 (2004)
Vasyliūnas, V. M.: Comment on `The superposition of rotating and stationary magnetic sources: implications for the auroral region' [Phys. Plasmas 10, 2971 (2003)]. Physics of Plasmas 11, pp. 1738 - 1739 (2004)
Nsumei, P. A.; Huang, X.; Reinisch, B. W.; Song, P.; Vasyliūnas, V. M.; Green, J. L.; Fung, S. F.; Benson, R. F.; Gallagher, D. L.: Electron density distribution over the northern polar region deduced from IMAGE/radio plasma imager sounding. Journal Geophysical Research 108 (A2), 1078 (2003)
Jurac, S.; McGrath, M. A.; Johnson, R. E.; Richardson, J. D.; Vasyliūnas, V. M.; Eviatar, A.: Saturn: Search for a missing water source. Geophysical Research Letters 29 (24), 2172 (2002)
Song, P.; Vasyliūnas, V. M.: Solar Wind - Magnetosphere - Ionosphere Coupling: Signal Arrival Time and Perturbation Relations. Journal Geophysical Research 107 (A11), 1358 (2002)
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, ...