Gonzalez, W. D.; Joselyn, J. A.; Kamide, Y.; Kroehl, H. W.; Rostoker, G.; Tsurutani, B. T.; Vasyliūnas, V. M.: What is a geomagnetic storm? Journal Geophysical Research 99 (A4), pp. 5771 - 5792 (1994)
Vasyliūnas, V. M.: Role of the plasma acceleration time in the dynamics of the Jovian magnetosphere. Geophysical Research Letters 21, pp. 401 - 404 (1994)
Schreier, R.; Eviatar, A.; Vasyliūnas, V. M.; Richardson, J. D.: Modeling the Europa plasma torus. Journal Geophysical Research 98, pp. 21231 - 21243 (1993)
Lepping, R. P.; Burlaga, L. F.; Lazarus, A. J.; Vasyliūnas, V. M.; Szabo, A.; Steinberg, J.; Ness, N. F.; Krimigis, S. M.: Neptune's polar cusp region: Observations and magnetic field analysis. Journal Geophysical Research 97, pp. 8135 - 8144 (1992)
Frank, L. A.; Paterson, W. R.; Ackerson, K. L.; Coroniti, F. V.; Vasyliūnas, V. M.: Plasma observations at Venus with Galileo. Science 253, pp. 1528 - 1531 (1991)
Zhang, M.; Belcher, J. W.; Richardson, J. D.; Vasyliūnas, V. M.; Lepping, R. P.; Ness, N. F.; Smith, C. W.: Low-frequency waves in the solar wind near Neptune. Geophysical Research Letters 18, pp. 1071 - 1074 (1991)
Dessler, A. J.; Sandel, B. R.; Vasyliūnas, V. M.: Terrestrial cometary tail and lunar corona induced by small comets: Predictions for Galileo. Geophysical Research Letters 17, pp. 2257 - 2260 (1990)
Zhang, M.; Vasyliūnas, V. M.; Siscoe, G. L.; Lepping, R. P.; Ness, N. F.: Evidence for a diurnally rocking plasma mantle at Neptune. Geophysical Research Letters 17, pp. 2285 - 2288 (1990)
Vasyliūnas, V. M.: Maximum scales for preserving flux tube content in radial diffusion driven by interchange motions. Geophysical Research Letters 16, pp. 1465 - 1468 (1989)
Vasyliūnas, V. M.: Heat conduction limits on calorimetric effects at Mercury due to solar wind - magnetosphere interaction. Journal Geophysical Research 92, pp. 13658 - 13660 (1987)
Vasyliūnas, V. M.: Non-existence of gravitationally controlled partial corotation in cosmogonic plasmas. Geophysical Research Letters 14, pp. 171 - 173 (1987)
Vasyliūnas, V. M.: A method for evaluating the total magnetospheric energy output independently of the ε parameter. Geophysical Research Letters 14, pp. 1183 - 1186 (1987)
Bridge, H. S.; Belcher, J. W.; Coppi, B.; Lazarus, A. J.; McNutt Jr., R. L.; Olbert, S.; Richardson, J. D.; Sands, M. R.; Selesnick, R. S.; Sullivan, J. D.et al.; Hartle, R. F.; Ogilvie, K. W.; Sittler Jr., E. C.; Bagenal, F.; Wolff, R. S.; Vasyliūnas, V. M.; Siscoe, G. L.; Goertz, C. K.; Eviatar, A.: Plasma observations near Uranus: Initial results from Voyager 2. Science 233, pp. 89 - 93 (1986)
Kivelson, M. G.; Behannon, K. W.; Cravens, T. E.; de Pater, I.; Johnson, T. V.; Masursky, H.; Matson, D. L.; Southwood, D. J.; Vasyliūnas, V. M.: The giant planets and their satellites: Report on the COSPAR symposium, Ottawa, Canada, May 18-21, 1982. Advances in Space Research 3, pp. 5 - 14 (1983)
Bridge, H. S.; Bagenal, F.; Belcher, J. W.; Lazarus, A. J.; McNutt, R. L.; Sullivan, J. D.; Gazis, P. R.; Hartle, R. E.; Ogilvie, K. W.; Scudder, J. D.et al.; Sittler, E. C.; Eviatar, A.; Siscoe, G. L.; Goertz, C. K.; Vasyliūnas, V. M.: Plasma observations near Saturn: Initial results from Voyager 2. Science 215, pp. 563 - 570 (1982)
Vasyliūnas, V. M.; Kan, J. R.; Siscoe, G. L.; Akasofu, S.-I.: Scaling relations governing magnetospheric energy transfer. Planetary and Space Science 30, pp. 359 - 365 (1982)
Bridge, H. S.; Belcher, J. W.; Lazarus, A. J.; Olbert, S.; Sullivan, J. D.; Bagenal, F.; Gazis, P. R.; Hartle, R. E.; Ogilvie, K. W.; Scudder, J. D.et al.; Sittler, E. C.; Eviatar, A.; Siscoe, G. L.; Goertz, C. K.; Vasyliūnas, V. M.: Plasma observations near Saturn: Initial results from Voyager 1. Science 212, pp. 217 - 224 (1981)
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, ...