Hamilton, D. C.; Brown, D. C.; Gloeckler, G.; Axford, W. I.: Energetic atomic and molecular ions in Saturn's magnetosphere. Journal Geophysical Research 88, pp. 8905 - 8922 (1983)
McKenzie, J. F.; Axford, W. I.: Comment on 'On rotational forces in the solar wind' by J. V. Hollweg and P. A. Isenberg. Journal Geophysical Research 88, pp. 7251 - 7252 (1983)
Webb, G.; Axford, W. I.; Terasawa, T.: On the drift mechanism for energetic charged particles at shocks. Astrophysical Journal 270, pp. 537 - 553 (1983)
Krimigis, S. M.; Armstrong, T. P.; Axford, W. I.; Bostrom, C. O.; Gloeckler, G.; Keath, E. P.; Lanzerotti, L. J.; Carbary, J. F.; Hamilton, D. C.; Roelof, E. C.: Low energy hot plasma and particles in Saturn's magnetosphere. Science 215, pp. 571 - 577 (1982)
Carbary, J. F.; Krimigis, S. M.; Keath, E. P.; Gloeckler, G.; Axford, W. I.; Armstrong, T. P.: Ion anisotropies in the outer Jovian magnetosphere. Journal Geophysical Research 86, pp. 8285 - 8299 (1981)
Krimigis, S. M.; Armstrong, T. P.; Axford, W. I.; Bostrom, C. O.; Gloeckler, G.; Keath, E. P.; Lanzerotti, L. J.; Carbary, J. F.; Hamilton, D. C.; Roelof, E. C.: Low-energy charged particles in Saturn's magnetosphere: Results form Voyager 1. Science 212, pp. 225 - 231 (1981)
Krimigis, S. M.; Carbary, J. F.; Keath, E. P.; Bostrom, C. O.; Axford, W. I.; Gloeckler, G.; Lanzerotti, L. J.; Armstrong, T. P.: Characteristics of hot plasma in the Jovian magnetosphere: Results from the Voyager spacecraft. Journal Geophysical Research 86, pp. 8227 - 8257 (1981)
Hamilton, D. C.; Gloeckler, G.; Krimigis, S. M.; Bostrom, C. O.; Armstrong, T. P.; Axford, W. I.; Fan, C. Y.; Lanzerotti, L. J.; Hunten, D. M.: Detection of energetic hydrogen molecules in Jupiter's magnetosphere by Voyager 2: Evidence for an ionospheric plasma source. Geophysical Research Letters 7, pp. 813 - 816 (1980)
Krimigis, S. M.; Armstrong, T. P.; Axford, W. I.; Bostrom, C. O.; Fan, C. Y.; Gloeckler, G.; Lanzerotti, L. J.; Hamilton, D. C.; Zwickl, R. D.: Energetic (∼ 100 keV) tailward-directed ion beam outside the Jovian plasma boundary. Geophysical Research Letters 7, pp. 13 - 16 (1980)
Krimigis, S. M.; Armstrong, T. P.; Axford, W. I.; Bostrom, C. O.; Fan, C. Y.; Gloeckler, G.; Lanzerotti, L. J.; Keath, E. P.; Zwickl, R. D.; Carbary, J. F.et al.; Hamilton, D. C.: Low-energy charged particle environment at Jupiter: A first look. Science 204, pp. 998 - 1003 (1979)
Krimigis, S. M.; Armstrong, T. P.; Axford, W. I.; Bostrom, C. O.; Fan, C. Y.; Gloeckler, G.; Lanzerotti, L. J.; Keath, E. P.; Zwickl, R. D.; Carbary, J. F.et al.; Hamilton, D. C.: Hot plasma environment at Jupiter: Voyager 2 results. Science 206, pp. 977 - 984 (1979)
Lanzerotti, L. J.; Krimigis, S. M.; Bostrom, C. O.; Axford, W. I.; Lepping, R. P.; Ness, N. F.: Measurements of plasma flow at the dawn magnetopause by Voyager 1. Journal Geophysical Research 84, pp. 6483 - 6488 (1979)
McKenzie, J. F.; Ip, W.-H.; Axford, W. I.: The acceleration of minor ion species in the solar wind. Astrophys. and Space Phys. 64, pp. 183 - 211 (1979)
Richter, A. K.; Keppler, E.; Axford, W. I.; Denskat, K. U.: Dynamics of low-energy electrons (gt; 17 keV) and ions (gt; 80 keV) in the vicinity of the low-latitude, duskside magnetopause: Helios 1 and 2 observations. Journal Geophysical Research 84, pp. 1453 - 1463 (1979)
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, ...