Rinnert, K.; Lanzerotti, L. J.; Krider, E. P.; Uman, M. A.; Dehmel, G.; Gliem, F. O.; Axford, W. I.: Electromagnetic noise and radio wave propagation below 100 kHz in the Jovian magnetosphere, 1. The equatorial region. Journal Geophysical Research 84, pp. 5181 - 5188 (1979)
Ip, W.-H.; Fillius, W.; Mogro-Campero, A.; Gleeson, L. J.; Axford, W. I.: Quiet-time interplanetary cosmic ray anisotropies observed from Pioneer 10 and 11. Journal Geophysical Research 83, pp. 1633 - 1640 (1978)
Krimigis, S. M.; Armstrong, T. P.; Axford, W. I.; Bostrom, C. O.; Fan, C. Y.; Gloeckler, G.; Lanzerotti, L. J.: The low energy charged particle (LECP) experiment on the Voyager spacecraft. Space Science Reviews 21, pp. 329 - 354 (1977)
Lee, H.-J.; McKenzie, J. F.; Axford, W. I.: Discontinuous transitions in a current-carrying plasma. Astrophysics and Space Science 51, pp. 3 - 32 (1977)
Messinger, H. F.; Greenstadt, E. W.; Axford, W. I.; Wetherill, G. W.: Comet exploration: Scientific objectives and mission strategy for a rendezvous with Encke. Progress in Astronautics and Aeronautics 50, pp. 209 - 236 (1977)
Axford, W. I.; Fillius, W.; Gleeson, L. J.; Ip, W.-H.: Cosmic-ray gradients from Pioneer-10 and Pioneer-11. Astrophysical Journal 210, pp. 603 - 613 (1976)
Gleeson, L. J.; Axford, W. I.: An analytic model illustrating the effects of rotation on a magnetosphere containing low-energy plasma. Journal Geophysical Research 81, pp. 3403 - 3406 (1976)
Marsch, E.; Axford, W. I.; McKenzie, J. F.: Solar Wind. In: The Dynamic Sun, pp. 374 - 402 (Ed. Dwivedi, B.). Cambridge University Press, Cambridge (2003)
Axford, W. I.: COSPAR during the period 1986-1994. In: 40 Years of COSPAR, pp. 131 - 137 (Eds. Haerendel, G.; Grzedzielski, S.; Cavallo, G.; Battrick, B.). ESA Publ. Div., Noordwijk (1998)
Axford, W. I.; Suess, S. T.: The outer heliosphere. In: From the Sun: Auroras, Magnetic Storms, Solar Flares, Cosmic Rays, pp. 143 - 152 (Eds. Suess, S. T.; Tsurutani, B. T.). American Geophysical Union, Washington D. C. (1998)
Axford, W. I.; McKenzie, J. F.: Acceleration of the high speed solar wind. In: Magnetodynamic Phenomena in the Solar Atmosphere-Prototypes of Stellar Magnetic Activity, pp. 115 - 122 (Eds. Uchida, Y.; Kosugi, T.; Hudson, H. S.). Kluwer, Dordrecht (1996)
Axford, W. I.: Magnetospheres of the earth and planets. In: Encyclopedia of Applied Physics, pp. 187 - 205 (Ed. Trigg, G. L.). VCH Publ. Inc., New York (1994)
Axford, W. I.; Breus, T. K.: Scenario of solar wind interaction with Venus and Mars. In: Plasma Environments of Non-Magnetic Planets (Proc. 4th COSPAR Colloquium, Ann Arbor, U. S. A., 1992), pp. 207 - 216 (Ed. Gombosi, T. I.). Pergamon Press, Oxford (1993)
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, ...