Nagy, A. F.; Winterhalter, D.; Sauer, K.; Cravens, T. E.; Brecht, S.; Mazelle, C.; Crider, D.; Kallio, E.; Zakharov, A.; Dubinin, E.et al.; Verigin, M.; Kotova, G.; Axford, W. I.; Bertucci, C.; Trotignon, J. G.: The plasma environment of Mars. Space Science Reviews 111 (1-2), pp. 33 - 114 (2004)
Florinski, V.; Zank, G. P.; Axford, W. I.: The solar system in a dense interstellar cloud: Implications for cosmic-ray fluxes at Earth and 10Be records. Geophysical Research Letters 30 (23), 2206 (2003)
Trotignon, J. G.; Parrot, M.; Cerisier, J. C.; Menvielle, M.; Axford, W. I.; Pätzold, M.; Warnant, R.; Wernik, A. W.: The plasma environment of Mars: from the shocked solar wind down to the ionosphere. Planetary and Space Science 48, pp. 1181 - 1191 (2000)
Axford, W. I.; McKenzie, J. F.; Sukhorukova, G. V.; Banaszkiewicz, M.; Czechowski, A.; Ratkiewicz, R.: Acceleration of the high speed solar wind in coronal holes. Space Science Reviews 87, pp. 25 - 41 (1999)
Krymskii, A. M.; Breus, T. K.; Axford, W. I.: Sources of heavy ions in the Venusian magnetosheath and their role in solar wind loading processes. Cosmic Research 37 (4), pp. 360 - 368 (1999)
Lieu, R.; Ip, W.-H.; Axford, W. I.; Bonamente, M.: Nonthermal origin of the EUV and soft X-rays from the Coma Cluster: Cosmic rays in equipartition with the thermal medium. Astrophys. J. Let. 510, pp. L25 - L28 (1999)
McKenzie, J. F.; Sukhorukova, G. V.; Axford, W. I.: The temperature and density structure in the closed field regions of the solar corona. Astronomy and Astrophysics 350, pp. 1035 - 1039 (1999)
Shukla, P. K.; Bingham, R.; McKenzie, J. F.; Axford, W. I.: Solar coronal heating by high-frequency dispersive Alfvén waves. Solar Physics 186, pp. 61 - 66 (1999)
Aellig, M. R.; Grünwaldt, H.; Bochsler, P.; Wurz, P.; Hefti, S.; Kallenbach, R.; Ipavich, F. M.; Axford, W. I.; Balsiger, H.; Bürgi, A.et al.; Coplan, M. A.; Galvin, A. B.; Geiss, J.; Gliem, F.; Gloeckler, G.; Hilchenbach, M.; Hovestadt, D.; Hsieh, K. C.; Klecker, B.; Lee, M. A.; Livi, S.; Managadze, G. G.; Marsch, E.; Möbius, E.; Neugebauer, M.; Reiche, K.-U.; Scholer, M.; Verigin, M. I.; Wilken, B.: Iron freeze-in temperatures measured by SOHO/CELIAS/CTOF. Journal Geophysical Research 103, pp. 17215 - 17222 (1998)
Axford, W. I.; Marsch, E.; Oraevsky, V. N.; Kuznetsov, V. D.; Breus, T. K.; Schwenn, R.; Ip, W.-H.; Ksanfomality, L. V.; Thomas, N.; Kogan, A.et al.; Utkin, V. F.; Uspensky, G. R.: Space mission for exploration of the Sun, Mercury and inner heliosphere (``InterHelios''). Advances in Space Research 21, pp. 275 - 289 (1998)
Breus, T. K.; Pimenov, K. Y.; Luhmann, J. G.; Krymskii, A. M.; Hagfors, T.; Axford, W. I.; Kliore, A. J.: Application of Viking radio occultation data to the future studies of the Martian ionosphere. Advances in Space Research 22, pp. 463 - 470 (1998)
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, ...