Woodward, T.; McKenzie, J. F.: Stationary MHD waves modified by Hall current coupling-I. Cold compressible flow. Planetary and Space Science 42, pp. 463 - 479 (1994)
Woodward, T.; McKenzie, J. F.: Stationary MHD waves modified by Hall current coupling-II. Incompressible flow. Planetary and Space Science 42, pp. 481 - 489 (1994)
McKenzie, J. F.; Marsch, E.; Baumgärtel, K.; Sauer, K.: Wave and stability properties of multi-ion plasmas with application to winds and flows. Annales Geophysicae 11, pp. 341 - 353 (1993)
Gloeckler, G.; Geiss, J.; Balsiger, H.; Bedini, P.; Cain, J. C.; Fisher, J.; Fisk, L. A.; Galvin, A. B.; Gliem, F.; Hamilton, D. C.et al.; Hollweg, J. V.; Ipavich, F. M.; Joos, R.; Livi, S.; Lundgren, R.; Mall, U.; McKenzie, J. F.; Ogilvie, K. W.; Ottens, F.; Rieck, W.; Tums, E. O.; von Steiger, R.; Weiss, W.; Wilken, B.: The solar wind ion composition spectrometer. Astronomy and Astrophysics, Suppl. Ser. 92, pp. 267 - 289 (1992)
Sauer, K.; Roatsch, T.; Baumgärtel, K.; McKenzie, J. F.: Critical density layer as obstacle at solar wind - exosphere interaction. Geophysical Research Letters 19, pp. 645 - 648 (1992)
McKenzie, J. F.; Ershkovich, A. I.; Axford, W. I.: Stability of a cometary ionosphere/ionopause including pressure effects. Astrophysical Journal 360, pp. 275 - 278 (1990)
Ershkovich, A. I.; McKenzie, J. F.; Axford, W. I.: Stability of a cometary ionosphere/ionopause determinated by ion-neutral friction. Astrophysical Journal 344, pp. 932 - 939 (1989)
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)
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)
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)
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.; 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)
Sauer, K.; Baumgärtel, K.; Roatsch, T.; McKenzie, J. F.: Laval nozzle effects in solar wind - exosphere interaction. In: Geographical Monograph ``Space Plasmas: coupling between small and medium scale processes'', pp. 43 - 47 (Eds. Ashour-Abdalla, M.; Chang, T.; Dusenbery, P.). American Geophysical Union, Washington, D. C., USA (1995)
Axford, W. I.; McKenzie, J. F.: The origin of high speed solar wind streams. In: Solar Wind Seven (Proc. 3rd COSPAR Colloquium, Goslar, Germany 16-20 September 1991), pp. 1 - 5 (Eds. Marsch, E.; Schwenn, R.). Pergamon Press, Oxford (1992)
Webb, G. M.; McKenzie, J. F.; Dubinin, E.; Sauer, K.: Hamiltonian approach to nonlinear travelling whistler waves. In: The Physics of collisionless shocks, p. 141 (Eds. Li, G.; Zank, G.; Russell, C. T.). ANY PUBLISHER, Palm Springs, USA (2005)
How does our star heat its outer atmosphere, the solar corona, to unimaginable temperatures of up to 10 million degrees Celsius? With unprecedented observational data from ESA's Solar Orbiter spacecraft and powerful computer simulations, ERC starting grant awardee Pradeep Chitta intends to bring new momentum to the search for the coronal heating mechanism.
The research group “Solar Lower Atmosphere and Magnetism” (SLAM) studies the conditions and dynamic processes in the atmospheric layer between the solar surface (photosphere) and the overlying chromosphere, an approximately 2000 km thick gas layer.
The main research fields of the department "Sun and Heliosphere" are covered by the research groups "Solar and Stellar Coronae", "Solar Lower Atmosphere and Magnetism", "Solar and Stellar Magnetohydrodynamics" and "Solar Variability and Climate".