Axford, W. I.; McKenzie, J. F.: Implications of observations of the solar wind and corona for solar wind models. Astrophysics and Space Science 243, pp. 1 - 3 (1996)
Daglis, I. A.; Axford, W. I.: Fast ionospheric response to enhanced activity in geospace: Ion feeding of the inner magnetotail. Journal Geophysical Research 101, pp. 5047 - 5065 (1996)
Daglis, I. A.; Axford, W. I.; Livi, S.; Wilken, B.; Grande, M.; Søraas, F.: Auroral ionospheric ion feeding of the inner plasma sheet during substorms. J. Geomag. Geoelectr. 48, pp. 729 - 739 (1996)
Hovestadt, D.; Hilchenbach, M.; Bürgi, A.; Klecker, B.; Laeverenz, P.; Scholer, M.; Grünwaldt, H.; Axford, W. I.; Livi, S.; Marsch, E.et al.; Wilken, B.; Winterhoff, H. P.; Ipavich, F. M.; Bedini, P.; Coplan, M. A.; Galvin, A. B.; Gloeckler, G.; Bochsler, P.; Balsiger, H.; Fischer, J.; Geiss, J.; Kallenbach, R.; Wurz, P.; Reiche, K.-U.; Gliem, F.; Judge, D. L.; Ogawa, H. S.; Hsieh, K. C.; Möbius, E.; Lee, M. A.; Managadze, G. G.; Verigin, M. I.; Neugebauer, M.: CELIAS-Charge, element and isotope analysis system for SOHO. Solar Physics 162, pp. 441 - 481 (1995)
Nielsen, E.; Axford, W. I.; Hagfors, T.; Kopka, H.; Armand, N. A.; Andrianov, V. A.; Shtern, D. J.; Breus, T.: The ``Long Wavelength Radar'' on the Mars-94 Orbiter. Advances in Space Research 15, pp. (4)163 - (4)178 (1995)
Ratkiewicz, R.; Axford, W. I.; McKenzie, J. F.: Similarity solutions for synchrotron emission from a supernova blast wave. Astronomy and Astrophysics 291, pp. 935 - 942 (1994)
Dougherty, M. K.; Krymskii, A. M.; Breus, T. K.; Southwood, D. J.; Axford, W. I.: The electromagnetic effects of the solar wind interaction with Phobos. Advances in Space Research 13, pp. (10)295 - (10)298 (1993)
Krymskii, A. M.; Breus, T. K.; Dougherty, M. K.; Southwood, D. J.; Axford, W. I.: The electromagnetic effects of the solar wind interaction with the Phobos neutral gas halo and dust torus. Planetary and Space Science 40, pp. 1033 - 1041 (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)
The Uranian magnetic field is more expansive than previously thought, according to newly analyzed data from Voyager 2, making it easier to search for moons with oceans.