McKenzie, J. F.; Sukhorukova, G. V.; Axford, W. I.: Structure of a photoionization layer in the solar chromosphere. Astronomy and Astrophysics 332, pp. 367 - 373 (1998)
Pokhotelov, O. A.; Khruschev, V. V.; Shukla, P. K.; Stenflo, L.; McKenzie, J. F.: Nonlinearly coupled Rossby-type and inertio-gravity waves in self-gravitating systems. Physica Scripta 58, pp. 618 - 621 (1998)
Czechowski, A.; Ratkiewicz, R.; McKenzie, J. F.; Axford, W. I.: Generalized sonic points and acceleration of multi-ion solar wind. Advances in Space Research 20, pp. 43 - 46 (1997)
Lieu, R.; Axford, W. I.; McKenzie, J. F.: Radiation by charged particles in nonuniform acceleration: The inapplicability of Larmor's formula. Physical Review E 55, pp. 1872 - 1875 (1997)
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)
Geiss, J.; Gloeckler, G.; von Steiger, R.; Balsiger, H.; Fisk, L. A.; Galvin, A. B.; Ipavich, F. M.; Livi, S.; McKenzie, J. F.; Ogilvie, K. W.et al.; Wilken, B.: The southern high-speed stream: Results from the SWICS instrument on Ulysses. Science 268, pp. 1033 - 1036 (1995)
Guglielmi, A. V.; Pokhotelov, O. A.; Feygin, F. Z.; Kurchashov, Y. P.; McKenzie, J. F.; Shukla, P. K.; Stenflo, L.; Potapov, A. S.: Ponderomotive wave forces in longitudinal MHD waveguides. Journal Geophysical Research 100, pp. 7997 - 8002 (1995)
Pokhotelov, O. A.; McKenzie, J. F.; Shukla, P. K.; Stenflo, L.: Nonlinearly coupled inertial and Rossby waves. Physics of Fluids 7, pp. 1785 - 1787 (1995)
Woodward, T.; McKenzie, J. F.: MHD Hall current wave pattern generated by conducting obstacles in a flowing plasma. Advances in Space Research 16, pp. 95 - 98 (1995)
McKenzie, J. F.: Comment on ``Solar wind from a corona with a large helium abundance'' by E. Leer, T. E. Holzer and E. C. Shoub. Journal Geophysical Research 99 (A2), pp. 2585 - 2586 (1994)
McKenzie, J. F.: Interaction between Alfvèn waves and a multicomponent plasma with differential ion streaming. Journal Geophysical Research 99 (A3), pp. 4193 - 4200 (1994)
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)
Analyzing the high spatial resolution solar Ca II H and K emission data obtained by the SUNRISE mission and building a model of other stars more active than the Sun
The Planetary Plasma Environments group (PPE) has a strong heritage in the exploration of planetary magnetospheres and space plasma interactions throughout the solar system. It has contributed instruments to several past missions that flew-by or orbited Jupiter (Galileo, Cassini, Ulysses). The PPE participates in the JUICE mission by contributing hardware and scientific expertise to the Particle Environment Package (PEP).
First Light for Sunrise III: the first tests with real sunlight were successful. The balloon-borne solar observatory should be ready for launch at the end of May.