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)
Images from ESA’s Solar Orbiter offer the best look yet at a source region of the solar wind - and challenge our view of the continuous particle stream from the Sun.
Deciphering the magnetic origins of the Sun's hot corona: developing a framework for coronal heating by probing the elusive photosphere-corona connection
Using unique observational data and computer simulations, the MPS scientist is striving to understand the incredibly hot temperatures in the solar corona.
For the first time, images of the Sun have been taken from a distance of only 77 million kilometres enabling a completely new view of our star possible.
In his doctoral thesis, Sudip Mandal investigated how special pressure waves help maintain temperatures of several million degrees in the outermost solar atmosphere.