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McKenzie, J. F.; Sauer, K.; Dubinin, E.: Stationary waves in a bi-ion plasma transverse to the magnetic field. Journal of Plasma Physics 65, pp. 197 - 212 (2001)
Sauer, K.; Dubinin, E.; McKenzie, J. F.: New type of soliton in bi-ion plasmas and possible implications. Geophysical Research Letters 28, pp. 3589 - 3592 (2001)
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)
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)
Woodward, T. I.; McKenzie, J. F.: Stationary incompressible MHD perturbations generated by a current source in a moving plasma. Planetary and Space Science 47, pp. 545 - 555 (1999)
Czechowski, A.; Ratkiewicz, R.; McKenzie, J. F.; Axford, W. I.: Heating and acceleration of minor ions in the solar wind. Astronomy and Astrophysics 335, pp. 303 - 308 (1998)
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.