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Grigorenko, E. E.; Malova, H. V.; Artemyev, A. V.; Mingalev, O. V.; Kronberg, E. A.; Koleva, R.; Daly, P. W.; Cao, J. B.; Sauvaud, J.-A.; Owen, C. J.et al.; Zelenyi, L. M.: Current sheet structure and kinetic properties of plasma flows during a near-Earth magnetic reconnection under the presence of a guide field. Journal Geophysical Research 118, pp. 3265 - 3287 (2013)
Kasahara, S.; Kronberg, E. A.; Kimura, T.; Tao, C.; Badman, S. V.; Masters, A.; Retinò, A.; Krupp, N.; Fujimoto, M.: Asymmetric distribution of reconnection jet fronts in the Jovian nightside magnetosphere. Journal Geophysical Research 118, pp. 375 - 384 (2013)
Kronberg, E. A.; Daly, P. W.: Spectral analysis for wide energy channels. Geoscientific Instrumentation Methods and Data Systems 2, pp. 257 - 261 (2013)
Li, K.; Haaland, S.; Eriksson, A.; André, M.; Engwall, E.; Wei, Y.; Kronberg, E. A.; Fränz, M.; Daly, P. W.; Zhao, H.et al.; Ren, Q. Y.: Transport of cold ions from the polar ionosphere to the plasma sheet. Journal Geophysical Research 118, pp. 5467 - 5477 (2013)
Nakamura, R.; Baumjohann, W.; Panov, E.; Volwerk, M.; Birn, J.; Artemyev, A.; Petrukovich, A. A.; Amm, O.; Juusola, L.; Kubyshkina, M. V.et al.; Apatenkov, S.; Kronberg, E. A.; Daly, P. W.; Fillingim, M.; Weygand, J. M.; Fazakerley, A.; Khotyaintsev, Y.: Flow bouncing and electron injection observed by Cluster. Journal Geophysical Research 118, pp. 2055 - 2072 (2013)
Rymer, A. M.; Mitchell, D. G.; Hill, T. W.; Kronberg, E. A.; Krupp, N.; Jackman, C. M.: Saturn's magnetospheric refresh rate. Geophysical Research Letters 40, pp. 2479 - 2483 (2013)
Wang, R.; Du, A.; Nakamura, R.; Lu, Q.; Khotyaintsev, Y. V.; Volwerk, M.; Zhang, T.; Kronberg, E. A.; Daly, P. W.; Fazakerley, A. N.: Observation of multiple sub-cavities adjacent to single separatrix. Geophysical Research Letters 40, pp. 2511 - 2517 (2013)
Fu, H.; Khotyaintsev, Y. V.; Vaivads, A.; Andre, M.; Sergeev, V. A.; Huang, S. Y.; Kronberg, E. A.; Daly, P. W.: Pitch angle distribution of suprathermal electrons behind dipolarization fronts: A statistical overview. Journal Geophysical Research 117, A12221 (2012)
Kronberg, E.; Haaland, S.; Daly, P.; Grigorenko, E.; Kistler, L.; Fränz, M.; Dandouras, I.: Oxygen and hydrogen ion abundance in the near-Earth magnetosphere: Statistical results on the response to the geomagnetic and solar wind activity conditions. Journal Geophysical Research 117, A12208 (2012)
Nykyri, K.; Otto, A.; Adamson, E.; Kronberg, E.; Daly, P.: On the origin of high-energy particles in the cusp diamagnetic cavity. Journal of Atmospheric and Solar-Terrestrial Physics 87-88, pp. 70 - 81 (2012)
Teh, W.-L.; Nakamura, R.; Fujimoto, M.; Kronberg, E. A.; Fazakerley, A. N.; Daly, P. W.; Baumjohann, W.: Electron dynamics in the reconnection ion diffusion region. Journal Geophysical Research 117, A12225 (2012)
Walsh, B. M.; Haaland, S. E.; Daly, P. W.; Kronberg, E. A.; Fritz, T. A.: Energetic electrons along the high-latitude magnetopause. Annales Geophysicae 30, pp. 1003 - 1013 (2012)
Kronberg, E. A.; Bučík, R.; Haaland, S.; Klecker, B.; Keika, K.; Desai, M. I.; Daly, P. W.; Yamauchi, M.; Gómez-Herrero, R.; Lui, A. T. Y.: On the origin of the energetic ion events measured upstream the Earth's bow shock by STEREO, Cluster and Geotail. Journal Geophysical Research 116, A02210 (2011)
Trattner, K. J.; Petrinec, S. M.; Fuselier, S. A.; Nykyri, K.; Kronberg, E.: Cluster observations of bow shock energetic ion transport through the magnetosheath into the cusp. Journal Geophysical Research 116, A09207 (2011)
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.