Wiedenbeck, M. E.; Bučík, R.; Mason, G. M.; Ho, G. C.; Leske, R. A.; Cohen, C. M. S.; Christian, E. R.; Cummings, A. C.; Davis, A. J.; Desai, M. I.et al.; Giacalone, J.; Haggerty, D. K.; Hill, M. E.; Joyce, C. J.; Labrador, A. W.; Malandraki, O.; Matthaeus, W. H.; McComas, D. J.; Jr., R. L. M.; Mewaldt, R. A.; Mitchell, D. G.; Posner, A.; Rankin, J. S.; Roelof, E. C.; Schwadron, N. A.; Stone, E. C.; Szalay, J. R.; Bale, S. D.; Case, A. W.; Kasper, J. C.; Korreck, K. E.; Larson, D. E.; MacDowall, R. J.; Pulupa, M.; Stevens, M. L.: 3He-rich Solar Energetic Particle Observations at the Parker Solar Probe and near Earth. The Astrophysical Journal Supplement Series 246 (2), 42 (2020)
Bučík, R.; Innes, D.; Mason, G. M.; Wiedenbeck, M. E.; Gómez-Herrero, R.; Nitta, N. V.: 3He-rich Solar Energetic Particles in Helical Jets on the Sun. The Astrophysical Journal 852, 76 (2018)
Bučík, R.; Wiedenbeck, M. E.; Mason, G. M.; Gómez-Herrero, R.; Nitta, N. V.; Wang, L.: 3He-rich Solar Energetic Particles from Sunspot Jets. The Astrophysical Journal Letters 869 (1), L21 (2018)
Roussos, E.; Jackman, C.; Thomsen, M. F.; Kurth, W. S.; Badman, S. V.; Paranicas, C.; Kollmann, P.; Krupp, N.; Bučík, R.; Mitchell, D. G.et al.; Krimigis, S. M.; Hamilton, D. C.; Radioti, A.: Solar Energetic Particles (SEP) and Galactic Cosmic Rays (GCR) as tracers of solar wind conditions near Saturn: Event lists and applications. Icarus 300, pp. 47 - 71 (2018)
Bučík, R.; Innes, D. E.; Mason, G. M.; Wiedenbeck, M. E.: Energy spectra of 3He-rich solar energetic particles associated with coronal waves. J. Phys.: Conf. Ser. 767, 012002 (2016)
Bučík, R.; Innes, D. E.; Mason, G. M.; Wiedenbeck, M. E.: Association of 3He-rich solar energetic particles with large-scale coronal waves. Astrophysical Journal 833, 63 (2016)
Innes, D. E.; Bučík, R.; Guo, L.-J.; Nitta, N.: Observations of solar X-ray and EUV jets and their related phenomena. Astron. Nachrichten 337, pp. 1024 - 1032 (2016)
Bučík, R.; Innes, D. E.; Chen, N.-H.; Mason, G. M.; Gomez-Herrero, R.; Wiedenbeck, M. E.: Long-lived energetic particle source regions on the Sun. Journal of Physics: Conference Series 642, 012002 (2015)
Bučík, R.; Innes, D. E.; Guo, L.; Mason, G. M.; Wiedenbeck, M. E.: Observations of EUV waves in 3He-rich solar energetic particle events. Astrophysical Journal 812 (1), 53 (2015)
Chen, N.-H.; Bučík, R.; Innes, D. E.; Mason, G. M.: Case studies of multi-day 3He-rich solar energetic particle periods. Astronomy and Astrophysics 580, A16 (2015)
Park, J.; Innes, D. E.; Bučík, R.; Moon, Y.-J.; Kahler, S. W.: Study of solar energetic particle associations with coronal extreme-ultraviolet waves. Astrophysical Journal 808 (1), 3 (2015)
Bučík, R.; Innes, D. E.; Mall, U.; Korth, A.; Mason, G. M.; Gomez-Herrero, R.: Multi-spacecraft observations of recurrent 3He-rich solar energetic particles. Astrophysical Journal 786 (1), 71 (2014)
Opitz, A.; Sauvaud, J.‐.; Klassen, A.; Gomez‐Herrero, R.; Bučík, R.; Kistler, L. M.; Jacquey, C.; Luhmann, J.; Mason, G.; Kajdic, P.et al.; Lavraud, B.: Solar wind control of the terrestrial magnetotail as seen by STEREO. Journal Geophysical Research 119, pp. 6342 - 6355 (2014)
Bučík, R.; Mall, U.; Korth, A.; Mason, G. M.: Abundances of suprathermal heavy ions in CIRs during the minimum of solar cycle 23. Solar Physics 281, pp. 411 - 422 (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)
First Light! The spectro-polarimeter of the world's largest solar telescope in Hawaii looks at the Sun for the first time. The instrument was developed in Germany.
Dr. Theodosios Chatzistergos receives award by the European Space Weather and Space Climate Association for his research findings on the historical activity of the Sun.
The Zdenĕk Švetska Senior Prize of the Solar Physics Division of the European Physical Society (EPS) recognizes Solanki’s pioneering contributions to solar research.
The magnetic field in the solar atmosphere exceeds the geomagnetic field strength by four orders of magnitude. It greatly influences the processes of energy transport within the solar atmosphere, and dominates the morphology of the solar chromosphere and corona. Kinetic energy from convective motions in the Sun can be efficiently stored in magnetic fields and subsequently released - to heat the solar corona to several million degrees or to blast off coronal mass ejections.
Application deadline 1 October 2024. PhD projects in planetary science, solar and stellar physics, solar magnetism, heliophysics, helioseismology, asteroseismology, ...