Michels, D. J.; Schwenn, R.; Howard, R. A.; Bartoe, J.-D. F.; Antiochos, S. K.; Brueckner, G. E.; Cheng, C.-C.; Dere, K. P.; Doschek, G. A.; Mariska, J. T.et al.; Sheeley Jr., N. R.; Socker, D. G.; Daly, P. W.; Inhester, B.; Keller, H.-U.; Kramm, J. R.; Rosenbauer, H.; Lamy, P.; Llebaria, A.; Maucherat, A.; Parker, E. N.; Kahler, S. W.; Koutchmy, S. L.; Smartt, R. N.; Wagner, W. J.; Bougeret, J.-L.; Pick, M.; Noens, J.-C.; Giese, R. H.; Koomen, M. J.; Giovane, F.; Misconi, N. Y.; Simnett, G. M.; Eyles, C.; Bedford, D.; Priest, E.; Lallement, R.: 'LASCO' - A wide-field white light and spectrometric coronagraph for SOHO. In: The SOHO Mission, pp. 55 - 61. ESA Publications Division, ESTEC, Noordwijk, Holland (1989)
Kronberg, E. A.; Ilie, R.; Smirnov, A.; Gastaldello, F.; Haaland, S.; Berrendorf, M.; Huang, Y.; Daly, P. W.; Ghizzardi, S.; Allen, R. C.: Prediction of soft protons in the near-Earth space using machine learning. ISSI team on “Soft protons in the magnetosphere focused by X-ray telescopes”, Bern, Switzerland (2019)
Grigorenko, E. E.; Malykhin, A. Y.; Kronberg, E. A.; Daly, P. W.: Electron and ion acceleration during dipolarizations in the near-Earth magnetotail: RAPID observations. 29th Cluster workshop, Lanzarote, Canary Islands, Spain (2019)
Kronberg, E. A.; Smirnov, A. G.; Latallerie, F.; Daly, P. W.; Aseev, N.; Shprits, Y. Y.; Kellerman, A.; Kasahara, S.; Turner, D.; Taylor, M. G. G. T.: Evolution of energetic electron intensities in the radiation belts measured by Cluster/RAPID during 1.5 solar cycles. 29th Cluster workshop, Lanzarote, Canary Islands, Spain (2019)
Kronberg, E. A.; Grigorenko, E.; Kozak, L.; Gorman, J.; Malykhin, A.; Petrenko, B.; Smirnov, A.; Daly, P. W.; Malova, H.: Energy transformation, turbulence and acceleration in space plasmas: why it is cool to be together? VWS Symposium, Dresden, Germany (2019)
Daly, P. W.; Haaland, S.; Vilenius, E.: The RAPID Direct Events product: what it is and how to use it. 24th Cluster Cross-Calibration Workshop, Maspalomas, Gran Canaria, Spain (2018)
Smirnov, A.; Kronberg, E. A.; Daly, P. W.: Electron intensity measurements in the radiation belts. 24th Cluster Cross-Calibration Workshop, Maspalomas, Gran Canaria, Spain (2018)
Kronberg, E. A.; Luo, H.; Nykyri, K.; Trattner, K. J.; Daly, P. W.; Grigorenko, E.: The energetic particle properties in the magnetosphere: results based on statistics from Cluster/RAPID observations. 5th Cluster-Themis Workshop, Chania, Greece (2018)
Kronberg, E. A.; Grigorenko, E.; Turner, D.; Daly, P. W.; Khotyaintsev, Y.; Kozak, L.: Comparing and contrasting dispersionless injections at geosynchronous orbit during a substorm event. COSPAR 2018, Pasadena, CA, USA (2018)
Kronberg, E. A.; Rashev, M.; Daly, P. W.; Shprits, Y.; Turner, D.; Drozdov, A.; Dobynde, M.; Kellerman, A.; Fritz, T. A.; Pierrard, V.et al.; Borremans, K.; Klecker, B.; Friedel, R.; Smirnov, A.; Aseev, N.: The Cluster II mission, recent observations and instrument calibrations. COSPAR 2018, Pasadena, CA, USA (2018)
Kronberg, E. A.; Welling, D.; Kistler, L.; Mouikis, C.; Daly, P. W.; Grigorenko, E.; Klecker, B.; Dandouras, I.: Evaluation of the plasma pressure during the magnetic storm. European Geosciences Union (EGU) General Assembly 2018, Vienna, Austria (2018)
Kronberg, E. A.; Welling, D.; Kistler, L.; Mouikis, C.; Daly, P. W.; Grigorenko, E.; Klecker, B.; Dandouras, a. I.: Constribution of energetic and heavy ions to the plasma pressure in the magnetotail and the ring current. COSPAR 2018, Pasadena, CA, USA (2018)
Haaland, S.; Kronberg, E. A.; Daly, P. W.; Vilenius, E.: Energetic Particles in Geospace: Characteristics, Sources and Impact Seminar. Istituto di Astrofisica Spaziale e Fisica Cosmica, Milano, Italy (2018)
Kronberg, E. A.; Grigorenko, E. E.; Turner, D. L.; Daly, P. W.; Khotyaintsev, Y.; Kozak, L.: Electron acceleration by ULF waves associated with dispersionless injections during a substorm event. IAGA, Cape Town, South Africa (2017)
The main research fields of the department "Sun and Heliosphere" are covered by the research groups "Solar and Stellar Coronae", "Solar Lower Atmosphere and Magnetism", "Solar and Stellar Magnetohydrodynamics" and "Solar Variability and Climate".
How does our star heat its outer atmosphere, the solar corona, to unimaginable temperatures of up to 10 million degrees Celsius? With unprecedented observational data from ESA's Solar Orbiter spacecraft and powerful computer simulations, ERC starting grant awardee Pradeep Chitta intends to bring new momentum to the search for the coronal heating mechanism.
The research group “Solar Lower Atmosphere and Magnetism” (SLAM) studies the conditions and dynamic processes in the atmospheric layer between the solar surface (photosphere) and the overlying chromosphere, an approximately 2000 km thick gas layer.