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)
Analyzing the high spatial resolution solar Ca II H and K emission data obtained by the SUNRISE mission and building a model of other stars more active than the Sun
The Planetary Plasma Environments group (PPE) has a strong heritage in the exploration of planetary magnetospheres and space plasma interactions throughout the solar system. It has contributed instruments to several past missions that flew-by or orbited Jupiter (Galileo, Cassini, Ulysses). The PPE participates in the JUICE mission by contributing hardware and scientific expertise to the Particle Environment Package (PEP).
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.