Vilenius, E.; Daly, P.; Kronberg, E.: Analysis of RAPID electron fluxes after corrections for the long-term detector decay. 23th Cluster Cross-Calibration Meeting, Mallorca, Spain (2017)
Grigorenko, E. E.; Zelenyi, L. M.; Dolgonosov, M. S.; Kronberg, E. A.; Daly, P. W.: CLUSTER view on PSBL ion beams in the Earth's magnetotail. 4th Cluster-THEMIS workshop, Palm Springs, USA (2016)
Kronberg, E.; Gilder, S.; Luo, H.; Daly, P.; Grigorenko, E.: Signature of solar wind turbulence in the ground magnetic field and its relation to ion acceleration. European Geosciences Union General Assembly, Vienna, Austria (2016)
Kronberg, E.; Grigorenko, E. E.; Daly, P. W.; Luo, H.; Khotyaintsev, Y.: Characterization of energetic O+ and H+ ions in the plasma sheet. 4th Cluster-THEMIS workshop, Palm Springs, USA (2016)
Kronberg, E.; Gilder, S.; Luo, H.; Daly, P. W.; Grigorenko, E.: Control of oxygen ion acceleration by turbulence. Cluster 15th and Double Star 10th anniversary workshop, Venice, Italy (2015)
Li, K.; Haaland, S.; Daly, P. W.; Kronberg, E. A.; André, M.; Eriksson, A.; Lybekk, B.; Pedersen, A.: On the dayside high altitude stagnant region of cold ion outflow. Cluster 15th and Double Star 10th anniversary workshop, Venice, Italy (2015)
Daly, P. W.: Long-term analysis of cosmic ray background seen by the RAPID electron detector on Cluster. Geospace Revisited: a Cluster/MAARBLE/Van Allen Probes Conference, Rhodes, Greece (2014)
Daly, P. W.: Status report of the RAPID instrument on board Cluster. Geospace Revisited: a Cluster/MAARBLE/Van Allen Probes Conference, Rhodes, Greece (2014)
Vilenius, E.; Daly, P. W.; Kronberg, E. A.: Calibration of RAPID/IES 3D electron data: detector-to-detector corrections and long-term degradation. 29th Cluster workshop, Lanzarote, Canary Islands, Spain (2019)
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. Machine Learning in Heliophysics, Amsterdam, Netherlands (2019)
Parkhomenko, E.; Malova, H.; Popov, V.; Grigorenko, E.; Delcourt, D.; Daly, P. W.; Kronberg, E. A.; Petrukovich, A.; Zelenyi, L.: Acceleration of plasma in current sheet during substorm dipolarizations in the Earth’s magnetotail: comparison of different mechanisms. EGU General Assembly, Vienna, Austria (2019)
Smirnov, A.; Kronberg, E. A.; Latallerie, F.; Daly, P. W.; Aseev, N.; Shprits, Y.; Kellerman, A.; Kasahara, S.; Turner, D.; Taylor, M.: Electron Intensity Measurements by Cluster Mission in Radiation Belts of the Earth. EGU General Assembly, Vienna, Austria (2019)
Vilenius, E.; Daly, P. W.; Kronberg, E. A.: Update on the long-term calibration of RAPID/IES 3D electron data. 5th Cluster-Themis Workshop, Chania, Greece (2018)
Malykhin, A.; Grigorenko, E.; Kronberg, E. A.; Koleva, R.; Ganushkina, N.; Kozak, L.; Daly, P. W.: Dynamics of suprathermal electron and proton fluxes during magnetotail dipolarization associated with magnetic flux pile up in the near-Earth plasma sheet. European Geosciences Union (EGU) General Assembly 2018, Vienna, Austria (2018)
Parkhomenko, E.; Malova, H.; Grigorenko, E.; Popov, V.; Petrukovich, A.; Delcourt, D.; Kronberg, E. A.; Daly, P. W.; Zelenyi, L.: Plasma acceleration on multiscale temporal variations of electric and magnetic fields during substorm dipolarization in the Earth’s magnetotail. European Geosciences Union (EGU) General Assembly 2018, Vienna, Austria (2018)
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.