Green, L. M.; Thalmann, J. K.; Valori, G.; Pariat, E.; Linan, L.; Moraitis, K.: Magnetic Helicity Evolution and Eruptive Activity in NOAA Active Region 11158. The Astrophysical Journal 937, p. 59 (2022)
Valori, G.; Löschl, P.; Stansby, D.; Pariat, E.; Hirzberger, J.; Chen, F.: Disambiguation of Vector Magnetograms by Stereoscopic Observations from the Solar Orbiter (SO)/Polarimetric and Helioseismic Imager (PHI) and the Solar Dynamic Observatory (SDO)/Helioseismic and Magnetic Imager (HMI). Solar Physics 297, p. 12 (2022)
Baker, D.; Mihailescu, T.; Démoulin, P.; Green, L. M.; van Driel-Gesztelyi, L.; Valori, G.; Brooks, D. H.; Long, D. M.; Janvier, M.: Plasma Upflows Induced by Magnetic Reconnection Above an Eruptive Flux Rope. Solar Physics 296, p. 103 (2021)
Long, D.M.; Reid, H.A.S.; Valori, G.; O'Kane, J.: Localized acceleration of energetic particles by a weak shock in the solar corona. The Astrophysical Journal 921 (1), 61 (2021)
Murabito, M.; Stangalini, M.; Baker, D.; Valori, G.; Jess, D. B.; Jafarzadeh, S.; Brooks, D. H.; Ermolli, I.; Giorgi, F.; Grant, S. D. T.et al.; Long, D. M.; van Driel-Gesztelyi, L.: Investigating the origin of magnetic perturbations associated with the FIP Effect. Astronomy and Astrophysics 656, A87 (2021)
Thalmann, J.K.; Georgoulis, M.K.; Liu, Y.; Pariat, E.; Valori, G.; Anfinogentov, S.; Chen, F.; Guo, Y.; Moraitis, K.; Yang, S.et al.; Mastrano, A.: Magnetic Helicity Estimations in Models and Observations of the Solar Magnetic Field. IV. Application to Solar Observations. The Astrophysical Journal 922 (1), 41 (2021)
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, ...