Yang, D.; Gizon, L.; Barucq, H.: Imaging individual active regions on the Sun's far side with improved helioseismic holography. Astronomy and Astrophysics 669, p. A89 (2023)
Yang, D.; Gizon, L.; Barucq, H.: Imaging individual active regions on the Sun's far side with improved helioseismic holography. Astronomy and Astrophysics 669, p. A89 (2023)
Heinemann, S. G.; Temmer, M.; Hofmeister, S. J.; Stojakovic, A.; Gizon, L.; Yang, D.: How to Estimate the Far-Side Open Flux Using STEREO Coronal Holes. Solar Physics 296, 141 (2021)
Yang, D.; Gizon, L.; Fournier, D.; Lindsey, C.: Improved helioseismic imaging of the farside. Dynamics of the Sun and Stars: Honoring the Life and Work of Michael J. Thompson,, Boulder, USA (2019)
Yang, D.; Gizon, L.; Fournier, D.: A Possible Improvement on Helioseismic Holography. the many Scales of the Universe: Galaxies, their Suns, and their Planets - Annual Meeting of the Astronomische Gesellschaft 2017, Göttingen, Germany (2017)
First icy cold, then midnight sun: at the Arctic Circle, the team will prepare the next flight of the balloon-borne solar observatory - and hopes for solar fireworks.
Astronomical teamwork: By combining data from Solar Orbiter and SDO, a group of researchers has unambiguously determined the magnetic field at the solar surface.
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.