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)
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
First Light for Sunrise III: the first tests with real sunlight were successful. The balloon-borne solar observatory should be ready for launch at the end of May.
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.
Images from ESA’s Solar Orbiter offer the best look yet at a source region of the solar wind - and challenge our view of the continuous particle stream from the Sun.