Dasi-Espuig, M.; Jiang, J.; Krivova, N. A.; Solanki, S. K.; Unruh, Y. C.; Yeo, K. L.: Reconstruction of spectral solar irradiance since 1700 from simulated magnetograms. Astronomy and Astrophysics 590, A63 (2016)
Dasi-Espuig, M.; Jiang, J.; Krivova, N. A.; Solanki, S. K.: Modelling total solar irradiance since 1878 from simulated magnetograms. Astronomy and Astrophysics 570, A23 (2014)
Muñoz-Jaramillo, A.; Dasi-Espuig, M.; Balmaceda, L. A.; DeLuca, E. E.: Solar Cycle Propagation, Memory, and Prediction: Insights from a Century of Magnetic Proxies. Astrophysical Journal 767 (2), L25 (2013)
Barrena, R.; Girardi, M.; Boschin, W.; Dasi, M.: Internal dynamics of Abell 1240: a galaxy cluster with symmetric double radio relics. Astronomy and Astrophysics 503 (2), pp. 357 - 371 (2009)
Espuig, M. D.; Jiang, J.; Krivova, N. A.; Solanki, S. K.: Total solar irradiance reconstruction since 1700 using a flux transport model. 40th COSPAR Scientific Assembly, Moscow, Russia (2014)
Espuig, M. D.: Solar variability: A new proxy and models of solar irradiance variations. Dissertation, Techn. Univ. Carolo-Wilhelmina, Braunschweig (2011)
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).
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.