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)
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.