This project aims to understand the key physical laws and processes underlying a range of basic phenomena observed in the solar atmosphere. We will study the emergence of magnetized plasma from the solar interior, the propagation of waves and shocks in the atmosphere, and the stability of structures (prominences, photospheric magnetic flux tubes)

In the last two decades, Spain has built up strong IR and X-ray communities which have successfully contributed, at Co-I level, to the construction and to the scientific exploitation of basically all European InfraRed (IR) space instruments and to the participation in X-ray missions, including Athena. The IAC has contributed to the construction of

This subproject aims to contribute with for scientific and technical work for the IACs contributions to the PLATO 2.0 mission is requested. This includes engineering work during the B2 phase, to be completed in July 2017 with the PDR, and during phase C, to finish in 2018 with the CDR, in addition to acquisitions of LLI (Long Lead Items) during

Grants for Short Stay of Predoctoral Researcher in a different center from the one in which the Thesis is developed. Alejandro Lumbreras Calle

This project aims at integrating the major European infrastructures in the field of high-resolution solar physics. The following actions will be taken: (i) realise transnational access to all European users (ii) integrate small communities and foster European collaboration (iii) enhance and spread data acquisition and processing expertise to the

Ramón y Cajal contract to develop its research work in the specific research project "Baryons and dark matter on the smallest galactic scales"