The Sun, our star, is not only the source of the electromagnetic radiation that bathes our planet; it also sweeps the Earth's magnetosphere with its wind and...
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GrantThe physics of the Solar Atmosphere: theory, radiation diagnostics and supercomputing
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GrantThe reionization of the universe
The Universe's re-ionisation is at the forefront of research. How the re-ionisation occurred is however still not known. This project intents to understand the...
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GrantThe role of starbursts in formation and evolution of galaxies: ESTALLIDOS 5.
Starsbursts play a key role in the cosmic evolution of galaxies. There is an intimate link between the average star formation (SF) rate history of the universe...
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GrantThe structure and evolution of galaxies and their central regions
We propose to study the evolution of galaxies through detailed analysis of observational data obtained with the most modern ground- and space-based telescopes...
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GrantThe structure and evolution of galaxies and their outskirts
We propose to study the evolution of galaxies through detailed analysis of observational data obtained with the most modern ground- and space-based telescopes...
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GrantThe structure and evolution of the galaxies and their central regions
We propose to study the evolution of galaxies through detailed analysis of images and spectra obtained with the most modern ground- and space-based telescopes...
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GrantThe three-dimensional Magnetic Structure of solar Filaments and Prominenses
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GrantThe whole sun project: untangling the complex physical mechanisms behind our eruptive star and its twins: "Whole sun"
The Sun is a magnetically active star with violent eruptions that can hit Earth´s magnetosphere and cause important perturbations in our technology-dependent...
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GrantThick discs, relics of the infancy of galaxies
Galaxy discs are made of two components, the thin and the thick disc. Thick discs contain up to 50% of the baryonic mass of a galaxy. Because their stars are...